ads_id stringlengths 4 8 | arxiv_id stringlengths 8 25 ⌀ | title stringlengths 3 340 | abstract stringlengths 1 9.28k | embed listlengths 1.54k 1.54k | umap_x float64 -5.05 18.9 | umap_y float64 -3.35 17.3 | date date32 | cites int64 0 15.7k | bibcode stringlengths 19 19 | keywords listlengths 0 20 | ads_keywords listlengths 1 58 ⌀ | read_count int64 0 645 | doi listlengths 1 3 | authors listlengths 1 2.31k ⌀ | aff listlengths 1 2.31k ⌀ | cite_bibcodes listlengths 1 15.7k ⌀ | ref_bibcodes listlengths 1 1.98k ⌀ |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
12465084 | 1607.03394 | Scalar and vector perturbations in a universe with discrete and continuous matter sources | We study a universe filled with dust-like matter in the form of discrete inhomogeneities (e.g., galaxies and their groups and clusters) and two sets of perfect fluids with linear and nonlinear equations of state, respectively. The background spacetime geometry is defined by the FLRW metric. In the weak gravitational fi... | [
-0.0018089126097038388,
0.040593914687633514,
-0.019252516329288483,
-0.004424365237355232,
-0.01197624858468771,
-0.03831935301423073,
0.014146363362669945,
0.01088538859039545,
-0.04971535876393318,
0.04595537483692169,
-0.014715003781020641,
0.0026734769344329834,
-0.027689272537827492,
... | 10.708581 | 0.528248 | 2016-07-01 | 24 | 2016JCAP...09..032E | [
"energy density fluctuations",
"individual contributions",
"cosmological models",
"super-horizon ones",
"numerical simulations",
"discrete inhomogeneities",
"linear",
"perfect fluids",
"linear and nonlinear equations",
"state",
"linear and nonlinear effects",
"the discrete matter sources",
"... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Phenomenology",
"High Energy Physics - Theory"
] | 4 | [
"10.1088/1475-7516/2016/09/032",
"10.48550/arXiv.1607.03394"
] | [
"Eingorn, Maxim",
"Kiefer, Claus",
"Zhuk, Alexander"
] | [
"North Carolina Central University, CREST and NASA Research Centers, Fayetteville st. 1801, Durham, North Carolina 27707, U.S.A. ; Institute for Theoretical Physics, University of Cologne, Zülpicher Strasse 77, 50937 Köln, Germany;",
"Institute for Theoretical Physics, University of Cologne, Zülpicher Strasse 77,... | [
"2017ApJ...845..153B",
"2017IJMPD..2643012E",
"2017IJMPD..2650121E",
"2017JCAP...12..022F",
"2017PDU....17...63E",
"2018EPJC...78..609A",
"2018EPJC...78..637B",
"2018Univ....4..109F",
"2019EPJC...79..655E",
"2019JCAP...10..065D",
"2019PDU....2600329E",
"2020PDU....2900565C",
"2020PhLB..80935... | [
"1980PhRvD..22.1882B",
"1992PhR...215..203M",
"1994csot.book.....V",
"1996CQGra..13.2163Z",
"2001IJMPD..10..213C",
"2001PhLB..511..265K",
"2002GrCo....8..285B",
"2002PhLB..535...17B",
"2002PhRvD..66d3507B",
"2003MNRAS.346..987W",
"2003PhRvL..90i1301L",
"2007PhLB..647...63A",
"2008cmb..book..... |
2774928 | 1607.03488 | Radiative transfer meets Bayesian statistics: where does a galaxy's [C II] emission come from? | The [C II] 158 μm emission line can arise in all phases of the interstellar medium (ISM), therefore being able to disentangle the different contributions is an important yet unresolved problem when undertaking galaxy-wide, integrated [C II] observations. We present a new multiphase 3D radiative transfer interface that ... | [
0.009866549633443356,
0.006452957633882761,
0.010575952008366585,
-0.022896122187376022,
-0.006905283313244581,
0.03199469670653343,
0.03446784242987633,
-0.007406420540064573,
0.012775749899446964,
0.030536841601133347,
0.002246983116492629,
0.0065017701126635075,
-0.0074324537999928,
-0.... | 12.734516 | 8.525039 | 2016-07-01 | 29 | 2017MNRAS.464.3315A | [
"H II region electron number density",
"molecular regions",
"II",
"dust mass fraction",
"cent",
"gas phase metallicity",
"galaxies",
"f_{[C II],mol",
"typical integrated properties",
"ISM",
"f_{[C",
"Universe",
"specific star formation rate",
"SSFR",
"the total integrated [C II] emission... | [
"astrochemistry - ISM: molecules",
"photodissociation region (PDR)",
"ISM: structure",
"infrared: galaxies",
"infrared: ISM",
"Astrophysics - Astrophysics of Galaxies"
] | 7 | [
"10.1093/mnras/stw2580",
"10.48550/arXiv.1607.03488"
] | [
"Accurso, G.",
"Saintonge, A.",
"Bisbas, T. G.",
"Viti, S."
] | [
"Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK",
"Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK",
"Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany; Departmen... | [
"2017ApJ...840...51L",
"2017ApJ...846...32D",
"2017ApJ...846..105O",
"2017MNRAS.470.4750A",
"2018ApJ...869...73L",
"2018MNRAS.481.1976Z",
"2018MNRAS.481.4277F",
"2018NewAR..82....1H",
"2019A&A...626A..23C",
"2020A&A...643A...5D",
"2020A&A...643A...6C",
"2020A&A...643A.141M",
"2020ApJ...899..... | [
"1968IAUS...34..205F",
"1977A&A....55..137D",
"1978ApJS...36..595D",
"1979ApJS...41..555H",
"1980A&A....91...68D",
"1984ApJ...285...89D",
"1988ApJ...334..771V",
"1991ApJ...374..580B",
"1991ApJ...377..192H",
"1994A&AS..105...29F",
"1994ApJ...423..223C",
"1994ApJ...436..720H",
"1996A&A...311..... |
4924940 | 1607.06772 | The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] Line and Dust Emission in 6 | We present a search for [C II] line and dust continuum emission from optical dropout galaxies at z > 6 using ASPECS, our Atacama Large Millimeter submillimeter Array Spectroscopic Survey in the Hubble Ultra-deep Field (UDF). Our observations, which cover the frequency range of 212-272 GHz, encompass approximately th... | [
0.02631862834095955,
0.018085889518260956,
0.01918358914554119,
-0.01713193766772747,
-0.025730576366186142,
0.04973619803786278,
0.0069716926664114,
0.011003120802342892,
-0.014008724130690098,
-0.018138160929083824,
-0.01016024500131607,
-0.03564906865358353,
-0.03402865305542946,
0.0005... | 13.29913 | 7.663112 | 2016-07-01 | 99 | 2016ApJ...833...71A | [
"C II",
"SUB>⊙</SUB",
"SFR relation",
"II",
"line emission",
"spurious sources",
"Array Spectroscopic Survey",
"SFR",
"UDF",
"optical dropout galaxies",
"candidates",
"Atacama Large Millimeter",
"lt",
"±",
"our Atacama Large Millimeter submillimeter Array Spectroscopic Survey",
"z",
... | [
"galaxies: evolution",
"galaxies: high-redshift",
"galaxies: ISM",
"galaxies: star formation",
"instrumentation: interferometers",
"submillimeter: galaxies",
"Astrophysics - Astrophysics of Galaxies"
] | 9 | [
"10.3847/1538-4357/833/1/71",
"10.48550/arXiv.1607.06772"
] | [
"Aravena, M.",
"Decarli, R.",
"Walter, F.",
"Bouwens, R.",
"Oesch, P. A.",
"Carilli, C. L.",
"Bauer, F. E.",
"Da Cunha, E.",
"Daddi, E.",
"Gónzalez-López, J.",
"Ivison, R. J.",
"Riechers, D. A.",
"Smail, I.",
"Swinbank, A. M.",
"Weiss, A.",
"Anguita, T.",
"Bacon, R.",
"Bell, E.",
... | [
"Núcleo de Astronomía, Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile",
"Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany",
"Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany; Astronomy Department, California Ins... | [
"2016ApJ...833...67W",
"2016ApJ...833...68A",
"2016ApJ...833...70D",
"2016ApJ...833...72B",
"2016ApJ...833...73C",
"2016ApJ...833..153S",
"2017A&A...605A..42C",
"2017A&A...608A...1B",
"2017A&A...608A.138G",
"2017ApJ...834...36H",
"2017ApJ...836....8T",
"2017ApJ...845..108Y",
"2017ApJ...847..... | [
"1991ApJ...373..423S",
"1994A&A...288..929K",
"2003AJ....126.1607S",
"2003PASP..115..763C",
"2005A&A...440L..51M",
"2006AJ....132..926C",
"2006AJ....132.1729B",
"2006ApJ...650..592K",
"2008ApJ...686.1503B",
"2008ApJS..178..280B",
"2009MNRAS.396..462K",
"2009Natur.457..699W",
"2010Natur.468..... |
12410081 | 1607.06877 | Exact power series solutions of the structure equations of the general relativistic isotropic fluid stars with linear barotropic and polytropic equations of state | Obtaining exact solutions of the spherically symmetric general relativistic gravitational field equations describing the interior structure of an isotropic fluid sphere is a long standing problem in theoretical and mathematical physics. The usual approach to this problem consists mainly in the numerical investigation o... | [
-0.0124045480042696,
0.026911940425634384,
0.006325312424451113,
-0.03203482925891876,
0.014093535020947456,
-0.0028550592251122,
0.01386982761323452,
-0.011358718387782574,
0.013086853548884392,
-0.03060310333967209,
0.005539542064070702,
0.02908189781010151,
-0.04028961434960365,
-0.0165... | 8.940554 | 3.876266 | 2016-07-01 | 18 | 2016Ap&SS.361..283H | [
"exact series solutions",
"infinite power series",
"exact solutions",
"general relativistic dense astrophysical objects",
"the exact power series solution",
"the power series solutions",
"the relativistic mass equation",
"n=1/5",
"The power series representations",
"a power series representation",... | [
"General relativistic fluid sphere",
"Exact power series solutions",
"Linear barotropic equation of state",
"Polytropic equation of state",
"General Relativity and Quantum Cosmology",
"Astrophysics - Solar and Stellar Astrophysics",
"Mathematical Physics"
] | 5 | [
"10.1007/s10509-016-2875-0",
"10.48550/arXiv.1607.06877"
] | [
"Harko, T.",
"Mak, M. K."
] | [
"Department of Physics, Babes-Bolyai University, Cluj-Napoca, Romania; Department of Mathematics, University College London, London, United Kingdom",
"Departamento de Física, Facultad de Ciencias Naturales, Universidad de Atacama, Copiapó, Chile"
] | [
"2017Ap&SS.362..131K",
"2017EPJC...77...97S",
"2018EPJC...78..241S",
"2018Prama..91...75S",
"2018ZNatA..73..805M",
"2019AnHP...20..813A",
"2019PTEP.2019e3E02S",
"2019Prama..92...63R",
"2020BrJPh..50..725S",
"2020EPJP..135..377I",
"2020IJMPD..2950082A",
"2020PDU....2800549A",
"2020PDU....3000... | [
"1870AmJS...50...57L",
"1926ics..book.....E",
"1930MNRAS..91....4M",
"1930MNRAS..91...63F",
"1939PhRv...55..364T",
"1959PhRv..116.1027B",
"1964ApJ...140..434T",
"1974PhRvL..32..324R",
"1980Ap&SS..73..227M",
"1980esef.book.....K",
"1988RvMP...60..297B",
"1998CoPhC.115..395D",
"1999MNRAS.303..... |
901417 | 1607.04569 | The redshift evolution of massive galaxy clusters in the MACSIS simulations | We present the MAssive ClusterS and Intercluster Structures (MACSIS) project, a suite of 390 clusters simulated with baryonic physics that yields realistic massive galaxy clusters capable of matching a wide range of observed properties. MACSIS extends the recent BAryons and HAloes of MAssive Systems simulation to highe... | [
0.02239937148988247,
0.03091534785926342,
0.024952923879027367,
0.0112058836966753,
0.016982367262244225,
0.024320734664797783,
-0.005364321172237396,
-0.029601383954286575,
-0.005615337751805782,
-0.005320935510098934,
-0.029898883774876595,
-0.010511714033782482,
-0.07556533813476562,
-0... | 13.030504 | 4.638669 | 2016-07-01 | 105 | 2017MNRAS.465..213B | [
"cluster properties",
"hot clusters",
"robust predictions",
"clusters",
"realistic massive galaxy clusters",
"observed properties",
"redshift depart",
"biased X-ray temperatures",
"evolution",
"redshift",
"the complete observed cluster mass range",
"mass",
"non-thermal pressure support",
"... | [
"hydrodynamics",
"methods: numerical",
"galaxies: clusters: general",
"galaxies: clusters: intracluster medium",
"galaxies: evolution",
"X-rays: galaxies: clusters",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 27 | [
"10.1093/mnras/stw2722",
"10.48550/arXiv.1607.04569"
] | [
"Barnes, David J.",
"Kay, Scott T.",
"Henson, Monique A.",
"McCarthy, Ian G.",
"Schaye, Joop",
"Jenkins, Adrian"
] | [
"Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK",
"Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK",
"Jodrell Bank Centre for Astrophysics, School of Physics a... | [
"2016arXiv161204247P",
"2017ApJ...843...28M",
"2017MNRAS.465.2936M",
"2017MNRAS.465.3361H",
"2017MNRAS.466.4442L",
"2017MNRAS.469.3069G",
"2017MNRAS.470.4186B",
"2017MNRAS.471.1088B",
"2018A&A...620A...2M",
"2018ApJ...866..148M",
"2018JCAP...04..019M",
"2018MNRAS.473.3072M",
"2018MNRAS.474.3... | [
"1959ApJ...129..243S",
"1978MNRAS.183..341W",
"1984PhST....7..157M",
"1985ApJ...292..371D",
"1986MNRAS.222..323K",
"1986RvMP...58....1S",
"1989GeCoA..53..197A",
"1991MNRAS.252..414E",
"1993ApJ...412..455K",
"1993ApJ...412..479D",
"1997ApJ...490..493N",
"1997MNRAS.286..865T",
"1998ARA&A..36..... |
12409466 | 1607.04275 | The Scaling of Stellar Mass and Central Stellar Velocity Dispersion for Quiescent Galaxies at z<0.7 | We examine the relation between stellar mass and central stellar velocity dispersion—the M <SUB>*</SUB> σ relation—for massive quiescent galaxies at z < 0.7. We measure the local relation from the Sloan Digital Sky Survey and the intermediate redshift relation from the Smithsonian Hectospec Lensing Survey. Both samp... | [
0.05833568051457405,
0.032287392765283585,
0.0198648814111948,
-0.0009518821025267243,
0.014784462749958038,
0.055572643876075745,
-0.0031279108952730894,
-0.008723612874746323,
-0.05272047966718674,
-0.018438799306750298,
-0.052052002400159836,
0.0190849918872118,
-0.08565406501293182,
0.... | 11.773829 | 5.900778 | 2016-07-01 | 74 | 2016ApJ...832..203Z | [
"dark matter halos",
"stellar mass and central stellar velocity dispersion",
"the dark matter halo velocity dispersion",
"stellar particles",
"the central stellar velocity dispersion",
"massive quiescent galaxies",
"galaxies",
"the dark matter halo",
"the stellar mass and velocity dispersion",
"th... | [
"dark matter",
"galaxies: evolution",
"galaxies: formation",
"galaxies: high-redshift",
"galaxies: structure",
"Astrophysics - Astrophysics of Galaxies"
] | 13 | [
"10.3847/0004-637X/832/2/203",
"10.48550/arXiv.1607.04275"
] | [
"Zahid, H. Jabran",
"Geller, Margaret J.",
"Fabricant, Daniel G.",
"Hwang, Ho Seong"
] | [
"Smithsonian Astrophysical Observatory, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Smithsonian Astrophysical Observatory, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Smithsonian Astrophysical Observatory, Harvard-Smit... | [
"2017ApJ...835L..25M",
"2017ApJ...836..105K",
"2017ApJ...841...32Z",
"2017ApJ...845...73S",
"2017ApJ...845...84S",
"2017ApJS..229...20S",
"2017NatAs...1..886M",
"2018ApJ...853...39G",
"2018ApJ...859...96Z",
"2018ApJ...861..101M",
"2018ApJS..234...21D",
"2018MNRAS.474.1995R",
"2018MNRAS.479.5... | [
"1972CoASP...4..173S",
"1976ApJ...204..668F",
"1980AJ.....85..801S",
"1987ApJ...313...42D",
"1987ApJ...313...59D",
"1995MNRAS.276.1341J",
"1998ApJ...508L..43F",
"1999ApJ...527...54B",
"1999MNRAS.310..540A",
"2000AJ....120.1579Y",
"2000ApJ...533..682C",
"2002AJ....123..485S",
"2002AJ....124.1... |
12405952 | 1607.08747 | Total infrared luminosity estimation from local galaxies in AKARI all sky survey | We aim to use the a new and improved version of AKARI all sky survey catalogue of far-infrared sources to recalibrate the formula to derive the total infrared luminosity. We cross-match the faint source catalogue (FSC) of IRAS with the new AKARI-FIS and obtained a sample of 2430 objects. Then we calculate the total inf... | [
-0.0040953801944851875,
-0.03469923883676529,
0.020591115579009056,
-0.04794804006814957,
0.005672618746757507,
-0.031566519290208817,
-0.024583160877227783,
-0.02215747721493244,
-0.00797864980995655,
-0.005618230905383825,
-0.024191569536924362,
-0.02971734292805195,
0.005835781339555979,
... | 13.468505 | 7.724092 | 2016-07-01 | 7 | 2016A&A...592A.155S | [
"total infrared luminosity",
"AKARI FIS bands",
"FIR luminosity",
"AKARI bands",
"AKARI FIS",
"AKARI",
"new coefficients",
"IRAS data",
"the total infrared luminosity",
"IRAS",
"TIR",
"the TIR luminosity",
"TIR</SUB",
"AKARI-FIS",
"FIR",
"the new AKARI-FIS",
"all sky survey catalogue... | [
"infrared: galaxies",
"galaxies: star formation",
"galaxies: evolution",
"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.1051/0004-6361/201629062",
"10.48550/arXiv.1607.08747"
] | [
"Solarz, A.",
"Takeuchi, T. T.",
"Pollo, A."
] | [
"National Center for Nuclear Research, ul. Hoża 69, 00-681, Warsaw, Poland",
"Division of Particle and Astrophysical Science, Nagoya University, Furo-cho, Chikusa-ku, 464-8602, Nagoya, Japan",
"National Center for Nuclear Research, ul. Hoża 69, 00-681, Warsaw, Poland; The Astronomical Observatory of the Jagiell... | [
"2017PASP..129d4102D",
"2017arXiv170701652M",
"2019ApJ...872...49F",
"2019PASJ...71...28S",
"2019csic.conf..203P",
"2021ApJ...908..246Y",
"2022arXiv220400831T"
] | [
"1987ARA&A..25..187S",
"1988ApJS...68..151H",
"1992ifss.book.....M",
"1996A&A...315L..27K",
"1996ARA&A..34..749S",
"1998ApJ...500..525S",
"2000prpl.conf...97W",
"2001ApJ...549..215D",
"2002ApJ...576..159D",
"2004ApJS..154....1W",
"2004fost.book.....S",
"2005A&A...440L..17T",
"2005MNRAS.362..... |
2555340 | 1607.03808 | The ALMA Frontier Fields Survey. I. 1.1 mm continuum detections in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223 | Context. Dusty star-forming galaxies are among the most prodigious systems at high redshift (z > 1), characterized by high star-formation rates and huge dust reservoirs. The bright end of this population has been well characterized in recent years, but considerable uncertainties remain for fainter dusty star-forming... | [
-0.00894100870937109,
0.002906443551182747,
0.012734164483845234,
-0.013670137152075768,
-0.024470778182148933,
0.03283296152949333,
0.011367150582373142,
0.0030957935377955437,
-0.01666278950870037,
0.014298224821686745,
-0.011250154115259647,
-0.003472953801974654,
-0.02020963653922081,
... | 13.258185 | 7.239614 | 2016-07-01 | 63 | 2017A&A...597A..41G | [
"high redshift faint dusty galaxies",
"galaxy growth",
"galaxies",
"high redshift",
"star formation",
"maximum intrinsic source sensitivity",
"fainter dusty star-forming galaxies",
"dusty star-forming galaxies",
"MACS",
"Dusty star-forming galaxies",
"observed rms sensitivities",
"huge dust re... | [
"gravitational lensing: strong",
"galaxies: high-redshift",
"submillimeter: galaxies",
"Astrophysics - Astrophysics of Galaxies"
] | 12 | [
"10.1051/0004-6361/201628806",
"10.48550/arXiv.1607.03808"
] | [
"González-López, J.",
"Bauer, F. E.",
"Romero-Cañizales, C.",
"Kneissl, R.",
"Villard, E.",
"Carvajal, R.",
"Kim, S.",
"Laporte, N.",
"Anguita, T.",
"Aravena, M.",
"Bouwens, R. J.",
"Bradley, L.",
"Carrasco, M.",
"Demarco, R.",
"Ford, H.",
"Ibar, E.",
"Infante, L.",
"Messias, H.",
... | [
"Instituto de Astrofísica and Centro de Astroingeniería, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, 22, Santiago, Chile",
"Instituto de Astrofísica and Centro de Astroingeniería, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, 22, Santiago, Chile; Millenn... | [
"2016ApJ...833...25Z",
"2017A&A...602A..54M",
"2017A&A...604A.132L",
"2017A&A...608A.138G",
"2017ApJ...837..139C",
"2017ApJ...840...29H",
"2017ApJ...846L..22G",
"2017ApJ...850...83F",
"2017ApJ...850..189H",
"2017ConPh..58..160B",
"2018A&A...620A.125M",
"2018A&A...620A.152F",
"2018ApJ...854..... | [
"1996MNRAS.283.1340B",
"1997ApJ...490L...5S",
"1999ASPC..180..127B",
"2000AJ....119.2092B",
"2001ITAP...49.1683P",
"2002AJ....123.2197C",
"2002PhR...369..111B",
"2004ApJ...616...71S",
"2004ApJ...616L...1H",
"2004ApJS..154..193W",
"2005A&A...437...39B",
"2005ApJ...622..772C",
"2005ApJ...632..... |
1991062 | 1607.06336 | Observational Constraints on First-star Nucleosynthesis. I. Evidence for Multiple Progenitors of CEMP-No Stars | We investigate anew the distribution of absolute carbon abundance, A(C) = log ɛ(C), for carbon-enhanced metal-poor (CEMP) stars in the halo of the Milky Way, based on high-resolution spectroscopic data for a total sample of 305 CEMP stars. The sample includes 147 CEMP-s (and CEMP-r/s) stars, 127 CEMP-no stars, and 31 C... | [
0.0815247893333435,
0.023696135729551315,
0.04421598091721535,
-0.0027256859466433525,
0.04608142375946045,
0.0428042970597744,
0.054904453456401825,
-0.017797311767935753,
-0.0027603479102253914,
0.03420814499258995,
0.01129347737878561,
-0.004276018124073744,
-0.007701244205236435,
-0.00... | 8.092659 | 9.05972 | 2016-07-01 | 156 | 2016ApJ...833...20Y | [
"CEMP stars",
"CEMP",
"absolute carbon abundance",
"305 CEMP stars",
"31 CEMP stars",
"multiple progenitors",
"A(C",
"s",
"their observed abundances",
"classes",
"high-resolution spectroscopic data",
"r",
"first-generation stellar progenitors",
"different locations",
"first",
"Ba/Fe",
... | [
"stars: abundances",
"stars: AGB and post-AGB",
"stars: chemically peculiar",
"stars: evolution",
"stars: massive",
"stars: Population II",
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 11 | [
"10.3847/0004-637X/833/1/20",
"10.48550/arXiv.1607.06336"
] | [
"Yoon, Jinmi",
"Beers, Timothy C.",
"Placco, Vinicius M.",
"Rasmussen, Kaitlin C.",
"Carollo, Daniela",
"He, Siyu",
"Hansen, Terese T.",
"Roederer, Ian U.",
"Zeanah, Jeff"
] | [
"Department of Physics, University of Notre Dame, Notre Dame, IN 46556, USA ; Joint Institute for Nuclear Astrophysics-Center for the Evolution of the Elements (JINA-CEE), USA;",
"Department of Physics, University of Notre Dame, Notre Dame, IN 46556, USA ; Joint Institute for Nuclear Astrophysics-Center for the E... | [
"2016A&A...595L...6C",
"2016ApJ...829L..24P",
"2016ApJ...832L...3J",
"2016ApJ...833...21P",
"2017A&A...604A...9A",
"2017A&A...606A.112S",
"2017A&A...607L...3C",
"2017ApJ...834...23S",
"2017ApJ...835...81B",
"2017ApJ...836...91L",
"2017MNRAS.469.4012S",
"2017MNRAS.469.4378M",
"2017MNRAS.471..... | [
"1985AJ.....90.2089B",
"1986ApJ...300..314D",
"1990ApJ...352..709M",
"1992AJ....103.1987B",
"1992AJ....103.2035V",
"1994A&A...290..148K",
"2000A&A...354..169G",
"2000AJ....120.1579Y",
"2001AJ....122.1545P",
"2002ApJ...576L.141A",
"2002ApJ...580.1149A",
"2003AJ....125..293C",
"2003ApJ...591..... |
12510013 | 1607.01720 | Approximation of the potential in scalar field dark energy models | We study the nature of potentials in scalar field based models for dark energy—with both canonical and noncanonical kinetic terms. We calculate numerically, and using an analytic approximation around a ≈1 , potentials for models with constant equation-of-state parameter w<SUB>ϕ</SUB> . We find that for a wide range of ... | [
-0.006889462471008301,
0.015424169600009918,
-0.02365039475262165,
-0.003604685654863715,
-0.016955161467194557,
-0.02716938965022564,
-0.009391605854034424,
0.03795488178730011,
-0.023833198472857475,
0.031213950365781784,
-0.03962297737598419,
-0.007797774858772755,
-0.07385320961475372,
... | 11.146501 | 0.368012 | 2016-07-01 | 24 | 2016PhRvD..94f3513B | [
"cosmological data",
"scalar field based models",
"models",
"potentials",
"canonical and noncanonical kinetic terms",
"dark energy",
"reconstruction",
"nonconstant w<SUB>ϕ</SUB",
"both canonical and noncanonical kinetic terms",
"a simple approximation",
"state",
"an analytic approximation",
... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology"
] | 2 | [
"10.1103/PhysRevD.94.063513",
"10.48550/arXiv.1607.01720"
] | [
"Battye, Richard A.",
"Pace, Francesco"
] | [
"Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom",
"Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom"
] | [
"2017CaJPh..95.1068R",
"2017JCAP...10..040P",
"2017MNRAS.466.1839P",
"2017PhRvD..96f4041B",
"2018JCAP...01..018S",
"2018PhRvD..97j4070B",
"2019Ap&SS.364..140P",
"2019JApA...40...44R",
"2019JCAP...09..060P",
"2020CaJPh..98.1119R",
"2020IJGMM..1750139A",
"2020MPLA...3550166P",
"2020Univ....6..... | [
"1987PhRvD..35.2339F",
"1988ApJ...325L..17P",
"1988NuPhB.302..668W",
"1988PhRvD..37.3406R",
"1991CQGra...8..667E",
"1993PhRvD..48.2529C",
"1998PhRvD..57.4686C",
"1998PhRvL..80.1582C",
"1999PhLB..458..209A",
"1999PhLB..458..219G",
"1999PhRvD..59l3504S",
"2000IJMPD...9..373S",
"2000PhRvD..61h1... |
12513428 | 1607.05103 | Universal Modified Newtonian Dynamics Relation between the Baryonic and "Dynamical" Central Surface Densities of Disc Galaxies | I derive a new modified Newtonian dynamics (MOND) relation for pure-disc galaxies: The "dynamical" central surface density, Σ<SUB>D</SUB><SUP>0</SUP> , deduced from the measured velocities, is a universal function of only the true, "baryonic'' central surface density, Σ<SUB>B</SUB><SUP>0</SUP> : Σ<SUB>D</SUB><SUP>0</SU... | [
0.028745371848344803,
0.013116586022078991,
0.018310077488422394,
0.02222331240773201,
0.0149161908775568,
0.05932658165693283,
0.051451798528432846,
-0.004900602623820305,
0.024131618440151215,
-0.00015191717830020934,
-0.04717622697353363,
-0.03248951584100723,
-0.10039139539003372,
0.02... | 10.064334 | 2.096279 | 2016-07-01 | 42 | 2016PhRvL.117n1101M | [
"SUB",
"Σ<SUB",
"Σ<SUB>D</SUB><SUP>0</SUP>=(4 Σ<SUB>M</SUB>Σ<SUB",
"Lelli et al",
"Σ<SUB>B</SUB><SUP>0</SUP>≫Σ<SUB",
"Σ<SUB>B</SUB><SUP>0</SUP>≪Σ<SUB",
"disc galaxies",
"Σ<SUB>D</SUB><SUP>0</SUP>=Σ<SUB>B</SUB><SUP>0</SUP",
"y",
"Σ<SUB>D</SUB><SUP>0</SUP>=Σ<SUB>M</SUB>S",
"related attributes",
... | [
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology",
"High Energy Physics - Phenomenology"
] | 11 | [
"10.1103/PhysRevLett.117.141101",
"10.48550/arXiv.1607.05103"
] | [
"Milgrom, Mordehai"
] | [
"Department of Particle Physics and Astrophysics, Weizmann Institute, Rehovot 7610001, Israel"
] | [
"2016ApJ...832L...8M",
"2016MNRAS.463.3637R",
"2016arXiv161007538M",
"2016arXiv161009181K",
"2017A&A...603A..11P",
"2017A&A...603A..65T",
"2017Galax...5...17D",
"2017IJMPD..2650118C",
"2017MNRAS.472..765T",
"2017PhRvD..95f3020C",
"2017RAA....17...74C",
"2017arXiv170306110M",
"2018ApJ...853..... | [
"1963ApJ...138..385T",
"1983ApJ...270..365M",
"1983ApJ...270..371M",
"1984ApJ...286....7B",
"1995MNRAS.276..453B",
"2002JPhA...35.1437M",
"2009MNRAS.397.1169D",
"2009MNRAS.398.1023M",
"2010MNRAS.403..886M",
"2012LRR....15...10F",
"2014MNRAS.437.2531M",
"2014SchpJ...931410M",
"2015MNRAS.452.3... |
14285808 | 1607.02515 | Dark energy from the motions of neutrinos | Ordinarily, a scalar field may only play the role of dark energy if it possesses a potential that is either extraordinarily flat or extremely fine-tuned. Here we demonstrate that these restrictions are lifted when the scalar field undergoes persistent energy exchange with another fluid. In this scenario, the field is p... | [
0.00036220200126990676,
0.038610734045505524,
-0.04406790807843208,
-0.005535653792321682,
-0.001277516596019268,
0.0008179728174582124,
0.001462390529923141,
0.015973107889294624,
-0.0056594060733914375,
0.006809397600591183,
-0.012616703286767006,
0.022722138091921806,
-0.06621052324771881... | 7.37601 | -1.149472 | 2016-07-01 | 11 | 2018PDU....20...72S | [
"cosmic acceleration",
"dark energy",
"mass-varying neutrino models",
"state mimicks",
"energy transfer",
"freezing",
"rest",
"a cosmological constant",
"motion",
"possible means",
"a scalar field",
"the scalar field",
"a neutrino-majoron coupling",
"a derivative coupling",
"a prolonged ... | [
"Neutrinos",
"Dark energy",
"Interactions in the dark sector",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology",
"High Energy Physics - Phenomenology",
"High Energy Physics - Theory"
] | 3 | [
"10.1016/j.dark.2018.04.002",
"10.48550/arXiv.1607.02515"
] | [
"Simpson, Fergus",
"Jimenez, Raul",
"Pena-Garay, Carlos",
"Verde, Licia"
] | [
"ICC, University of Barcelona (UB-IEEC), Marti i Franques 1, 08028, Barcelona, Spain",
"ICC, University of Barcelona (UB-IEEC), Marti i Franques 1, 08028, Barcelona, Spain",
"Instituto de Fisica Corpuscular, CSIC-UVEG, P.O. 22085, Valencia, 46071, Spain",
"ICC, University of Barcelona (UB-IEEC), Marti i Franq... | [
"2016PhRvD..94j3518C",
"2016arXiv160800493M",
"2016arXiv161105710S",
"2020IJMPD..2950106R",
"2020PhRvD.101l3505K",
"2020arXiv201008181R",
"2021PDU....3100777K",
"2021PDU....3400897K",
"2021arXiv210507973R",
"2022JHEAp..34...49A",
"2024PhLB..85338687C"
] | [
"1959PhRv..115..485A",
"1981PhLB...98..265C",
"1981PhLB...99..411G",
"1982PhRvL..48.1522F",
"1983NuPhB.219...31G",
"1983RSPTA.310..347C",
"1987PhRvL..59.2607W",
"1988PhRvD..37.3406R",
"1990PhRvD..42..293C",
"1992PhR...215..203M",
"1994PhRvD..49.5925B",
"1995MNRAS.274L..73E",
"1995NuPhB.449..... |
12593474 | 1607.00383 | Correcting cosmological parameter biases for all redshift surveys induced by estimating and reweighting redshift distributions | Photometric redshift uncertainties are a major source of systematic error for ongoing and future photometric surveys. We study different sources of redshift error caused by choosing a suboptimal redshift histogram bin width and propose methods to resolve them. The selection of a too large bin width is shown to oversmoo... | [
0.036509063094854355,
-0.004236847162246704,
0.04969415441155434,
0.029439125210046768,
-0.05164918303489685,
-0.0031939747277647257,
0.004313570912927389,
-0.021039312705397606,
-0.059423841536045074,
0.031803347170352936,
-0.011394874192774296,
0.01624266803264618,
-0.015083289705216885,
... | 12.115953 | 4.110194 | 2016-07-01 | 7 | 2017MNRAS.466.2927R | [
"redshift error",
"tomographic redshift bin",
"unbiased cosmological parameter constraints",
"cosmological parameter constraints",
"suboptimal histogram bin width selection",
"Photometric redshift uncertainties",
"systematic error",
"bin width",
"errors",
"bin",
"spectroscopic calibration data",... | [
"catalogues",
"surveys",
"galaxies: distances and redshifts",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 5 | [
"10.1093/mnras/stw3338",
"10.48550/arXiv.1607.00383"
] | [
"Rau, Markus Michael",
"Hoyle, Ben",
"Paech, Kerstin",
"Seitz, Stella"
] | [
"Ludwig-Maximilians-Universität München, Universitäts-Sternwarte, Scheinerstr. 1, D-81679 Munich, Germany; Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany",
"Ludwig-Maximilians-Universität München, Universitäts-Sternwarte, Scheinerstr. 1, D-81679 Munich, Germany"... | [
"2019MNRAS.485.3642H",
"2019MNRAS.486.2730A",
"2020MNRAS.491.4768R",
"2020MNRAS.496.4769H",
"2021A&A...655A..44E",
"2022MNRAS.509.4886R",
"2023MNRAS.524.5109R"
] | [
"1985AJ.....90..418K",
"1992mde..book.....S",
"1996ApJ...461L..65F",
"1998PhRvL..81.2004K",
"2000ApJ...536..571B",
"2002PhRvD..65f3001H",
"2005IJMPA..20.3121F",
"2008ApJ...684...88N",
"2009A&A...504..359J",
"2009A&A...507..105J",
"2009MNRAS.396.2379C",
"2010ApJ...720.1351H",
"2013ApJ...764..... |
14285822 | 1607.04987 | Local Helioseismology of Emerging Active Regions: A Case Study | Local helioseismology provides a unique opportunity to investigate the subsurface structure and dynamics of active regions and their effect on the large-scale flows and global circulation of the Sun. We use measurements of plasma flows in the upper convection zone, provided by the Time-Distance Helioseismology Pipeline... | [
0.01832464523613453,
0.0454103909432888,
0.0664580836892128,
0.030466530472040176,
-0.012299743480980396,
0.020403103902935982,
-0.0006881607696413994,
-0.04122716188430786,
0.02361287735402584,
0.01466760877519846,
-0.019534887745976448,
0.040490493178367615,
-0.07303548604249954,
0.02232... | 12.008876 | 15.623784 | 2016-07-01 | 3 | 2018vsss.book...15K | [
"active region",
"active regions",
"emerging active region",
"sunspots local converging flows",
"flows",
"plasma flows",
"The active region emergence",
"large-scale flows",
"some active regions",
"the active region",
"deep layers",
"Solar Dynamics Observatory",
"the larger scale converging",... | [
"Sun: activity",
"Sun: helioseismology",
"Sun: interior",
"Sun: magnetic fields",
"Sun: oscillations",
"Astrophysics - Solar and Stellar Astrophysics",
"Physics - Fluid Dynamics",
"Physics - Plasma Physics"
] | 3 | [
"10.48550/arXiv.1607.04987"
] | [
"Kosovichev, Alexander G.",
"Zhao, Junwei",
"Ilonidis, Stathis"
] | [
"New Jersey Institute of Technology",
"Stanford University",
"Stanford University"
] | [
"2017ApJ...839...63K",
"2019LRSP...16....3T",
"2021arXiv210901833R"
] | [
"1979ApJ...230..905P",
"1996ApJ...461L..55K",
"1997ASSL..225..241K",
"1999PCEA...24..215J",
"2000SoPh..192..193B",
"2001ApJ...557..384Z",
"2001ApJ...561L.229B",
"2001ESASP.464..187B",
"2002ApJ...570..855H",
"2002ApJ...571..966G",
"2003ApJ...591..446Z",
"2003ESASP.517..103H",
"2004ApJ...603..... |
12516676 | 1607.01877 | Influence of the Magnetic Field on Oscillation Spectra in Solar Faculae | We study oscillation parameters in faculae above magnetic knots and in the areas adjacent to them. Using Solar Dynamics Observatory (SDO) data, we analyse oscillations in magnetic field strength, Doppler velocity, and intensity signals for the lower photosphere, and in intensity for the higher levels. We find peaks in ... | [
-0.0025516923051327467,
0.03637566789984703,
0.04901047796010971,
-0.02915898524224758,
0.008498147130012512,
0.06933408975601196,
-0.02024492435157299,
-0.05175326392054558,
0.014186060056090355,
-0.022819098085165024,
-0.017187390476465225,
0.01653541624546051,
-0.04662739858031273,
0.02... | 12.026763 | 15.428726 | 2016-07-01 | 8 | 2016SoPh..291.3329C | [
"magnetic field strength",
"magnetic knots",
"the magnetic field strength",
"oscillation parameters",
"oscillations",
"a moderate field strength",
"moderate-field patches",
"Doppler velocity",
"regions",
"intensity",
"the adjacent facular patches",
"the Doppler velocity oscillations",
"The t... | [
"Active regions",
"magnetic fields",
"Magnetic fields",
"photosphere",
"Oscillations",
"solar",
"Astrophysics - Solar and Stellar Astrophysics"
] | 6 | [
"10.1007/s11207-016-0954-6",
"10.48550/arXiv.1607.01877"
] | [
"Chelpanov, A. A.",
"Kobanov, N. I.",
"Kolobov, D. Y."
] | [
"Institute of Solar-Terrestrial Physics of Siberian Branch of Russian Academy of Sciences, Irkutsk, Russia",
"Institute of Solar-Terrestrial Physics of Siberian Branch of Russian Academy of Sciences, Irkutsk, Russia",
"Institute of Solar-Terrestrial Physics of Siberian Branch of Russian Academy of Sciences, Irk... | [
"2018SoPh..293..157C",
"2019A&A...627A..10R",
"2019Ap&SS.364...29S",
"2020AstBu..75..176S",
"2020Ge&Ae..59..904E",
"2020SoPh..295...94C",
"2021A&A...652A..43Y",
"2022SoPh..297...52C"
] | [
"1965ApJ...141.1131O",
"1967SoPh....2....3H",
"1969SoPh....9...35P",
"1977A&A....55..239B",
"1995itsa.conf..387M",
"1997ApJ...474..810M",
"1998BAMS...79...61T",
"1999ASPC..184..136N",
"2001A&A...379.1052K",
"2002A&A...386.1123S",
"2005A&A...437.1055M",
"2006ApJ...647L..77M",
"2006ApJ...648L.... |
12437382 | 1607.08351 | Laser-guide-stars used for cophasing broad capture ranges | Segmented primary mirrors are indispensable to master the steady increase in spatial resolution. Phasing optics systems must reduce segment misalignments to guarantee the high optical quality required for astronomical science programs. Modern telescopes routinely use adaptive optics systems to compensate for the atmosp... | [
0.020239360630512238,
0.03447147458791733,
0.026990491896867752,
-0.008491548709571362,
-0.014344400726258755,
0.05198792740702629,
-0.0229341983795166,
-0.024393903091549873,
-0.038850586861371994,
0.03879444673657417,
0.006782711949199438,
-0.025993963703513145,
-0.024562329053878784,
-0... | 14.285099 | 10.546966 | 2016-07-01 | 0 | 2016arXiv160708351M | [
"adaptive optics systems",
"adaptive optics",
"artificial stars",
"optics systems",
"astronomical science programs",
"mechanical integration requirements",
"optics",
"spatial resolution",
"observation",
"integration and re-integration process",
"bright references",
"segment misalignments",
"... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 5 | [
"10.48550/arXiv.1607.08351"
] | [
"Martinez",
"Janin-Potiron"
] | [
"-",
"-"
] | null | [
"1985A&A...152L..29F",
"1998ApOpt..37..140C",
"1999A&A...344L..45P",
"2000A&AS..144..533A",
"2005JGRD..11023302S",
"2006SPIE.6267E..2YP",
"2008SPIE.7012E..3CB",
"2011ApOpt..50.2708V",
"2012ApPhL.101x1109H",
"2012JASTP..74..181P"
] |
12521176 | 1607.01793 | Searching for High-energy Gamma-ray Counterparts to Gravitational-wave Sources with Fermi-LAT: A Needle in a Haystack | At least a fraction of gravitational-wave (GW) progenitors are expected to emit an electromagnetic (EM) signal in the form of a short gamma-ray burst (sGRB). Discovering such a transient EM counterpart is challenging because the LIGO/VIRGO localization region is much larger (several hundreds of square degrees) than the... | [
-0.053118981420993805,
-0.007308315951377153,
0.012496711686253548,
-0.03323119506239891,
-0.06524009257555008,
-0.008307798765599728,
-0.004780963063240051,
0.009822936728596687,
-0.0015780042158439755,
-0.019327567890286446,
-0.028061896562576294,
0.05454499274492264,
-0.015762535855174065... | 15.907813 | 1.393187 | 2016-07-01 | 6 | 2017ApJ...841L..16V | [
"EM counterparts",
"EM",
"radio telescopes",
"LAT",
"the short prompt phase",
"the afterglow phase",
"enough precision",
"the prompt phase",
"square degrees",
"≲",
"normal operations",
"an EM counterpart",
"any EM counterpart",
"view",
"gamma-ray bursts",
"LVT151012",
"∼2.4 sr",
"G... | [
"gamma rays: general",
"gravitational waves",
"methods: observational",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 5 | [
"10.3847/2041-8213/aa7262",
"10.48550/arXiv.1607.01793"
] | [
"Vianello, G.",
"Omodei, N.",
"Chiang, J.",
"Digel, S."
] | [
"W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA",
"W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmol... | [
"2017ApJ...835...82R",
"2017ApJ...846L...5G",
"2017PhLB..773..219D",
"2017arXiv171005450F",
"2018ApJ...861...85A",
"2019ApJ...878...52A"
] | [
"1983NIMPR.212..319H",
"1989Natur.340..126E",
"1992ApJ...395L..83N",
"1992Sci...256..325A",
"1996ApJ...461..396M",
"1998PhRvD..57.3873F",
"2002AJ....123.1086H",
"2003A&A...411L.291M",
"2005ApJ...622..759G",
"2005SSRv..120..143B",
"2007ApJ...657.1026W",
"2007NJPh....9...17L",
"2007PhR...442..... |
2074333 | 1607.03796 | Polarization sensitive Multi-Chroic MKIDs | We report on the development of scalable prototype microwave kinetic inductance detector (MKID) arrays tai- lored for future multi-kilo-pixel experiments that are designed to simultaneously characterize the polarization properties of both the cosmic microwave background (CMB) and Galactic dust emission. These modular a... | [
-0.00025076771271415055,
-0.026325292885303497,
-0.027333272621035576,
0.011781582608819008,
-0.04351331293582916,
0.062259119004011154,
-0.009673988446593285,
0.0035704742185771465,
-0.01570877805352211,
-0.011185958050191402,
0.04029301553964615,
-0.028747063130140305,
0.033930957317352295... | 10.373469 | 3.039539 | 2016-07-01 | 9 | 2016SPIE.9914E..0XJ | [
"scalable prototype microwave kinetic inductance detector",
"Galactic dust emission",
"a hybrid co-planar waveguide microwave kinetic inductance detector",
"resonant-stub band-pass filters",
"Array fabrication",
"future multi-kilo-pixel experiments",
"two spectral bands",
"190 to 280 GHz pass bands",
... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 14 | [
"10.1117/12.2233243",
"10.48550/arXiv.1607.03796"
] | [
"Johnson, Bradley R.",
"Flanigan, Daniel",
"Abitbol, Maximilian H.",
"Ade, Peter A. R.",
"Bryan, Sean",
"Cho, Hsiao-Mei",
"Datta, Rahul",
"Day, Peter",
"Doyle, Simon",
"Irwin, Kent",
"Jones, Glenn",
"Kernasovskiy, Sarah",
"Li, Dale",
"Mauskopf, Philip",
"McCarrick, Heather",
"McMahon, ... | [
"Columbia Univ. (United States)",
"Columbia Univ. (United States)",
"Columbia Univ. (United States)",
"Cardiff Univ. (United Kingdom)",
"Arizona State Univ. (United States)",
"SLAC National Accelerator Lab. (United States)",
"Univ. of Michigan (United States)",
"Jet Propulsion Lab. (United States)",
... | [
"2017ApPhL.110v2601J",
"2017arXiv170602464A",
"2018JLTP..193..103J",
"2018JLTP..193..149T",
"2018JLTP..193..170T",
"2018JLTP..193..633H",
"2020JLTP..199..362T",
"2020JLTP..200..353K",
"2022arXiv220315902B"
] | [
"2004ApPhL..85.2137D",
"2006NIMPA.559..561D",
"2008ApPhL..92u2504G",
"2008JLTP..151..530D",
"2008JLTP..151..684S",
"2010ITAP...58.1383Z",
"2010SPIE.7741E..1SN",
"2010SPIE.7741E..1VD",
"2011ApJS..194...24M",
"2012JLTP..167..852S",
"2012SPIE.8452E..05G",
"2012SPIE.8452E..1CK",
"2012SPIE.8452E.... |
12406030 | 1607.01931 | Template matching method for the analysis of interstellar cloud structure | Context. The structure of interstellar medium can be characterised at large scales in terms of its global statistics (e.g. power spectra) and at small scales by the properties of individual cores. Interest has been increasing in structures at intermediate scales, resulting in a number of methods being developed for the... | [
-0.013473416678607464,
0.02283516339957714,
0.04106311500072479,
-0.0371791273355484,
-0.02994687855243683,
0.011578299105167389,
-0.0064186230301856995,
-0.020772632211446762,
-0.019982442259788513,
0.05450974777340889,
-0.02279498428106308,
-0.03334871307015419,
0.020504772663116455,
-0.... | 11.477574 | 10.151374 | 2016-07-01 | 10 | 2016A&A...593A..58J | [
"exploratory data analysis",
"filamentary structures",
"structures",
"elongated structures",
"map analysis",
"image data",
"data quality control",
"other image features",
"small scales",
"large scales",
"intermediate scales",
"Herschel surface brightness data",
"individual cores",
"TM",
... | [
"ISM: clouds",
"ISM: structure",
"infrared: ISM",
"submillimeter: ISM",
"techniques: image processing",
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 3 | [
"10.1051/0004-6361/201628727",
"10.48550/arXiv.1607.01931"
] | [
"Juvela, M."
] | [
"Department of Physics, PO Box 64, University of Helsinki, 00014, Helsinki, Finland ; Institut UTINAM, UMR 6213, CNRS, Univ. Bourgogne Franche Comte, 41bis avenue de l'Observatoire, 25000, Besançon, France"
] | [
"2018A&A...614A..83J",
"2021A&A...649A..89M",
"2021A&A...654A..78M",
"2022A&A...668A..41C",
"2022IEEEA..1074472A",
"2022arXiv220500683A",
"2023ASPC..534..233P",
"2023MNRAS.518.5904Y",
"2023MNRAS.524.2994H",
"2024RvMPP...8...21Y"
] | [
"1981Natur.291..561A",
"1990ASSL..162..151S",
"1990ApJ...356..513S",
"1991ApJ...368..432L",
"1991ApJ...376..561M",
"1992AJ....103.1313G",
"1993MNRAS.262..327G",
"1996A&A...314..625A",
"1997ApJ...486..944E",
"1998A&A...336..150M",
"1999MNRAS.305..143W",
"2002A&A...384..225S",
"2002ApJ...580L.... |
12406155 | 1607.08021 | Study of a new central compact object: The neutron star in the supernova remnant G15.9+0.2 | We present our study of the central point source CXOU J181852.0-150213 in the young Galactic supernova remnant (SNR) G15.9+0.2 based on the recent ~90 ks Chandra observations. The point source was discovered in 2005 in shorter Chandra observations and was hypothesized to be a neutron star associated with the SNR. Our X... | [
-0.01585070602595806,
0.0059103332459926605,
-0.03882427141070366,
-0.013531089760363102,
-0.011633222922682762,
0.0016650269972160459,
0.0049936166033148766,
-0.027671372517943382,
0.05159386992454529,
-0.05121898278594017,
-0.03137338533997536,
-0.02266896888613701,
-0.07385280728340149,
... | 4.524018 | 4.696459 | 2016-07-01 | 23 | 2016A&A...592L..12K | [
"Chandra observations",
"shorter Chandra observations",
"central compact objects",
"Chandra",
"SNR",
"Galaxy",
"HESS J1731",
"Cas A",
"a neutron star",
"the neutron star",
"our hydrogen and carbon neutron star atmosphere models",
"which carbon atmosphere models",
"G15.9",
"CCOs",
"young ... | [
"stars: neutron",
"ISM: supernova remnants",
"stars: atmospheres",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 5 | [
"10.1051/0004-6361/201629208",
"10.48550/arXiv.1607.08021"
] | [
"Klochkov, D.",
"Suleimanov, V.",
"Sasaki, M.",
"Santangelo, A."
] | [
"Institut für Astronomie und Astrophysik (IAAT), Universität Tübingen, Sand 1, 72076, Tübingen, Germany",
"Institut für Astronomie und Astrophysik (IAAT), Universität Tübingen, Sand 1, 72076, Tübingen, Germany",
"Institut für Astronomie und Astrophysik (IAAT), Universität Tübingen, Sand 1, 72076, Tübingen, Germ... | [
"2017A&A...597A..65M",
"2017A&A...600A..43S",
"2017ApJ...844...84H",
"2017JPhCS.932a2006D",
"2018A&A...609A..74P",
"2018A&A...618A..76D",
"2018MNRAS.479.3033S",
"2019ApJ...875..122A",
"2019MNRAS.483...70C",
"2019MNRAS.484..974W",
"2019PASP..131k4301T",
"2019PhRvC.100e5801B",
"2020ApJ...904..... | [
"1979ApJ...228..939C",
"1982GeCoA..46.2363A",
"1983ApJ...270..119M",
"1987PASA....7..167P",
"2002ASPC..271..247P",
"2004ApJS..155..623P",
"2004IAUS..218..239P",
"2006ApJ...652L..45R",
"2006NuPhA.777..497P",
"2006SPIE.6270E..1VF",
"2007ASSL..326.....H",
"2009ApJ...703..910P",
"2009Natur.462..... |
1360289 | 1607.07456 | Upper Limits on the Rates of Binary Neutron Star and Neutron Star-Black Hole Mergers from Advanced LIGO’s First Observing Run | We report here the non-detection of gravitational waves from the merger of binary-neutron star systems and neutron star-black hole systems during the first observing run of the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO). In particular, we searched for gravitational-wave signals from binary-neut... | [
-0.008982690051198006,
0.051357824355363846,
-0.0028001596219837666,
-0.04413716867566109,
-0.023177558556199074,
-0.007029663771390915,
0.01998617872595787,
-0.003094345796853304,
-0.0012229520361870527,
0.014663102105259895,
-0.028340449556708336,
0.014120937325060368,
-0.07432591170072556... | 7.268023 | 2.479157 | 2016-07-01 | 165 | 2016ApJ...832L..21A | [
"neutron star masses",
"neutron star",
"black hole masses",
"black hole",
"neutron star-black hole systems",
"binary-neutron star systems",
"neutron star-binary mergers",
"Advanced LIGO",
"the same neutron star parameters",
"Advanced Virgo",
"(neutron star-black hole",
"∼70 Mpc",
"the black ... | [
"binaries: general",
"gamma-ray burst: general",
"gravitational waves",
"stars: black holes",
"stars: neutron",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology"
] | 14 | [
"10.3847/2041-8205/832/2/L21",
"10.48550/arXiv.1607.07456"
] | [
"Abbott, B. P.",
"Abbott, R.",
"Abbott, T. D.",
"Abernathy, M. R.",
"Acernese, F.",
"Ackley, K.",
"Adams, C.",
"Adams, T.",
"Addesso, P.",
"Adhikari, R. X.",
"Adya, V. B.",
"Affeldt, C.",
"Agathos, M.",
"Agatsuma, K.",
"Aggarwal, N.",
"Aguiar, O. D.",
"Aiello, L.",
"Ain, A.",
"Aj... | [
"LIGO, California Institute of Technology, Pasadena, CA 91125, USA",
"LIGO, California Institute of Technology, Pasadena, CA 91125, USA",
"Louisiana State University, Baton Rouge, LA 70803, USA",
"American University, Washington, D.C. 20016, USA",
"Università di Salerno, Fisciano, I-84084 Salerno, Italy ; I... | [
"2015mbhe.confE..53F",
"2016ApJ...829L..15S",
"2016CQGra..33u5004U",
"2016PhRvD..94e3013L",
"2016PhRvX...6d1015A",
"2016arXiv161201471C",
"2017A&A...604A..55M",
"2017AcA....67...37C",
"2017ApJ...836..230C",
"2017ApJ...837...57D",
"2017ApJ...837...67C",
"2017ApJ...841...89A",
"2017ApJ...844L.... | [
"1973grav.book.....M",
"1974ApJ...192L.145L",
"1974PhRvL..32..324R",
"1989Natur.340..126E",
"1992ApJ...395L..83N",
"1996ApJ...470L..61K",
"1998ApJ...507L..59L",
"1999PhRvD..60b2002O",
"2001MNRAS.322..695H",
"2002RvMP...74.1015W",
"2003ApJ...591..288H",
"2004PhRvD..69l2001A",
"2005AJ....129.1... |
12406239 | 1607.00871 | Magnetic fields during galaxy mergers | Galaxy mergers are expected to play a central role for the evolution of galaxies and may have a strong effect on their magnetic fields. We present the first grid-based 3D magnetohydrodynamical simulations investigating the evolution of magnetic fields during merger events. For this purpose, we employed a simplified mod... | [
-0.012071260251104832,
0.03388502821326256,
-0.023535020649433136,
0.0046209413558244705,
-0.044010039418935776,
0.006615005899220705,
-0.01363501138985157,
-0.0015707826241850853,
-0.033637527376413345,
-0.003600003197789192,
-0.021431269124150276,
-0.0023821895010769367,
-0.021476268768310... | 12.883754 | 9.462264 | 2016-07-01 | 13 | 2016A&A...593A..89R | [
"magnetic fields",
"magnetic field structures",
"merger events",
"efficient angular momentum transport",
"observed galaxies",
"stellar feedback",
"galaxies",
"magnetized gaseous disks",
"geometrical effects",
"Galaxy mergers",
"the average magnetic field strength",
"the magnetic field strength... | [
"Galaxy: evolution",
"galaxies: interactions",
"galaxies: magnetic fields",
"methods: numerical",
"Astrophysics - Astrophysics of Galaxies"
] | 7 | [
"10.1051/0004-6361/201527393",
"10.48550/arXiv.1607.00871"
] | [
"Rodenbeck, Kai",
"Schleicher, Dominik R. G."
] | [
"Max-Planck-Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077, Göttingen, Germany",
"Departamento de Astronomía, Facultad Ciencias Físicas y Matemáticas, Universidad de Concepción, Av. Esteban Iturra s/n Barrio Universitario, Casilla 160-C, Concepción, Chile"
] | [
"2016A&A...593A..77S",
"2017PhDT.........3G",
"2017PhRvE..95c3206G",
"2018MNRAS.475.3283C",
"2021MNRAS.506..229W",
"2022arXiv220307241S",
"2023ARA&A..61..561B",
"2023ApJ...942L..13L",
"2023EPJP..138..590S",
"2023IAUS..362...94S",
"2023arXiv231017036K",
"2024arXiv240604242N",
"2024arXiv240612... | [
"1970ApJ...160..811F",
"1977egsp.conf..401T",
"1979JCoPh..32..101V",
"1980Natur.285..643M",
"1981A&A....96..111H",
"1983ApJS...53..459C",
"1985A&A...147L...6D",
"1985AJ.....90..708K",
"1985ApJ...298L...7H",
"1985MNRAS.214...87J",
"1987ApJ...320..238S",
"1988ApJ...328...88S",
"1988ApJ...331..... |
12464338 | 1607.02363 | Behaviour of Magnetoacoustic Waves in the Neighbourhood of a Two-Dimensional Null Point: Initially Cylindrically Symmetric Perturbations | The propagation of magnetoacoustic waves in the neighbourhood of a 2D null point is investigated for both β=0 and β ≠ 0 plasmas. Previous work has shown that the Alfvén speed, here v <SUB> A </SUB>∝ r, plays a vital role in such systems and so a natural choice is to switch to polar coordinates. For β=0 plasma, we deriv... | [
-0.02393813244998455,
0.036929622292518616,
0.038888752460479736,
-0.018366854637861252,
-0.014362880028784275,
0.024440160021185875,
-0.025885019451379776,
-0.019713755697011948,
0.0022269811015576124,
0.032546065747737885,
-0.023460594937205315,
-0.020950457081198692,
-0.024378936737775803... | 12.466367 | 14.627411 | 2016-07-01 | 2 | 2016JApA...37....2M | [
"wave speed",
"magnetoacoustic waves",
"β=0 plasma",
"polar coordinates",
"such systems",
"exponential decay",
"the fast magnetoacoustic wave",
"the fast wave",
"the wave morphology",
"a 2D null point",
"large radii",
"a quasi-diamond shape",
"a semi-analytical WKB approximation",
"turn",
... | [
"Magnetohydrodynamics (MHD)",
"waves",
"magnetic fields",
"Sun: atmosphere",
"corona",
"Astrophysics - Solar and Stellar Astrophysics"
] | 3 | [
"10.1007/s12036-016-9376-y",
"10.48550/arXiv.1607.02363"
] | [
"McLaughlin, J. A."
] | [
"Department of Mathematics and Information Sciences, Northumbria University, Newcastle-upon-Tyne, United Kingdom"
] | [
"2019A&A...624A..90P",
"2019A&A...629A..60H"
] | [
"1932hydr.book.....L",
"1958ApJ...127..459F",
"1978amms.book.....B",
"1982A&A...112...16Z",
"1983A&A...117..220H",
"1991ApJ...376..355P",
"1997ApJ...486L..67C",
"1997SoPh..175...93N",
"1998A&A...337..287E",
"1998A&A...339..208B",
"2001A&A...367..339B",
"2001ApJ...548..473C",
"2002A&A...392..... |
12409306 | 1607.05775 | Vortices and Spirals in the HD135344B Transition Disk | In recent years, spiral structures have been seen in scattered light observations and signs of vortices in millimeter images of protoplanetary disks, both probably linked with the presence of planets. We present Atacama Large Millimeter/submillimeter Array Band 7 (335 GHz or 0.89 mm) continuum observations of the trans... | [
-0.01193424966186285,
-0.005556252785027027,
0.02385585755109787,
0.007383052725344896,
-0.03603031113743782,
0.0579519085586071,
0.02498101443052292,
-0.00999366957694292,
-0.0036283154040575027,
-0.020859653130173683,
-0.017534751445055008,
0.001566844410263002,
-0.04075849801301956,
-0.... | 9.515188 | 13.043775 | 2016-07-01 | 72 | 2016ApJ...832..178V | [
"vortices",
"planets",
"superuniform weighting",
"protoplanetary disks",
"longer timescales",
"spiral structures",
"scattered light observations",
"millimeter images",
"∼30 au",
"a second generation vortex",
"continuum observations",
"scattered light",
"HD 135344B",
"the secondary vortex",... | [
"instabilities",
"planet–disk interactions",
"planets and satellites: formation",
"protoplanetary disks",
"Astrophysics - Earth and Planetary Astrophysics"
] | 11 | [
"10.3847/0004-637X/832/2/178",
"10.48550/arXiv.1607.05775"
] | [
"van der Marel, N.",
"Cazzoletti, P.",
"Pinilla, P.",
"Garufi, A."
] | [
"Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, 96822 Honolulu, HI, USA",
"Max-Planck-Institut fur Extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany",
"Leiden Observatory, P.O. Box 9513, 2300 RA Leiden, the Netherlands",
"ETH, Zurich, Wolfgang-Pauli-Strasse 27, 80... | [
"2016arXiv160805123I",
"2017A&A...601A.134M",
"2017A&A...604A..88W",
"2017ASSL..445...39V",
"2017ApJ...835...38D",
"2017ApJ...835..118M",
"2017ApJ...848L..11K",
"2017ApJ...849..136T",
"2017MNRAS.464.1449R",
"2018A&A...619A.161C",
"2018ApJ...853..162B",
"2018ApJ...860...27I",
"2018ApJ...868L.... | [
"1999ApJ...513..805L",
"2002ApJ...569..997R",
"2004MNRAS.351..630L",
"2004MNRAS.355..543R",
"2005A&A...441..563V",
"2005A&A...443..945P",
"2005MNRAS.358.1489L",
"2007A&A...471.1043D",
"2007ApJ...664L.107B",
"2008ApJ...684.1323P",
"2008ApJ...686L.115C",
"2009ApJ...699.1822G",
"2009ApJ...704..... |
1867405 | 1607.07894 | The search for IR excess in low signal to noise sources | We present sources selected from their Wide-field Infrared Survey Explorer (WISE) colors that merit future observations to image for disks and possible exoplanet companions. Introducing a weighted detection method, we eliminated the enormous number of specious excess seen in low signal to noise objects by requiring gre... | [
-0.018687201663851738,
-0.005539893638342619,
0.010741827078163624,
-0.012716574594378471,
-0.010218320414423943,
-0.027076561003923416,
0.00016556313494220376,
0.010861107148230076,
-0.021510161459445953,
0.02445240132510662,
-0.026162082329392433,
-0.0017892001196742058,
-0.029660962522029... | 8.970161 | 12.9432 | 2016-07-01 | 0 | 2016arXiv160707894Z | [
"IR excess",
"disk",
"disks",
"greater excess",
"possible exoplanet companions",
"possible direct imagining",
"fainter stars",
"specious excess",
"direct imaging",
"non-Gaussian",
"disk and host star",
"noise objects",
"low signal",
"TYC",
"future observations",
"natural fluctuations",... | [
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - Solar and Stellar Astrophysics"
] | 3 | [
"10.48550/arXiv.1607.07894"
] | [
"Zink, Jonathon K.",
"Christian, Damian"
] | [
"-",
"-"
] | null | null |
12435116 | 1607.02964 | Agnostic cosmology in the CAMEL framework | Cosmological parameter estimation is traditionally performed in the Bayesian context. By adopting an "agnostic" statistical point of view, we show the interest of confronting the Bayesian results to a frequentist approach based on profile-likelihoods. To this purpose, we have developed the Cosmological Analysis with a ... | [
0.019127877429127693,
0.011999137699604034,
0.01722325198352337,
-0.033983953297138214,
-0.03082771599292755,
0.006479126401245594,
-0.01620291732251644,
-0.0036936120595782995,
0.00409494386985898,
0.04141199216246605,
0.017699409276247025,
-0.03090934455394745,
0.00883609987795353,
0.004... | 11.595018 | 3.077035 | 2016-07-01 | 8 | 2016arXiv160702964H | [
"new data",
"several Planck data analyzes",
"several estimation methods",
"Maximum Likelihood Estimate",
"Adaptive Metropolis MCMC",
"Cosmological parameter estimation",
"cosmological computations",
"http://camel.in2p3.fr",
"advanced C++ skills",
"A high quality Maximum Likelihood Estimate",
"re... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 5 | [
"10.48550/arXiv.1607.02964"
] | [
"Henrot-Versillé, S.",
"Perdereau, O.",
"Plaszczynski, S.",
"Rouillé d'Orfeuil, B.",
"Spinelli, M.",
"Tristram, M."
] | [
"-",
"-",
"-",
"-",
"-",
"-"
] | [
"2017A&A...606A.104C",
"2019A&A...623A...9H",
"2019MNRAS.482.4290H",
"2019PDU....24..260B",
"2021MNRAS.504.5840F",
"2023PDU....4201348P",
"2023PhRvD.108l3514H",
"2024arXiv240504455G"
] | [
"1953JChPh..21.1087M",
"1975CoPhC..10..343J",
"1980CoPhC..20...29J",
"1992StaSc...7..457G",
"1996NIMPA.368..793P",
"1998PhRvD..57.3873F",
"2001CQGra..18.2677C",
"2002PhRvD..66j3511L",
"2004AIPC..735..395S",
"2005MNRAS.356..925D",
"2005MNRAS.358..833T",
"2007ApJ...654....2F",
"2009MNRAS.398.1... |
2495381 | 1607.05319 | Monte Carlo simulations of soft proton flares: testing the physics with XMM-Newton | Low energy protons (< 100 - 300 keV) in the Van Allen belt and the outer regions can enter the field of view of X-ray focusing telescopes, interact with the Wolter-I optics, and reach the focal plane. The funneling of soft protons was discovered after the damaging of the Chandra/ACIS Front-Illuminated CCDs in Septem... | [
-0.009518220089375973,
0.0021295000333338976,
0.003137785941362381,
0.0016108377603814006,
-0.0037653432227671146,
0.038666557520627975,
0.009311722591519356,
0.014738721773028374,
0.025424940511584282,
0.002164991572499275,
-0.011550924740731716,
0.023230908438563347,
-0.029554879292845726,... | 9.811527 | 3.476039 | 2016-07-01 | 12 | 2016SPIE.9905E..6WF | [
"soft proton events",
"soft protons",
"soft proton flares",
"X-ray focusing telescopes",
"X-ray photons",
"board future X-ray focusing telescopes",
"Low energy protons",
"physics interaction",
"real events",
"observing time",
"EPIC",
"the X-ray mirror module",
"the soft proton population",
... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 3 | [
"10.1117/12.2232537",
"10.48550/arXiv.1607.05319"
] | [
"Fioretti, Valentina",
"Bulgarelli, Andrea",
"Malaguti, Giuseppe",
"Spiga, Daniele",
"Tiengo, Andrea"
] | [
"INAF Istituto di Astrofisica Spaziale e Fisica Cosmica Bologna (Italy)",
"INAF Istituto di Astrofisica Spaziale e Fisica Cosmica Bologna (Italy)",
"INAF Istituto di Astrofisica Spaziale e Fisica Cosmica Bologna (Italy)",
"INAF Osservatorio Astronomico di Brera (Italy)",
"INAF Istituto di Astrofisica Spazia... | [
"2016SPIE.9905E..5OS",
"2017ExA....44..321G",
"2018ApJ...866..126H",
"2018SPIE10699E..3JF",
"2020Ap&SS.365..158Z",
"2020ApJ...903...89K",
"2020SPIE11444E..2OW",
"2021JGRA..12629273K",
"2022APh...13702668Z",
"2022ApJ...928..168G",
"2023A&A...672A.156O",
"2023ApJ...947...49H"
] | [
"1967SPhD...11..732F",
"1981A&AS...44..363W",
"1987PhRvB..36....7K",
"1996SPIE.2808..402V",
"1997NIMPB.125..124W",
"1998SSRv...86..541G",
"2000AdSpR..25.1277H",
"2000SPIE.4012..154B",
"2000SPIE.4012..342S",
"2000SPIE.4140...99O",
"2000SPIE.4140..111B",
"2000SPIE.4140..123P",
"2000SPIE.4140..... |
12472677 | 1607.05633 | Finding Planet Nine: apsidal anti-alignment Monte Carlo results | The distribution of the orbital elements of the known extreme trans-Neptunian objects or ETNOs has been found to be statistically incompatible with that of an unperturbed asteroid population following heliocentric or, better, barycentric orbits. Such trends, if confirmed by future discoveries of ETNOs, strongly suggest... | [
-0.011892277747392654,
0.017290830612182617,
0.0716371238231659,
0.02494414895772934,
-0.003222704166546464,
0.023243412375450134,
0.007505148183554411,
0.008136482909321785,
-0.010127118788659573,
-0.008922429755330086,
-0.008059176616370678,
-0.020267121493816376,
-0.012768414802849293,
... | 7.603109 | 16.111691 | 2016-07-01 | 21 | 2016MNRAS.462.1972D | [
"barycentric orbits",
"Planet Nine",
"Monte Carlo techniques",
"ETNOs",
"trans-Neptunian",
"trans-Plutonian",
"Monte Carlo",
"Pluto",
"physical space",
"orbital pole position",
"much attention",
"the apsidal anti-alignment constraint",
"visibility maps",
"perihelia",
"the known extreme t... | [
"methods: statistical",
"celestial mechanics",
"minor planets",
"asteroids: general",
"Oort Cloud",
"planets and satellites: detection",
"planets and satellites: general",
"Astrophysics - Earth and Planetary Astrophysics"
] | 6 | [
"10.1093/mnras/stw1778",
"10.48550/arXiv.1607.05633"
] | [
"de la Fuente Marcos, C.",
"de la Fuente Marcos, R."
] | [
"Apartado de Correos 3413, E-28080 Madrid, Spain",
"Apartado de Correos 3413, E-28080 Madrid, Spain"
] | [
"2016PhDT.......541S",
"2017AJ....153...63S",
"2017AJ....153...65M",
"2017Ap&SS.362...11I",
"2017Ap&SS.362..198D",
"2017MNRAS.467L..66D",
"2017MNRAS.471L..61D",
"2017RNAAS...1....5D",
"2018AJ....155..166M",
"2018AJ....156...81B",
"2018AJ....156..263L",
"2018MNRAS.474..838D",
"2018RNAAS...2..... | [
"1996DPS....28.2504G",
"1999ssd..book.....M",
"2014ApJ...781....4L",
"2014MNRAS.443L..59D",
"2014Natur.507..471T",
"2015ApJ...806...42K",
"2015Icar..258...37G",
"2015MNRAS.446.1867D",
"2015MNRAS.446.3788B",
"2015MNRAS.453.3157J",
"2015MNRAS.454.3267F",
"2016A&A...587L...8F",
"2016A&A...589A.... |
5012167 | 1607.00016 | The Circumgalactic Medium of Submillimeter Galaxies. I. First Results from a Radio-identified Sample | We present the first results from an ongoing survey to characterize the circumgalactic medium (CGM) of massive high-redshift galaxies detected as submillimeter galaxies (SMGs). We constructed a parent sample of 163 SMG-QSO pairs with separations less than ∼36″ by cross-matching far-infrared-selected galaxies from Hersc... | [
0.022502506151795387,
0.050408657640218735,
0.007756641600281,
0.011536656878888607,
-0.02463352121412754,
0.016857853159308434,
-0.017035437747836113,
-0.04353359714150429,
-0.00871433038264513,
-0.008073757402598858,
-0.020954983308911324,
-0.01877322979271412,
-0.021322837099432945,
0.0... | 13.410819 | 7.307139 | 2016-07-01 | 13 | 2016ApJ...832...52F | [
"SMGs",
"prominent cool gas reservoirs",
"strong neutral absorbers",
"submillimeter galaxies",
"secure redshift identification",
"systematically strong H I Lyα absorption",
"foreground redshifts",
"compelling evidence",
"massive high-redshift galaxies",
"optically thick H I gas or metal absorption... | [
"galaxies: halos",
"intergalactic medium",
"quasars: absorption lines",
"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.3847/0004-637X/832/1/52",
"10.48550/arXiv.1607.00016"
] | [
"Fu, Hai",
"Hennawi, J. F.",
"Prochaska, J. X.",
"Mutel, R.",
"Casey, C.",
"Cooray, A.",
"Kereš, D.",
"Zhang, Z. -Y.",
"Clements, D.",
"Isbell, J.",
"Lang, C.",
"McGinnis, D.",
"Michałowski, M. J.",
"Mooley, K.",
"Perley, D.",
"Stockton, A.",
"Thompson, D."
] | [
"Department of Physics & Astronomy, University of Iowa, Iowa City, IA 52242, USA",
"Max-Planck-Institut fur Astronomie, Heidelberg, Germany",
"Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064, USA",
"Department of Physics &... | [
"2016MNRAS.463.3921M",
"2017A&A...606A..17M",
"2017ASSL..430..271F",
"2017ApJ...844..123F",
"2018ApJ...854..151M",
"2018ApJ...859..125S",
"2018ApJ...861..148M",
"2018AsBio..18..630M",
"2018AsBio..18..709C",
"2020ApJ...905...86S",
"2021ApJ...908..188F",
"2023ApJ...957...91S",
"2024arXiv240500... | [
"1985ApJ...298L...7H",
"1986PASP...98..609H",
"1992ARA&A..30..575C",
"1995AJ....110.1526H",
"1995PASP..107..375O",
"1996ApJ...462..563N",
"1997ApJ...490L...5S",
"1998A&A...331L...1S",
"1998Natur.394..241H",
"1998Natur.394..248B",
"1999ApJ...515..518E",
"2001MNRAS.321..559B",
"2002AJ....124.2... |
12472788 | 1607.03709 | The faint source population at 15.7 GHz - III. A high-frequency study of HERGs and LERGs | A complete sample of 96 faint (S > 0.5 mJy) radio galaxies is selected from the Tenth Cambridge (10C) survey at 15.7 GHz. Optical spectra are used to classify 17 of the sources as high-excitation or low-excitation radio galaxies (HERGs and LERGs, respectively), for the remaining sources three other methods are used;... | [
-0.0389772392809391,
0.016518037766218185,
-0.00024831172777339816,
-0.041534870862960815,
0.011948934756219387,
0.0573335736989975,
-0.05568176880478859,
0.0020197962876409292,
0.014240146614611149,
-0.02480369806289673,
-0.033675480633974075,
-0.017943384125828743,
-0.010323773138225079,
... | 14.947228 | 5.779402 | 2016-07-01 | 21 | 2016MNRAS.462.2122W | [
"sources",
"FR0 sources",
"low flux densities",
"flux density",
"high flux",
"radio galaxies",
"flatter radio spectra",
"higher redshifts",
"gigahertz-peaked spectrum sources",
"the AT20G sources",
"the remaining sources",
"smaller linear sizes",
"linear sizes",
"The FR0 sources",
"lower... | [
"surveys",
"galaxies: active",
"radio continuum: galaxies",
"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.1093/mnras/stw1725",
"10.48550/arXiv.1607.03709"
] | [
"Whittam, I. H.",
"Riley, J. M.",
"Green, D. A.",
"Jarvis, M. J."
] | [
"Physics and Astronomy Department, University of the Western Cape, Bellville 7535, South Africa",
"Astrophysics Group, Cavendish Laboratory, 19 JJ Thomson Avenue, Cambridge CB3 0HE, UK",
"Astrophysics Group, Cavendish Laboratory, 19 JJ Thomson Avenue, Cambridge CB3 0HE, UK",
"Physics and Astronomy Department,... | [
"2017MNRAS.464.3357W",
"2017MNRAS.471..908W",
"2018A&A...609A...1B",
"2018AstBu..73..142Z",
"2018MNRAS.474.4133H",
"2018MNRAS.480..358W",
"2019A&A...621A..19R",
"2019Galax...7...76B",
"2019MNRAS.482.2294B",
"2020MNRAS.493.2841W",
"2020MNRAS.494.2053P",
"2021A&A...650A.127T",
"2021A&ARv..29..... | [
"1973A&A....24..337S",
"1974MNRAS.167...31S",
"1974MNRAS.167P..31F",
"1979MNRAS.188..111H",
"1990AJ.....99...14B",
"1993ARA&A..31..473A",
"1994ASPC...54..201L",
"1994ApJS...95....1E",
"1995ApJ...452..710N",
"1995PASP..107..803U",
"1997ApJ...475..479W",
"1997MNRAS.286..241J",
"1998AJ....115.1... |
2774734 | 1607.03153 | The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space | We perform a tomographic baryon acoustic oscillations (BAO) analysis using the monopole, quadrupole and hexadecapole of the redshift-space galaxy power spectrum measured from the pre-reconstructed combined galaxy sample of the completed Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey (BOSS) Data Releas... | [
0.03613661602139473,
0.004896856844425201,
0.03473258018493652,
-0.010121705010533333,
-0.015478900633752346,
0.05685187131166458,
-0.01065109483897686,
-0.04131542891263962,
-0.03542308881878853,
-0.04168369993567467,
-0.055516887456178665,
-0.026860782876610756,
-0.07370027899742126,
-0.... | 12.140838 | 2.51858 | 2016-07-01 | 57 | 2017MNRAS.466..762Z | [
"lt",
"z",
"effective redshifts",
"neighbouring redshift slices",
"z <",
"BAO distance measurements",
"SUB",
"Data Release12",
"the completed Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey",
"BOSS",
"d</SUB",
"BAO",
"the pre-reconstructed combined galaxy sample",
"cosmo... | [
"galaxies: distances and redshifts",
"cosmological parameters",
"cosmology: observations",
"dark energy",
"distance scale",
"large-scale structure of Universe",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 6 | [
"10.1093/mnras/stw3199",
"10.48550/arXiv.1607.03153"
] | [
"Zhao, Gong-Bo",
"Wang, Yuting",
"Saito, Shun",
"Wang, Dandan",
"Ross, Ashley J.",
"Beutler, Florian",
"Grieb, Jan Niklas",
"Chuang, Chia-Hsun",
"Kitaura, Francisco-Shu",
"Rodriguez-Torres, Sergio",
"Percival, Will J.",
"Brownstein, Joel R.",
"Cuesta, Antonio J.",
"Eisenstein, Daniel J.",
... | [
"National Astronomy Observatories, Chinese Academy of Science, Beijing, 100012, P.R.China; Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth PO1 3FX, UK",
"National Astronomy Observatories, Chinese Academy of Science, Beijing, 100012, P.R.China; Institute of Cosm... | [
"2017ApJ...849...84W",
"2017JCAP...09..012O",
"2017JCAP...10..009H",
"2017MNRAS.464.3121W",
"2017MNRAS.468.2938S",
"2017MNRAS.468.4116P",
"2017MNRAS.469.3762W",
"2017MNRAS.470.2617A",
"2017MNRAS.471.1788C",
"2017MNRAS.471.2370C",
"2017NatAs...1..627Z",
"2017RAA....17...50Z",
"2018ApJ...855..... | [
"1970Ap&SS...7....3S",
"1970ApJ...162..815P",
"1979Natur.281..358A",
"1987MNRAS.227....1K",
"1988ApJ...325L..17P",
"1988PhRvD..37.3406R",
"1994ApJ...426...23F",
"1996AJ....111.1748F",
"1996MNRAS.282..877B",
"1998AJ....116.1009R",
"1998ApJ...496..605E",
"1999ApJ...517..565P",
"2000ApJ...538..... |
2555647 | 1607.03365 | Neutral hydrogen and magnetic fields in M83 observed with the SKA Pathfinder KAT-7 | We present new KAT-7 observations of the neutral hydrogen (H I) spectral line, and polarized radio continuum emission, in the grand-design spiral M83. These observations provide a sensitive probe of the outer-disc structure and kinematics, revealing a vast and massive neutral gas distribution that appears to be tightly... | [
0.005750826094299555,
0.029738670215010643,
-0.027530353516340256,
-0.004186601378023624,
-0.014170034788548946,
0.03616732731461525,
-0.014341793023049831,
0.0008265853975899518,
-0.013556613586843014,
0.032854851335287094,
-0.01151392050087452,
-0.03857193887233734,
-0.04497605934739113,
... | 12.636614 | 9.069626 | 2016-07-01 | 31 | 2016MNRAS.462.1238H | [
"M83",
"other nearby star-forming galaxies",
"form",
"polarized radio continuum emission",
"the main optical disc",
"the large-scale magnetic field topology",
"a large-scale regular magnetic field",
"the outer disc",
"the gaseous disc",
"spectral line",
"the magnetic field",
"the disc-halo int... | [
"galaxies: evolution",
"galaxies: individual: M83",
"galaxies: ISM",
"galaxies: kinematics and dynamics",
"galaxies: magnetic fields",
"Astrophysics - Astrophysics of Galaxies"
] | 6 | [
"10.1093/mnras/stw1698",
"10.48550/arXiv.1607.03365"
] | [
"Heald, G.",
"de Blok, W. J. G.",
"Lucero, D.",
"Carignan, C.",
"Jarrett, T.",
"Elson, E.",
"Oozeer, N.",
"Randriamampandry, T. H.",
"van Zee, L."
] | [
"CSIRO Astronomy and Space Science, 26 Dick Perry Avenue, Kensington, WA 6151, Australia; ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, NL-7990 AA Dwingeloo, the Netherlands; Kapteyn Astronomical Institute, University of Groningen, PO Box 800, NL-9700 AV Groningen, the Netherlands",
"ASTRON, t... | [
"2013pss5.book..641B",
"2016mks..confE...7D",
"2017A&A...603A.121C",
"2017ASSL..434..209B",
"2017ApJ...836..182J",
"2017ApJ...839..118V",
"2017ApJ...845..155B",
"2017ApJ...849...51B",
"2017arXiv170309345V",
"2018AJ....155..233I",
"2018MNRAS.477.3539N",
"2018MNRAS.478..487N",
"2018PASJ...70..... | [
"1981A&A...100...72H",
"1984A&A...137..159S",
"1988ngc..book.....T",
"1989Natur.340..537S",
"1991ApJ...368...60P",
"1993A&A...274..687N",
"1993ApJ...414...41M",
"1995ASPC...77..433S",
"1995PhDT.......238B",
"1996MNRAS.281...27P",
"1997PASA...14...52M",
"1998A&AS..127..409K",
"1998AJ....115.1... |
12623388 | 1607.01360 | Classes of Hydrodynamic and Magnetohydrodynamic Turbulent Decay | We perform numerical simulations of decaying hydrodynamic and magnetohydrodynamic turbulence. We classify our time-dependent solutions by their evolutionary tracks in parametric plots between instantaneous scaling exponents. We find distinct classes of solutions evolving along specific trajectories toward points on a l... | [
0.002552773803472519,
0.048667747527360916,
-0.001809307374060154,
-0.031688328832387924,
-0.006817679852247238,
0.037216510623693466,
-0.015609711408615112,
-0.00667577376589179,
0.017793836072087288,
0.04669339582324028,
-0.005873693618923426,
-0.01361068058758974,
-0.06949714571237564,
... | 12.018258 | 14.038465 | 2016-07-01 | 69 | 2017PhRvL.118e5102B | [
"solutions",
"instantaneous scaling exponents",
"specific trajectories",
"k",
"parametric plots",
"self-similar solutions",
"individual cases",
"Batchelor",
"number",
"points",
"the same trajectory",
"the solution",
"a Batchelor spectrum",
"hydrodynamic and magnetohydrodynamic turbulence",... | [
"Physics - Fluid Dynamics",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - Solar and Stellar Astrophysics"
] | 14 | [
"10.1103/PhysRevLett.118.055102",
"10.48550/arXiv.1607.01360"
] | [
"Brandenburg, Axel",
"Kahniashvili, Tina"
] | [
"Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado 80303, USA; JILA and Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, Colorado 80303, USA; Nordita, KTH Royal Institute of Technology and Stockholm University, Roslagstullsbacken 23, 10691 St... | [
"2016PhRvD..94j3510C",
"2016PhyS...91j4008K",
"2017ApJ...845L..21B",
"2017ApJ...850L...8S",
"2017JCAP...12..002K",
"2017MNRAS.472.1628P",
"2017PhRvD..96h3505P",
"2017PhRvD..96h3511S",
"2017PhRvD..96l3528B",
"2018AN....339..641B",
"2018ApJ...858..124S",
"2018CQGra..35l4003C",
"2018CQGra..35l4... | [
"1956RSPTA.248..369B",
"1967PhFl...10.1349S",
"1976JFM....77..321P",
"1979JFM....93..631C",
"1983JAtS...40..749L",
"1992PhFlA...4.1492G",
"1996PhRvD..54.1291B",
"1997PhLB..398..321O",
"1998PhRvL..80.2754M",
"1999PhRvL..82.4831S",
"1999PhRvL..83.2195B",
"2001PhRvE..64e6405C",
"2002CoPhC.147..... |
12468275 | 1607.05363 | Optical Properties of Amorphous Alumina Dust in the Envelopes around O-Rich AGB Stars | We investigate optical properties of amorphous alumina (Al_2O_3) dust grains in the envelopes around O-rich asymptotic giant branch (AGB) stars considering the laboratory measured optical data. We derive the optical constants of amorphous alumina in a wide wavelength range that satisfy the Kramers-Kronig relation and r... | [
0.010351479053497314,
0.00030043217702768743,
0.0034626855049282312,
0.0007578434888273478,
0.02984737418591976,
0.0006008643540553749,
0.033505141735076904,
-0.04564892500638962,
-0.0010211264016106725,
0.020934617146849632,
-0.0055354200303554535,
-0.02197098359465599,
0.010333189740777016... | 9.763103 | 11.231462 | 2016-07-01 | 7 | 2016JKAS...49..127S | [
"measured optical data",
"thin dust envelopes",
"amorphous alumina",
"dust",
"amorphous silicate",
"optical properties",
"the amorphous alumina dust",
"a large sample O-rich AGB stars",
"AGB",
"the laboratory measured data",
"the O-rich AGB stars",
"the observed spectral energy distributions",... | [
"Astrophysics - Solar and Stellar Astrophysics"
] | 3 | [
"10.5303/JKAS.2016.49.4.127",
"10.48550/arXiv.1607.05363"
] | [
"Suh, Kyung-Won"
] | [
"Department of Astronomy and Space Science, Chungbuk National University, Cheongju 28644, Korea"
] | [
"2018A&A...620A..75K",
"2018JKAS...51..155S",
"2019IAUS..343...31K",
"2019IAUS..343..159S",
"2020ApJ...891...43S",
"2021ApJS..256...43S",
"2022JKAS...55..195S"
] | [
"1976ApJ...209..509J",
"1983asls.book.....B",
"1995A&AS..112..143H",
"1995Icar..114..203K",
"1997ApJ...476..199B",
"1997MNRAS.287..799I",
"1998ApJS..119..141S",
"1999MNRAS.304..389S",
"2000A&AS..146..437S",
"2001ApJ...558..165E",
"2003yCat.2246....0C",
"2003yCat.5114....0E",
"2004ApJ...615..... |
12520735 | 1607.05649 | Borexino's search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts | A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos (νbar<SUB>e</SUB>) that inverse beta decay on ... | [
-0.03127787634730339,
0.021394532173871994,
0.006028839852660894,
-0.022487513720989227,
-0.04618428274989128,
0.016604017466306686,
0.013720407150685787,
0.013034386560320854,
0.0035725380294024944,
-0.04192863404750824,
-0.028626814484596252,
0.040068238973617554,
-0.06371849775314331,
-... | 5.83112 | -0.648954 | 2016-07-01 | 13 | 2017APh....86...11A | [
"Borexino data",
"Borexino",
"time correlations",
"solar neutrino physics",
"GRBs",
"events",
"November",
"MeV",
"bursts",
"December",
"the primary Borexino readout",
"neutrinos",
"two semi-independent data acquisition systems",
"neutrino and antineutrino events",
"a fast waveform digiti... | [
"Neutrinos",
"Antineutrinos",
"Gamma-ray bursts",
"Low energy/MeV neutrinos",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 4 | [
"10.1016/j.astropartphys.2016.10.004",
"10.48550/arXiv.1607.05649"
] | [
"Agostini, M.",
"Altenmüller, K.",
"Appel, S.",
"Atroshchenko, V.",
"Bellini, G.",
"Benziger, J.",
"Bick, D.",
"Bonfini, G.",
"Bravo, D.",
"Caccianiga, B.",
"Calaprice, F.",
"Caminata, A.",
"Carlini, M.",
"Cavalcante, P.",
"Chepurnov, A.",
"Choi, K.",
"D'Angelo, D.",
"Davini, S.",
... | [
"Gran Sasso Science Institute (INFN), 67100 Ł'Aquila, Italy",
"Physik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany",
"Physik-Department and Excellence Cluster Universe, Technische Universität München, 85748 Garching, Germany",
"National Research Centre Ku... | [
"2017ApJ...850...21A",
"2017arXiv170900756T",
"2018APh....97..136A",
"2018ApJ...852..120B",
"2018IJMPA..3343009C",
"2018JMPh....9..573T",
"2018JMPh....9.1827T",
"2020JPhCS1342a2035M",
"2020PhRvD.101f2001A",
"2021APh...12502509A",
"2021PTEP.2021j3F01O",
"2021Univ....7..231K",
"2022ApJ...927..... | [
"1996PhRvD..54.2779H",
"1998PhRvD..57.3873F",
"2001PhRvD..64d3004B",
"2001PhRvL..87q1102M",
"2002ApJ...578..317F",
"2003PhLB..564...42S",
"2005PhRvD..71d7303S",
"2006ApJ...641..961L",
"2006RPPh...69.2259M",
"2007ApJ...664..397A",
"2007RSPTA.365.1323W",
"2009NIMPA.600..568A",
"2009NIMPA.609..... |
12472413 | 1607.03768 | Fundamental properties of Kepler and CoRoT targets - III. Tuning scaling relations using the first adiabatic exponent | So-called scaling relations based on oscillation frequencies have the potential to reveal the mass and radius of solar-like oscillating stars. In the derivation of these relations, it is assumed that the first adiabatic exponent at the surface (Γ_{1s}) of such stars is constant. However, by constructing interior models... | [
0.01824108138680458,
0.017162172123789787,
0.06970250606536865,
-0.0346505269408226,
0.01684853620827198,
0.0528414249420166,
-0.016309082508087158,
-0.04232834279537201,
0.021264534443616867,
-0.003330816514790058,
-0.058511968702077866,
-0.03339598327875137,
-0.056203607469797134,
0.0199... | 7.57889 | 11.763339 | 2016-07-01 | 25 | 2016MNRAS.462.1577Y | [
"effective temperatures",
"new scaling relations",
"non-asteroseismic",
"stellar surfaces",
"such stars",
"oscillation frequencies",
"stellar interior models",
"stars",
"asteroseismic",
"fundamental properties",
"solar-like oscillating stars",
"_",
"solar-like oscillation frequencies",
"in... | [
"stars: evolution",
"stars: fundamental parameters",
"stars: interiors",
"stars: late-type",
"stars: oscillations",
"Astrophysics - Solar and Stellar Astrophysics"
] | 7 | [
"10.1093/mnras/stw1709",
"10.48550/arXiv.1607.03768"
] | [
"Yıldız, M.",
"Çelik Orhan, Z.",
"Kayhan, C."
] | [
"Department of Astronomy, Space Sciences, Science Faculty, Ege University, 35100, Bornova, İzmir, Turkey",
"Department of Astronomy, Space Sciences, Science Faculty, Ege University, 35100, Bornova, İzmir, Turkey",
"Department of Astronomy, Space Sciences, Science Faculty, Ege University, 35100, Bornova, İzmir, ... | [
"2017ApJ...843...11V",
"2017MNRAS.470L..25Y",
"2018ApJS..236...42Y",
"2018ApJS..239...16F",
"2019AJ....157..245H",
"2019ApJ...879...33V",
"2019ApJ...885...31C",
"2019MNRAS.487.1335K",
"2019MNRAS.489.1753Y",
"2019MNRAS.490.1509K",
"2020FrASS...7....3H",
"2020NatAs...4..382C",
"2021MNRAS.501.3... | [
"1958ZA.....46..108B",
"1983SoPh...82...55G",
"1990ApJ...362..256B",
"1991ApJ...368..599B",
"1993ApJ...412..752I",
"1995A&A...293...87K",
"1996ApJ...464..943I",
"1997A&A...323..909F",
"1998A&AS..130...65L",
"1999MNRAS.308..424C",
"1999NuPhA.656....3A",
"2002ApJ...567..643K",
"2002RvMP...74.1... |
12513984 | 1607.06821 | Solving the Hierarchy Problem at Reheating with a Large Number of Degrees of Freedom | We present a new solution to the electroweak hierarchy problem. We introduce N copies of the standard model with varying values of the Higgs mass parameter. This generically yields a sector whose weak scale is parametrically removed from the cutoff by a factor of 1 /√{N }. Ensuring that reheating deposits a majority of... | [
0.0319579541683197,
-0.04080866277217865,
0.017939912155270576,
-0.02203402854502201,
-0.057556115090847015,
0.01224922388792038,
-0.008241229690611362,
0.022590508684515953,
-0.0250549279153347,
0.020059842616319656,
-0.018363898620009422,
0.0214245468378067,
-0.08681115508079529,
0.02803... | 10.135414 | -1.446428 | 2016-07-01 | 134 | 2016PhRvL.117y1801A | [
"TeV",
"mass",
"the natural parameter space",
"varying values",
"the Higgs mass parameter",
"grand unification",
"m",
"SUB>W</SUB>M<SUB>pl</SUB>/M<SUB>GUT</SUB>∼10 TeV",
"Higgs",
"superpartners",
"the standard cosmological history",
"the electroweak hierarchy problem",
"a powerful probe",
... | [
"High Energy Physics - Phenomenology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Theory"
] | 16 | [
"10.1103/PhysRevLett.117.251801",
"10.48550/arXiv.1607.06821"
] | [
"Arkani-Hamed, Nima",
"Cohen, Timothy",
"D'Agnolo, Raffaele Tito",
"Hook, Anson",
"Kim, Hyung Do",
"Pinner, David"
] | [
"School of Natural Sciences, Institute for Advanced Study, Princeton, New Jersey 08540, USA",
"Institute of Theoretical Science, University of Oregon, Eugene, Oregon 97403, USA",
"School of Natural Sciences, Institute for Advanced Study, Princeton, New Jersey 08540, USA",
"Stanford Institute for Theoretical P... | [
"2016JHEP...12..101H",
"2016arXiv161002743A",
"2017JCAP...11..007B",
"2017JHEP...05..038C",
"2017JHEP...06..126K",
"2017JHEP...07..023C",
"2017JHEP...11..125H",
"2017JHEP...12..139B",
"2017MPLA...3250049A",
"2017PhRvD..96b3501A",
"2017PhRvD..96e5013C",
"2017arXiv170104338H",
"2017arXiv170305... | [
"1988PhRvL..60.1793R",
"1991PhRvD..43.2314D",
"2000JHEP...05..003D",
"2005JHEP...06..073A",
"2005NuPhB.708..215C",
"2006PhRvD..73f3523B",
"2009PhRvD..80e5001D",
"2010ForPh..58..528D",
"2010JHEP...03..080H",
"2013PhRvD..87h3008H",
"2014ApJ...781...31C",
"2014JHEP...01..060A",
"2014JHEP...01..... |
3481653 | 1607.01406 | Evolution of cosmic filaments and of their galaxy population from MHD cosmological simulations | Despite containing about a half of the total matter in the Universe, at most wavelengths the filamentary structure of the cosmic web is difficult to observe. In this work, we use large unigrid cosmological simulations to investigate how the geometrical, thermodynamical and magnetic properties of cosmological filaments ... | [
0.04891849681735039,
0.03468344733119011,
-0.0023734744172543287,
-0.0073087941855192184,
-0.025943031534552574,
0.0010628470918163657,
-0.04124455153942108,
-0.02789049781858921,
-0.01315698865801096,
0.013017884455621243,
-0.022442229092121124,
-0.031344931572675705,
-0.006903072353452444,... | 12.077209 | 5.132595 | 2016-07-01 | 42 | 2016MNRAS.462..448G | [
"cosmological filaments",
"filaments",
"z ≤",
"mass",
"galaxy catalogues",
"scale",
"galaxies",
"large unigrid cosmological simulations",
"magnetic field",
"statistical predictions",
"most wavelengths",
"masses",
"the host filaments",
"Mpc",
"tens",
"their observational properties",
... | [
"methods: numerical",
"intergalactic medium",
"large-scale structure of Universe",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 10 | [
"10.1093/mnras/stw1595",
"10.48550/arXiv.1607.01406"
] | [
"Gheller, C.",
"Vazza, F.",
"Brüggen, M.",
"Alpaslan, M.",
"Holwerda, B. W.",
"Hopkins, A. M.",
"Liske, J."
] | [
"ETHZ-CSCS, Via Trevano 131, CH-6900 Lugano, Switzerland",
"Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, D-21029 Hamburg, Germany; INAF-Istituto di Radio Astronomia, Via Gobetti 101, I-40129 Bologna, Italy",
"Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, D-21029 Hamburg, Germany... | [
"2017A&A...602L...6V",
"2017CQGra..34w4001V",
"2017MNRAS.467.4914V",
"2017PhDT........11N",
"2017PhRvL.119j1101M",
"2018Galax...6..128L",
"2018JHEAp..20....1G",
"2018MNRAS.478.4336M",
"2018MNRAS.479..776V",
"2018MNRAS.479.3343M",
"2018MNRAS.480.3749G",
"2018PhRvD..98d3018G",
"2018SSRv..214..... | [
"1996Natur.380..603B",
"1999ApJ...514....1C",
"2001ApJ...552..473D",
"2002JCoPh.175..645D",
"2003A&A...410..777F",
"2003AJ....126.1183C",
"2005MNRAS.359..272C",
"2005MNRAS.360.1110V",
"2005MNRAS.361..776S",
"2006ApJ...645..986R",
"2006MNRAS.370..656D",
"2007A&A...468...61D",
"2007MNRAS.380.1... |
12406440 | 1607.04479 | Partition functions. I. Improved partition functions and thermodynamic quantities for normal, equilibrium, and ortho and para molecular hydrogen | Context. Hydrogen is the most abundant molecule in the Universe. Its thermodynamic quantities dominate the physical conditions in molecular clouds, protoplanetary disks, etc. It is also of high interest in plasma physics. Therefore thermodynamic data for molecular hydrogen have to be as accurate as possible in a wide t... | [
0.005251667927950621,
0.022780796512961388,
-0.0010967757552862167,
-0.0067236777395009995,
0.039390724152326584,
-0.0221122857183218,
-0.026817575097084045,
0.010998290963470936,
0.025930512696504593,
0.008754922077059746,
0.0007267646142281592,
0.0016335130203515291,
0.023307891562581062,
... | 11.580459 | 11.650002 | 2016-07-01 | 18 | 2016A&A...595A.130P | [
"accurate partition functions",
"internal partition functions",
"New partition functions",
"excited electronic states",
"experimental values",
"ad hoc summation limits",
"thermodynamic quantities",
"anonymous ftp",
"molecular hydrogen",
"thermodynamic data",
"direct summation",
"various simpli... | [
"miscellaneous",
"molecular data",
"astrochemistry",
"equation of state",
"Physics - Chemical Physics",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Solar and Stellar Astrophysics"
] | 9 | [
"10.1051/0004-6361/201527209",
"10.48550/arXiv.1607.04479"
] | [
"Popovas, A.",
"Jørgensen, U. G."
] | [
"Niels Bohr Institute & Centre for Star and Planet Formation, University of Copenhagen, Øster Voldgade 5-7, 1350, Copenhagen K, Denmark",
"Niels Bohr Institute & Centre for Star and Planet Formation, University of Copenhagen, Øster Voldgade 5-7, 1350, Copenhagen K, Denmark"
] | [
"2018ASPC..515..145Z",
"2019A&A...630A..82L",
"2019A&A...632A.118S",
"2019JPCA..123.9905G",
"2019MNRAS.488.1846N",
"2019MNRAS.489.4890B",
"2020AcAC.1104...28G",
"2020ApPhB.126...83R",
"2021JPCA..125..795B",
"2021JPCA..125.9226Z",
"2021MNRAS.502.3394N",
"2022A&A...664A..91P",
"2022InJPh..96.2... | [
"1932PhRv...41..721D",
"1950msms.book.....H",
"1965MNRAS.129..345V",
"1966PDAO...13....1T",
"1970JChPh..52.2575T",
"1981ApJS...45..621I",
"1984A&A...130..202B",
"1984ApJS...56..193S",
"1984CaJPh..62.1639D",
"1985A&A...148...93R",
"1985JChPh..83.3034J",
"1987A&A...182..348I",
"1987JChPh..87.6... |
1367063 | 1607.01776 | In-focus wavefront sensing using non-redundant mask-induced pupil diversity | Wavefront estimation using in-focus image data is critical to many applications. This data is invariant to a sign flip with complex conjugation of the complex amplitude in the pupil, making for a non-unique solution. Information from an in-focus image taken through a non-redundant pupil mask (NRM) can break this ambigu... | [
-0.008259556256234646,
0.034936051815748215,
0.028734702616930008,
0.02203884907066822,
0.017321011051535606,
-0.013912941329181194,
0.030124660581350327,
0.043329257518053055,
-0.02294766716659069,
0.03950687497854233,
0.03464202210307121,
-0.006622346583753824,
-0.013177867978811264,
0.0... | 14.30557 | 10.590846 | 2016-07-01 | 8 | 2016OExpr..2415506G | [
"NRM fringe phase information",
"full pupil",
"NRM data",
"NRM",
"James Webb Space",
"many applications",
"a non-redundant pupil mask",
"simulated aberrations",
"Near Infrared Imager",
"Slitless Spectrograph",
"NIRISS",
"complex conjugation",
"a non-unique solution",
"Information",
"the ... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 5 | [
"10.1364/OE.24.015506",
"10.48550/arXiv.1607.01776"
] | [
"Greenbaum, Alexandra Z.",
"Sivaramakrishnan, Anand"
] | [
"-",
"-"
] | [
"2016SPIE.9904E..0FP",
"2018JATIS...4a9003D",
"2018OptCo.425...85K",
"2020Photo...8....3Q",
"2022RemS...14.4681W",
"2023ApPhL.123c4101Z",
"2023PASP..135a5003S",
"2023arXiv230904934D"
] | [
"1973JPhD....6L...6M",
"1976JOSA...66..207N",
"1982ApOpt..21.2758F",
"1986JOSAA...3.1897F",
"1995ApOpt..34.4951K",
"1999JOSAA..16.1831F",
"2004OptL...29.2840U",
"2006SPIE.6265E..0RA",
"2006SPIE.6265E..0XC",
"2006SSRv..123..485G",
"2008ApJ...688..701S",
"2008SPIE.7010E..3CB",
"2009SPIE.7440E.... |
12473506 | 1607.04686 | Cosmology and astrophysics from relaxed galaxy clusters - V. Consistency with cold dark matter structure formation | This is the fifth in a series of papers studying the astrophysics and cosmology of massive, dynamically relaxed galaxy clusters. Our sample comprises 40 clusters identified as being dynamically relaxed and hot in Papers I and II of this series. Here we use constraints on cluster mass profiles from X-ray data to test so... | [
0.040856122970581055,
0.03861516714096069,
0.02703297697007656,
-0.019637830555438995,
0.01872965320944786,
0.029391875490546227,
0.03389737010002136,
-0.006056471727788448,
-0.011275534518063068,
0.026797086000442505,
-0.05500951409339905,
0.016842534765601158,
-0.03602037951350212,
0.013... | 12.557557 | 4.61085 | 2016-07-01 | 23 | 2016MNRAS.462..681M | [
"-0.16 ±",
"CDM predictions",
"cluster mass profiles",
"massive clusters",
"cosmological structure formation",
"SUB",
"cluster",
"σ",
"small radii",
"X-ray data",
"β = 1.02 ±",
"kpc-1 Mpc",
"an intrinsic scatter",
"NFW",
"=",
"CDM) paradigm",
"Papers I",
"the cold dark matter",
"... | [
"galaxies: clusters: general",
"dark matter",
"X-rays: galaxies: clusters",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 5 | [
"10.1093/mnras/stw1707",
"10.48550/arXiv.1607.04686"
] | [
"Mantz, A. B.",
"Allen, S. W.",
"Morris, R. G."
] | [
"Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305, USA; Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, USA",
"Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanfo... | [
"2017A&A...607A..81B",
"2017MNRAS.469.1476S",
"2018ApJ...861...71S",
"2018JCAP...02..005H",
"2018MNRAS.480.2898C",
"2018MNRAS.481..361L",
"2019A&A...621A..39E",
"2019MNRAS.486.4001R",
"2019SSRv..215...25P",
"2019cxro.book...10A",
"2020MNRAS.493.4783Y",
"2020arXiv200904256D",
"2022A&A...663A.... | [
"1969Ap......5...67E",
"1993Natur.366..429W",
"1997ApJ...490..493N",
"1998ApJ...503..569E",
"1998ApJ...504....1B",
"2001MNRAS.321..372J",
"2001MNRAS.321..559B",
"2002ApJ...567..716R",
"2002ApJ...568...52W",
"2002ApJ...573....7E",
"2003A&A...398..879E",
"2003ApJ...597L...9Z",
"2004ApJ...607..... |
12462297 | 1607.03767 | A study of the lunisolar secular resonance 2dot{ω}+dot{Ω}=0 | The dynamics of small bodies around the Earth has gained a renewed interest, since the awareness of the problems that space debris can cause in the nearby future. A relevant role in space debris is played by lunisolar secular resonances, which might contribute to an increase of the orbital elements, typically of the ec... | [
0.005226595792919397,
0.041388001292943954,
0.014933130703866482,
0.002810747129842639,
0.021875377744436264,
0.07539571821689606,
0.01456146128475666,
0.008555024862289429,
-0.03899870067834854,
0.020123222842812538,
-0.0006052065873518586,
-0.022592168301343918,
-0.07151973992586136,
-0.... | 7.904739 | 15.530165 | 2016-07-01 | 9 | 2016FrASS...3...11C | [
"nearby resonances",
"space debris",
"lunisolar secular resonances",
"eccentricity",
"the lunisolar secular resonance",
"the space debris",
"the secular resonance",
"interaction",
"overlapping",
"perigee",
"2dot{ω}+dot{Ω}=0",
"increasing complexity",
"the nearby future",
"MEO",
"the orbi... | [
"space debris",
"Lunisolar secular resonance",
"Eccentricity growth",
"Astrodynamics",
"Celestial mechanics",
"Astrophysics - Earth and Planetary Astrophysics",
"70F15",
"37N05",
"34D08"
] | 4 | [
"10.3389/fspas.2016.00011",
"10.48550/arXiv.1607.03767"
] | [
"Celletti, Alessandra",
"Gales, Catalin"
] | [
"University of Roma Tor Vergata, Department of Mathematics, Roma, Italy",
"University of Iasi, Department of Mathematics, Iasi, Romania"
] | [
"2016MNRAS.460..802L",
"2017IJNLM..90..147C",
"2017MNRAS.464.4063R",
"2019Chaos..29j1106G",
"2022AdSpR..70..125C",
"2022AdSpR..70.1234T",
"2022CeMDA.134....6D",
"2023AdSpR..72.2460L",
"2023PhyD..45633946L"
] | [
"1962AJ.....67..300K",
"1962GeoJ....6..271C",
"1979PhR....52..263C",
"1980RSPSA.372..243H",
"1989CeMDA..46..287L",
"1997CeMDA..67...41F",
"2001CeMDA..81...81B",
"2008CeMDA.100..267R",
"2015AdSpR..56..388C",
"2015AdSpR..56.2626R",
"2015MNRAS.449.3522R",
"2015arXiv151202178C",
"2016CeMDA.124..... |
12406109 | 1607.08643 | Effect of bars on the galaxy properties | <BR /> Aims: With the aim of assessing the effects of bars on disk galaxy properties, we present an analysis of different characteristics of spiral galaxies with strong bars, weak bars and without bars. <BR /> Methods: We identified barred galaxies from the Sloan Digital Sky Survey (SDSS). By visual inspection of SDSS ... | [
0.017450975254178047,
0.01630564033985138,
0.014507586136460304,
0.007715621963143349,
0.0020320473704487085,
0.06364618241786957,
-0.03364577516913414,
-0.04231584444642067,
-0.0073030549101531506,
0.02471708320081234,
-0.0036884737201035023,
-0.014704632572829723,
-0.01879335753619671,
0... | 10.578901 | 6.80389 | 2016-07-01 | 32 | 2016A&A...595A..63V | [
"barred galaxies",
"unbarred galaxies",
"spiral galaxies",
"galaxy properties",
"disk galaxy properties",
"weak bars",
"strong bars",
"Strong-barred galaxies",
"strong-barred galaxies",
"bars",
"prominent bars",
"unbarred and weak-barred galaxies",
"similar distributions",
"strong-barred d... | [
"galaxies: spiral",
"galaxies: formation",
"galaxies: evolution",
"Astrophysics - Astrophysics of Galaxies"
] | 11 | [
"10.1051/0004-6361/201628750",
"10.48550/arXiv.1607.08643"
] | [
"Vera, Matias",
"Alonso, Sol",
"Coldwell, Georgina"
] | [
"ICATE, UNSJ-CONICET, CC49, 5400, San Juan, Argentina",
"Facultad de Ciencias Exactas, Físicas y Naturales, UNSJ-CONICET, 5400, San Juan, Argentina",
"Facultad de Ciencias Exactas, Físicas y Naturales, UNSJ-CONICET, 5400, San Juan, Argentina"
] | [
"2017ApJ...845...93K",
"2017MNRAS.469.1054A",
"2018A&A...618A.149A",
"2019A&A...622A.132M",
"2019A&A...632A..51C",
"2019BAAA...61..169P",
"2019MNRAS.489.4992D",
"2020A&A...641A..77C",
"2020A&A...644A..38D",
"2020AJ....159..186D",
"2020MNRAS.492.4697N",
"2020MNRAS.499.1116F",
"2020arXiv200309... | [
"1973ugcg.book.....N",
"1979A&A....80..155L",
"1979ApJ...233...67R",
"1981A&A....96..164C",
"1983IAUS..100..243A",
"1984MNRAS.210P..19B",
"1985ApJ...288..438E",
"1985MNRAS.213..451W",
"1986MNRAS.221P..41H",
"1987ApJ...323...91D",
"1989ApJ...342..677E",
"1990A&A...236..333H",
"1990ApJ...356..... |
3815852 | 1607.06697 | X-Raying the Dark Side of Venus—Scatter from Venus’ Magnetotail? | We analyze significant X-ray, EUV, and UV emission coming from the dark side of Venus observed with Hinode/XRT and Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) during a transit across the solar disk that occurred in 2012. As a check we have analyzed an analogous Mercury transit that occurred in 200... | [
-0.019748415797948837,
-0.034585174173116684,
0.0027739396318793297,
-0.019519373774528503,
0.031683988869190216,
0.06092487648129463,
-0.025716202333569527,
-0.01949392445385456,
0.017737945541739464,
-0.018196025863289833,
-0.032091174274683,
0.03903874754905701,
-0.00398594792932272,
0.... | 8.273252 | 15.162262 | 2016-07-01 | 4 | 2016AJ....152..107A | [
"Venus",
"disk line",
"residual flux",
"Venus and Mercury X-ray images",
"significant EUV",
"Venus’ shadow",
"XRT",
"UV bands",
"instrumental scattering",
"significant X",
"sight",
"Atmospheric Imaging Assembly",
"dark side",
"UV emission",
"SDO",
"Solar Dynamics Observatory",
"-",
... | [
"planets and satellites: atmospheres",
"planets and satellites: individual: Venus",
"planets and satellites: terrestrial planets",
"Sun: UV radiation",
"Sun: X-rays",
"gamma rays",
"Astrophysics - Earth and Planetary Astrophysics"
] | 4 | [
"10.3847/0004-6256/152/4/107",
"10.48550/arXiv.1607.06697"
] | [
"Afshari, M.",
"Peres, G.",
"Jibben, P. R.",
"Petralia, A.",
"Reale, F.",
"Weber, M."
] | [
"Dipartimento di Fisica e Chimica, Università di Palermo, Piazza del Parlamento 1, I-90134, Italy; INAF—Osservatorio Astronomico di Palermo, Palermo, Piazza del Parlamento 1, I-90134, Italy;",
"Dipartimento di Fisica e Chimica, Università di Palermo, Piazza del Parlamento 1, I-90134, Italy; INAF—Osservatorio Astr... | [
"2017ApJ...844....3L",
"2018ApJ...865..132D",
"2019PASJ...71R...1H",
"2023JCAP...03..001F"
] | [
"1972JOSA...62...55R",
"1974AJ.....79..745L",
"1997GeoRL..24.1163G",
"1997dis..book.....J",
"2000eaa..bookE3390F",
"2001ApJ...556L..91S",
"2002A&A...394.1119D",
"2002PASP..114.1051S",
"2007PASJ...59S.853W",
"2007SoPh..243...63G",
"2008P&SS...56.1414D",
"2008SoPh..249..263K",
"2009ApJ...690.1... |
12581239 | 1607.06468 | NLO+NLL collider bounds, Dirac fermion and scalar dark matter in the B-L model | Baryon and lepton numbers being accidental global symmetries of the Standard Model (SM), it is natural to promote them to local symmetries. However, to preserve anomaly-freedom, only combinations of B-L are viable. In this spirit, we investigate possible dark matter realizations in the context of the U(1)_B{-L} model: ... | [
0.0005890420870855451,
0.0318819023668766,
-0.02015014737844467,
-0.01795351132750511,
-0.01425972767174244,
0.015045116655528545,
0.015511441975831985,
0.022260881960392,
-0.035833392292261124,
0.003736735787242651,
-0.04785966873168945,
0.01817440241575241,
-0.03990760073065758,
0.023868... | 8.509995 | -1.766763 | 2016-07-01 | 95 | 2017EPJC...77..348K | [
"scalar dark matter",
"possible dark matter realizations",
"local symmetries",
"accidental global symmetries",
"both dark matter candidates",
"SM",
"XENON1T.",
"Z^",
"unbroken B-L",
"broken B-L",
"recent results",
"a minimal two-component dark matter model",
"prospects",
"TeV",
"LUX-2016... | [
"High Energy Physics - Phenomenology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Experiment"
] | 6 | [
"10.1140/epjc/s10052-017-4904-8",
"10.48550/arXiv.1607.06468"
] | [
"Klasen, Michael",
"Lyonnet, Florian",
"Queiroz, Farinaldo S."
] | [
"Institut für Theoretische Physik, Westfälische Wilhelms-Universität Münster, Münster, Germany",
"Southern Methodist University, Dallas, TX, USA",
"Particle and Astroparticle Physics Division, Max-Planck-Institut für Kernphysik, Heidelberg, Germany"
] | [
"2016JHEP...12..081A",
"2016JHEP...12..106A",
"2016PhLB..763..269Q",
"2016PhRvD..94g6008L",
"2016PhRvD..94i5024H",
"2016arXiv161005237M",
"2016arXiv161006587L",
"2017EPJC...77..889W",
"2017JCAP...01..042A",
"2017JCAP...04..016A",
"2017JCAP...07..016C",
"2017JCAP...11..020A",
"2017JHEP...04..... | [
"1975PhRvD..11..566M",
"1975PhRvD..11.2558M",
"1975PhRvD..12.1502S",
"1977PhLB...67..421M",
"1980PhRvD..22.2227S",
"1980PhRvL..44..912M",
"1981NuPhB.181..287L",
"1981PhRvD..23..165M",
"1983PhRvL..50.1427K",
"1991NuPhB.351..623G",
"1997PhRvD..56.1879E",
"2000PhRvD..62a3001F",
"2006JHEP...05..... |
12311754 | 1607.03883 | Two-dimensional Cellular Automaton Model for the Evolution of Active Region Coronal Plasmas | We study a two-dimensional cellular automaton (CA) model for the evolution of coronal loop plasmas. The model is based on the idea that coronal loops are made of elementary magnetic strands that are tangled and stressed by the displacement of their footpoints by photospheric motions. The magnetic stress accumulated bet... | [
0.02739850804209709,
0.030327582731842995,
0.009441728703677654,
-0.016187671571969986,
-0.017755892127752304,
0.02931666374206543,
0.0035252575762569904,
-0.06278068572282791,
-0.01814470812678337,
0.054174911230802536,
0.007296764757484198,
-0.017133789137005806,
-0.042665984481573105,
0... | 12.88736 | 15.367373 | 2016-07-01 | 21 | 2015ApJ...799..128L | [
"critical misalignment angle",
"coronal loop plasmas",
"strand length",
"active region coronal plasmas",
"field strength",
"sudden reconnection events",
"synthetic data",
"photospheric motions",
"elementary magnetic strands",
"Loops model",
"coronal loops",
"neighbor strands",
"board Hinode"... | [
"Sun: activity",
"Sun: corona",
"Sun: magnetic fields",
"Sun: X-rays",
"gamma rays",
"Astrophysics - Solar and Stellar Astrophysics"
] | 4 | [
"10.1088/0004-637X/799/2/128",
"10.48550/arXiv.1607.03883"
] | [
"López Fuentes, Marcelo",
"Klimchuk, James A."
] | [
"Instituto de Astronomía y Física del Espacio, CONICET-UBA, CC. 67, Suc. 28, 1428 Buenos Aires, Argentina; Member of the Carrera del Investigador Científico, Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Argentina.;",
"NASA Goddard Space Flight Center, Code 671, Greenbelt, MD 20771, USA"
] | [
"2015BAAA...57..231L",
"2015RSPTA.37340256K",
"2016ApJ...817....5H",
"2016ApJ...817L..11T",
"2016ApJ...821...63B",
"2016ApJ...828...86L",
"2017ApJ...840....4A",
"2017ApJ...842..108V",
"2017ApJ...849...46V",
"2018ApJ...853...82K",
"2018BAAA...60..207L",
"2020ApJ...899..156K",
"2020ApJ...905..... | [
"1978ApJ...220..643R",
"1979ApJ...233..987V",
"1983ApJ...264..635P",
"1983ApJ...264..642P",
"1988ApJ...330..474P",
"1990PhyA..163..403B",
"1991ApJ...380L..89L",
"1991SoPh..133..357H",
"1994ApJ...422..381C",
"1995ApJ...446L.109L",
"1998ApJ...501L.213K",
"1999SoPh..187..229H",
"2000ApJ...529..... |
12437432 | 1607.08533 | General background conditions for K-bounce and adiabaticity | We study the background conditions for a bounce uniquely driven by a single scalar field model with a generalized kinetic term $K(X)$, without any additional matter field. At the background level we impose the existence of two turning points where the derivative of the Hubble parameter $H$ changes sign and of a bounce ... | [
0.008877425454556942,
0.0503857396543026,
0.03561391308903694,
-0.0049467384815216064,
-0.007867887616157532,
-0.0039078909903764725,
-0.003263089107349515,
-0.01877090334892273,
0.012107948772609234,
0.023825109004974365,
-0.055387843400239944,
0.0017650640802457929,
-0.09566517174243927,
... | 10.550447 | -0.259994 | 2016-07-01 | 0 | 2016arXiv160708533E | [
"super-horizon scales",
"consecutive bounces",
"curvature perturbations",
"models",
"general gradient instabilities",
"Galileion terms",
"a single scalar field model",
"sound",
"instabilities",
"the bounce time",
"Hubble",
"the second time derivative",
"any additional matter field",
"a neg... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 5 | [
"10.48550/arXiv.1607.08533"
] | [
"Enea Romano, Antonio"
] | [
"-"
] | null | [
"2001PhRvD..64l3522K",
"2002PhRvD..65h6007K",
"2004JHEP...05..074H",
"2004PhRvD..69f3514E",
"2005PhRvD..71b3515V",
"2006JHEP...12..080C",
"2007JCAP...11..010C",
"2007JHEP...10..071C",
"2007PhRvD..75h3513A",
"2007PhRvD..76j3501L",
"2007PhRvD..76l3503B",
"2008JCAP...04..017L",
"2008PhR...465..... |
12473412 | 1607.08828 | e-MERLIN 21 cm constraints on the mass-loss rates of OB stars in Cyg OB2 | We present e-MERLIN 21 cm (L-band) observations of single luminous OB stars in the Cygnus OB2 association, from the Cyg OB2 Radio Survey Legacy programme. The radio observations potentially offer the most straightforward, least model-dependent, determinations of mass-loss rates, and can be used to help resolve current ... | [
0.02520117349922657,
0.04404954984784126,
0.012475892901420593,
-0.027983803302049637,
-0.014661307446658611,
0.036279190331697464,
0.021959146484732628,
-0.019202768802642822,
0.035386648029088974,
0.029060102999210358,
-0.024951785802841187,
-0.009509504772722721,
-0.05675514042377472,
-... | 9.076729 | 10.72618 | 2016-07-01 | 13 | 2016MNRAS.463..763M | [
"structured hot star winds",
"single luminous OB stars",
"Cyg OB2",
"evolved OB stars",
"giant stars",
"Cygnus OB2",
"multiple observations",
"luminous blue variable candidate",
"∼70 μJy",
"O6 supergiant",
"O3 supergiants",
"Hα forms",
"the Cyg OB2 Radio Survey Legacy programme",
"mass-los... | [
"stars: early type",
"stars: mass-loss",
"galaxies: clusters: individual: (Cygnus OB2)",
"radio continuum: stars",
"Astrophysics - Solar and Stellar Astrophysics"
] | 3 | [
"10.1093/mnras/stw1914",
"10.48550/arXiv.1607.08828"
] | [
"Morford, J. C.",
"Fenech, D. M.",
"Prinja, R. K.",
"Blomme, R.",
"Yates, J. A."
] | [
"Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK",
"Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK",
"Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK",
"Royal ... | [
"2017A&A...608A..69B",
"2017AcASn..58...43A",
"2017ApJ...845...39O",
"2018A&A...617A.137F",
"2018A&A...619A..54V",
"2019A&A...627A..99N",
"2019PASP..131a6001M",
"2020A&A...637A..64M",
"2020A&A...642A.168B",
"2020ApJ...895...38H",
"2022A&A...658A..61R",
"2023AJ....166...23H",
"2024ApJ...961..... | [
"1958ApJ...128...41S",
"1975MNRAS.170...41W",
"1984A&AS...57..327W",
"1985ApJ...297..751D",
"1988ApJ...335..914O",
"1989ApJ...340..518B",
"1989ApJS...71..267D",
"1990ApJ...357..573D",
"1990ApJ...361..607P",
"1991AJ....101.1408M",
"1991ApJ...377..629L",
"1993ApJ...412..771L",
"1994PASP..106.1... |
12518439 | 1607.01976 | Neutron monitors and muon detectors for solar modulation studies: 2. ϕ time series | The level of solar modulation at different times (related to the solar activity) is a central question of solar and galactic cosmic-ray physics. In the first paper of this series, we have established a correspondence between the uncertainties on ground-based detectors count rates and the parameter ϕ (modulation level i... | [
-0.03012493997812271,
0.022065414115786552,
0.012507010251283646,
-0.015185329131782055,
0.02280256524682045,
0.05307493731379509,
0.005239921156316996,
0.0077155232429504395,
0.028503205627202988,
0.0105289863422513,
-0.001224747160449624,
0.00804724171757698,
-0.04820973426103592,
0.0048... | 6.935895 | 0.093205 | 2016-07-01 | 50 | 2017AdSpR..60..833G | [
"ϕ time series",
"solar modulation",
"neutron monitor data",
"different times",
"rates",
"a reference ϕ time series",
"detectors",
"the parameter ϕ (modulation level",
"today",
"solar and galactic cosmic-ray physics",
"an unbiased and accurate ϕ reconstruction",
"these count rates",
"ground-... | [
"Solar modulation",
"Cosmic rays",
"Neutron monitor",
"Muon detector",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Solar and Stellar Astrophysics"
] | 7 | [
"10.1016/j.asr.2016.06.027",
"10.48550/arXiv.1607.01976"
] | [
"Ghelfi, A.",
"Maurin, D.",
"Cheminet, A.",
"Derome, L.",
"Hubert, G.",
"Melot, F."
] | [
"LPSC, Université Grenoble-Alpes, CNRS/IN2P3, 53 avenue des Martyrs, 38026 Grenoble, France",
"LPSC, Université Grenoble-Alpes, CNRS/IN2P3, 53 avenue des Martyrs, 38026 Grenoble, France",
"ONERA (French Aerospace Lab), 2 avenue Edouard Belin, 31055 Toulouse Cedex 4, France",
"LPSC, Université Grenoble-Alpes, ... | [
"2016PhRvD..94l3007F",
"2016PhRvD..94l3019K",
"2017ApJ...844L..26T",
"2017ICRC...35..271T",
"2017JGRA..122.3875U",
"2017JGRA..122.9790A",
"2017JGRA..12210964G",
"2017JInst..12P2021L",
"2017PhRvD..96d3007D",
"2017PhRvD..96j3005T",
"2017PhRvL.119x1101G",
"2017ehep.confE.620T",
"2018ApJ...858..... | [
"1956PhRv..104.1723M",
"1957PMag....2..157F",
"1957PhRv..107.1386M",
"1959PhRv..115..194M",
"1959PhRv..116..462M",
"1960JGR....65..767M",
"1961PhRv..121.1206A",
"1963PhRv..129.2275M",
"1964CaJPh..42.2443H",
"1964JGR....69.3097W",
"1964JGR....69.3293F",
"1964JGR....69.3939S",
"1964PhRv..133..... |
12409071 | 1607.07528 | Carbon-to-oxygen Ratios in M Dwarfs and Solar-type Stars | It has been suggested that high C/O ratios (>0.8) in circumstellar disks lead to the formation of carbon-dominated planets. Based on the expectation that elemental abundances in the stellar photospheres give the initial abundances in the circumstellar disks, the frequency distributions of C/O ratios of solar-type st... | [
0.05334382504224777,
0.032939083874225616,
0.04119814559817314,
0.002157376380637288,
0.052663665264844894,
0.05727902427315712,
0.02859092876315117,
-0.028469473123550415,
-0.015935132279992104,
0.02447354421019554,
-0.001887134974822402,
-0.0260403361171484,
-0.01656670682132244,
0.02064... | 8.082848 | 13.464513 | 2016-07-01 | 9 | 2016ApJ...830..159N | [
"oxygen lines",
"differential abundance analyses",
"stars",
"elemental abundances",
"M dwarfs",
"circumstellar disks",
"molecular line spectroscopy",
"oxygen",
"high C/O ratios",
"M",
"Carbon and oxygen abundances",
"carbon and oxygen abundances",
"neutral carbon and oxygen lines",
"solar-... | [
"stars: abundances",
"stars: low-mass",
"Astrophysics - Solar and Stellar Astrophysics"
] | 6 | [
"10.3847/0004-637X/830/2/159",
"10.48550/arXiv.1607.07528"
] | [
"Nakajima, Tadashi",
"Sorahana, Satoko"
] | [
"Astrobiology Center, 2-21-1, Osawa, Mitaka, Tokyo, 181-8588, Japan ;;",
"Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan"
] | [
"2017PASJ...69....1T",
"2018MNRAS.476.3432P",
"2019A&A...630A.104A",
"2019A&A...630A.152H",
"2019AsBio..19..867H",
"2022A&A...661A.109D",
"2023ApJ...944...41I",
"2023MNRAS.521.5761G",
"2024ApJ...961..210P"
] | [
"1987AJ.....93..864J",
"1989GeCoA..53..197A",
"1995AJ....110.1838R",
"1996AJ....112.2799H",
"2000Icar..145..637G",
"2002A&A...390..235N",
"2003Msngr.114...20M",
"2005ApJ...620..481F",
"2005ApJS..159..141V",
"2005PASJ...57...65T",
"2005astro.ph..4214K",
"2009ARA&A..47..481A",
"2009ApJ...691L.... |
11453947 | 1607.00849 | Plyades: A Python Library for Space Mission Design | Plyades: A Python Library for Space Mission Design Designing a space mission is a computation-heavy task. Software tools that conduct the necessary numerical simulations and optimizations are therefore indispensable. The usability of existing software, written in Fortran and MATLAB, suffers because of high complexity, ... | [
-0.0014797996263951063,
-0.0060340105555951595,
0.0498284250497818,
-0.039087120443582535,
0.04291418939828873,
0.015410327352583408,
0.0029452478047460318,
0.009880213998258114,
0.02070443704724312,
0.009038259275257587,
-0.018344411626458168,
-0.068938247859478,
0.00012059250730089843,
-... | 10.238004 | 4.30442 | 2016-07-01 | 0 | 2016arXiv160700849E | [
"Pythonic ease",
"use",
"Space Mission Design Designing",
"low levels",
"powerful features",
"high complexity",
"astrodynamics tools",
"Software tools",
"Pythonic",
"Plyades",
"optimizations",
"concept",
"existing software",
"MATLAB",
"a computation-heavy task",
"abstraction and out-da... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 8 | [
"10.48550/arXiv.1607.00849"
] | [
"Eichhorn, Helge",
"Anderl, Reiner"
] | [
"-",
"-"
] | null | null |
12460181 | 1607.05377 | Modeling the source of GW150914 with targeted numerical-relativity simulations | In fall of 2015, the two LIGO detectors measured the gravitational wave signal GW150914, which originated from a pair of merging black holes (Abbott et al Virgo, LIGO Scientific 2016 Phys. Rev. Lett. <A href="http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.116.061102">116</A> <A href="http://journals.aps.org/p... | [
-0.017676761373877525,
0.03981252387166023,
-0.013522987253963947,
-0.01624350994825363,
0.031478434801101685,
-0.00036619228194467723,
-0.018393386155366898,
0.007670546416193247,
-0.03437148034572601,
-0.014889883808791637,
-0.020901575684547424,
-0.016097530722618103,
-0.08318163454532623... | 8.120753 | 2.314487 | 2016-07-01 | 76 | 2016CQGra..33x4002L | [
"full numerical relativity",
"black holes",
"Abbott et al LIGO Scientific Collaboration",
"al LIGO Scientific Collaboration",
"general relativity",
"Abbott et al Virgo",
"LIGO Scientific",
"modern numerical-relativity codes",
"al Virgo",
"numerical-relativity simulations",
"LIGO",
"the same me... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 3 | [
"10.1088/0264-9381/33/24/244002",
"10.48550/arXiv.1607.05377"
] | [
"Lovelace, Geoffrey",
"Lousto, Carlos O.",
"Healy, James",
"Scheel, Mark A.",
"Garcia, Alyssa",
"O'Shaughnessy, Richard",
"Boyle, Michael",
"Campanelli, Manuela",
"Hemberger, Daniel A.",
"Kidder, Lawrence E.",
"Pfeiffer, Harald P.",
"Szilágyi, Béla",
"Teukolsky, Saul A.",
"Zlochower, Yosef... | [
"Gravitational Wave Physics and Astronomy Center, California State University Fullerton, Fullerton, CA 92834, USA ;;",
"Center for Computational Relativity and Gravitation, School of Mathematical Sciences, Rochester Institute of Technology, 85 Lomb Memorial Drive, Rochester, NY, 14623, USA",
"Center for Computa... | [
"2016PhRvD..94f4035A",
"2016arXiv161107529G",
"2017CQGra..34j4002A",
"2017CQGra..34n5011H",
"2017CQGra..34v4001H",
"2017EPJC...77..482G",
"2017PhRvD..95b4033R",
"2017PhRvD..95b4037H",
"2017PhRvD..96b4006K",
"2017PhRvD..96b4031H",
"2017PhRvD..96d4002Z",
"2017PhRvD..96h4045N",
"2017PhRvD..96j2... | [
"1964AnPhy..29..304H",
"1974PhRvD..10..428O",
"1975PhDT.......168S",
"1980PhRvD..21.2047B",
"1985CMaPh.100..525F",
"1987PThPS..90....1N",
"1995PhRvD..52.5428S",
"1997PhRvD..56.3405B",
"1997PhRvD..56.6298B",
"1997PhRvL..78.3606B",
"1998PhRvD..57..863G",
"1998PhRvD..59b4007B",
"1998PhRvL..80.1... |
4056591 | 1607.02761 | Subarcsecond international LOFAR radio images of Arp 220 at 150 MHz. A kpc-scale star forming disk surrounding nuclei with shocked outflows | Context. Arp 220 is the prototypical ultra luminous infrared galaxy (ULIRG). Despite extensive studies, the structure at MHz-frequencies has remained unknown because of limits in spatial resolution. <BR /> Aims: This work aims to constrain the flux and shape of radio emission from Arp 220 at MHz frequencies. <BR /> Met... | [
-0.014192099682986736,
-0.005173444747924805,
-0.02036626823246479,
-0.031901899725198746,
-0.01861954852938652,
0.033308979123830795,
-0.06370675563812256,
-0.04645789787173271,
0.023507939651608467,
0.015768999233841896,
-0.03723909705877304,
-0.02036626823246479,
-0.016181418672204018,
... | 12.913674 | 8.691044 | 2016-07-01 | 49 | 2016A&A...593A..86V | [
"star formation rates",
"star formation",
"steep spectrum outflows",
"dust",
"radio emission",
"spatial resolution",
"such galaxies",
"high spatial resolution",
"probe regions",
"thermal absorption",
"anonymous ftp",
"MHz frequencies",
"a star formation rate",
"resolution",
"outflows",
... | [
"ISM: structure",
"techniques: high angular resolution",
"galaxies: individual: Arp 220",
"galaxies: starburst",
"Astrophysics - Astrophysics of Galaxies"
] | 5 | [
"10.1051/0004-6361/201628702",
"10.48550/arXiv.1607.02761"
] | [
"Varenius, E.",
"Conway, J. E.",
"Martí-Vidal, I.",
"Aalto, S.",
"Barcos-Muñoz, L.",
"König, S.",
"Pérez-Torres, M. A.",
"Deller, A. T.",
"Moldón, J.",
"Gallagher, J. S.",
"Yoast-Hull, T. M.",
"Horellou, C.",
"Morabito, L. K.",
"Alberdi, A.",
"Jackson, N.",
"Beswick, R.",
"Carozzi, T... | [
"Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 439 92, Onsala, Sweden",
"Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 439 92, Onsala, Sweden",
"Department of Earth and Space Sciences, Chalmers Universi... | [
"2016PhDT.......253B",
"2017A&A...602A..42K",
"2017A&A...602A..54M",
"2017ApJ...841...44P",
"2017ApJ...844..108M",
"2017ApJ...849...14S",
"2017MNRAS.468..946S",
"2017MNRAS.469L..89Y",
"2017MNRAS.471.1634H",
"2018A&A...610L..18R",
"2018A&A...613C...3V",
"2018A&A...619A..36C",
"2018ApJ...853L.... | [
"1966ApJS...14....1A",
"1988MNRAS.230..345N",
"1988MNRAS.234..919H",
"1990ApJS...74..833H",
"1990MNRAS.246..110M",
"1991ApJ...378...65C",
"1991MNRAS.251..112S",
"1992ARA&A..30..575C",
"1995PhDT.......238B",
"1996AJ....111.1945D",
"1996MNRAS.282..779W",
"1997ApJ...484..702S",
"1998ApJ...492L.... |
12513976 | 1607.00764 | New Solutions for Non-Abelian Cosmic Strings | We study the properties of classical vortex solutions in a non-Abelian gauge theory. A system of two adjoint Higgs fields breaks the SU(2) gauge symmetry to Z<SUB>2</SUB> , producing 't Hooft-Polyakov monopoles trapped on cosmic strings, termed beads; there are two charges of monopole and two degenerate string solution... | [
-0.00742980046197772,
0.0020218694116920233,
-0.01829775609076023,
-0.0020023344550281763,
-0.02997966669499874,
0.01755542680621147,
-0.02432755008339882,
-0.010431674309074879,
0.002767454134300351,
-0.0031109440606087446,
-0.016813097521662712,
-0.018831711262464523,
-0.04886347055435181,... | 10.193118 | -1.467085 | 2016-07-01 | 23 | 2016PhRvL.117y1601H | [
"additional string solutions",
"cosmic strings",
"GUT strings",
"kink solutions",
"classical vortex solutions",
"two degenerate string solutions",
"monopole",
"grand unified theories",
"the string solutions",
"termed beads",
"a non-Abelian gauge theory",
"non-Abelian",
"SO(10",
"t Hooft-Po... | [
"High Energy Physics - Theory",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Phenomenology"
] | 16 | [
"10.1103/PhysRevLett.117.251601",
"10.48550/arXiv.1607.00764"
] | [
"Hindmarsh, Mark",
"Rummukainen, Kari",
"Weir, David J."
] | [
"Department of Physics and Astronomy, University of Sussex, Falmer, Brighton BN1 9QH, United Kingdom; Department of Physics and Helsinki Institute of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland",
"Department of Physics and Helsinki Institute of Physics, P.O. Box 64, FI-00014 University of Helsi... | [
"2016PhRvD..94d5015W",
"2017PhRvD..95f3520H",
"2017PhRvD..96b3525H",
"2017PhRvD..96j3535R",
"2017PhRvD..96l3512A",
"2018EL....12261001B",
"2018PhLB..778...22B",
"2018PhLB..780..485B",
"2018PhRvD..98f3519R",
"2018PhRvD..98j3533H",
"2018arXiv180605814X",
"2019FrP.....7...76C",
"2019RPPh...82g6... | [
"1973NuPhB..61...45N",
"1974JETPL..20..194P",
"1974NuPhB..79..276T",
"1976JPhA....9.1387K",
"1982PhLB..113..237K",
"1985NuPhB.249..557W",
"1985PhLB..153..243W",
"1985PhRvL..55.2398H",
"1986PhRvD..34.3206D",
"1986PhRvL..56.2564D",
"1987PhRvD..35.3105A",
"1987PhRvL..58.1910C",
"1989NuPhB.323..... |
12472810 | 1607.04284 | A semi-analytic dynamical friction model for cored galaxies | We present a dynamical friction model based on Chandrasekhar's formula that reproduces the fast inspiral and stalling experienced by satellites orbiting galaxies with a large constant density core. We show that the fast inspiral phase does not owe to resonance. Rather, it owes to the background velocity distribution fu... | [
0.030180195346474648,
0.03760568052530289,
-0.0033068584743887186,
0.0016974786994978786,
0.01453633327037096,
0.08387023210525513,
-0.009747523814439774,
0.017418427392840385,
0.017141545191407204,
0.033905524760484695,
-0.013038650155067444,
-0.02025018073618412,
-0.055577874183654785,
-... | 9.63481 | 5.646629 | 2016-07-01 | 58 | 2016MNRAS.463..858P | [
"constant density background distributions",
"large cores",
"SUB",
"satellites",
"a large constant density core",
"stalling",
"the constant density core",
"galaxies",
"the correct background velocity distribution function",
"the background velocity distribution function",
"core-stalling",
"pre... | [
"methods: numerical",
"galaxies: kinematics and dynamics",
"Astrophysics - Astrophysics of Galaxies"
] | 9 | [
"10.1093/mnras/stw2011",
"10.48550/arXiv.1607.04284"
] | [
"Petts, J. A.",
"Read, J. I.",
"Gualandris, A."
] | [
"Department of Physics, University of Surrey, Guildford GU2 7XH, UK",
"Department of Physics, University of Surrey, Guildford GU2 7XH, UK",
"Department of Physics, University of Surrey, Guildford GU2 7XH, UK"
] | [
"2017ApJ...837...54C",
"2017ApJ...840...31D",
"2017ApJ...844...64A",
"2017MNRAS.467.3775P",
"2017MNRAS.467.4491I",
"2017MNRAS.469.2845D",
"2017MNRAS.471..478A",
"2017PhRvD..96f3001G",
"2018A&A...615A..91B",
"2018ApJ...864L..19T",
"2018ApJ...867..119F",
"2018ApJ...868..134K",
"2018MNRAS.476.3... | [
"1943ApJ....97..255C",
"1959AnAp...22..126H",
"1960AnAp...23..474H",
"1962AJ.....67..471K",
"1983ApJ...274...53W",
"1987MNRAS.224..349B",
"1988MNRAS.235..289Z",
"1993MNRAS.262.1062S",
"1993MNRAS.265..250D",
"1994AJ....107..634T",
"1997MNRAS.289..253C",
"2003ApJ...582..196H",
"2005A&A...431..... |
1118259 | 1607.01468 | Dark matter, light mediators, and the neutrino floor | We analyze direct dark matter detection experiments for ≲100 MeV mass mediators with general interactions. We compare the nuclear recoil energy spectra from these interactions to the solar neutrino spectrum. A set of interactions that generate spectra similar to the neutrino background is identified; however, this set ... | [
-0.02020016498863697,
0.024638166651129723,
-0.01084347628057003,
-0.037247899919748306,
-0.024146296083927155,
0.07458522915840149,
0.012263189069926739,
0.037247899919748306,
0.01710362732410431,
0.015750987455248833,
-0.02866254933178425,
0.01420830748975277,
-0.03458733484148979,
0.013... | 7.492461 | -1.913864 | 2016-07-01 | 34 | 2017PhRvD..95e1701D | [
"general interactions",
"interactions",
"≳100 MeV mass mediators",
"≲100 MeV mass mediators",
"MeV",
"lower nuclear recoil energy thresholds",
"the neutrino background",
"each interaction saturates",
"direct dark matter detection experiments",
"these interactions",
"the dark matter-nucleus inter... | [
"High Energy Physics - Phenomenology",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 4 | [
"10.1103/PhysRevD.95.051701",
"10.48550/arXiv.1607.01468"
] | [
"Dent, James B.",
"Dutta, Bhaskar",
"Newstead, Jayden L.",
"Strigari, Louis E."
] | [
"Department of Physics, University of Louisiana at Lafayette, Lafayette, Louisiana 70504, USA; Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106-4030, USA",
"Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&... | [
"2017JHEP...04..073B",
"2017PhRvD..95c5017F",
"2017PhRvD..96i5007D",
"2017arXiv171206675P",
"2018JCAP...07..009G",
"2018JHEP...11..203I",
"2018PhLB..785..610M",
"2018PhRvD..97c5009D",
"2018PhRvD..98j3006O",
"2018arXiv180408995P",
"2018arXiv180411319P",
"2019ARNPS..69..137D",
"2019JCAP...01..... | [
"2010JCAP...11..042F",
"2011EPJC...71.1554C",
"2011PhRvL.107m1302A",
"2013EPJC...73.2501C",
"2013JCAP...02..004F",
"2013PhRvD..88g6011N",
"2013arXiv1311.0029E",
"2014PDU.....5...45P",
"2014PhRvC..89f5501A",
"2014PhRvD..89b3524B",
"2014PhRvD..89l3521G",
"2014PhRvD..90h3510R",
"2014PhRvL.113b1... |
12593450 | 1607.03147 | The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges | We explore the cosmological implications of anisotropic clustering measurements in configuration space of the final galaxy samples from Data Release 12 of the Sloan Digital Sky Survey III Baryon Oscillation Spectroscopic Survey. We implement a new detailed modelling of the effects of non-linearities, bias and redshift-... | [
0.060258474200963974,
0.02393989823758602,
0.02669590525329113,
-0.038000207394361496,
-0.006919214501976967,
0.015928789973258972,
0.021113822236657143,
-0.03701925650238991,
-0.03991540148854256,
-0.0030975891277194023,
-0.04617480933666229,
0.009178906679153442,
-0.09024757891893387,
-0... | 12.094464 | 2.467475 | 2016-07-01 | 165 | 2017MNRAS.464.1640S | [
"SUB",
"Baryon Oscillation Spectroscopic Survey",
"cosmological model",
"unbiased cosmological information",
"the Sloan Digital Sky Survey III Baryon Oscillation Spectroscopic Survey",
"BOSS",
"good agreement",
"cosmic structures",
"CMB",
"anisotropic clustering measurements",
"configuration spa... | [
"cosmological parameters",
"large-scale structure of Universe",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 8 | [
"10.1093/mnras/stw2443",
"10.48550/arXiv.1607.03147"
] | [
"Sánchez, Ariel G.",
"Scoccimarro, Román",
"Crocce, Martín",
"Grieb, Jan Niklas",
"Salazar-Albornoz, Salvador",
"Dalla Vecchia, Claudio",
"Lippich, Martha",
"Beutler, Florian",
"Brownstein, Joel R.",
"Chuang, Chia-Hsun",
"Eisenstein, Daniel J.",
"Kitaura, Francisco-Shu",
"Olmstead, Matthew D... | [
"Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, Giessenbachstr., D-85741 Garching, Germany",
"Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, NY 10003, USA",
"Institut de Ciències de l'Espai, IEEC-CSIC, Campus UAB, Carrer de Can Magrans, s/n, E... | [
"2016ApJ...832..103L",
"2016PhRvD..94h4022B",
"2017A&A...604A..33P",
"2017ApJ...844...91L",
"2017JCAP...02..020L",
"2017JCAP...07..014H",
"2017JCAP...08..029B",
"2017JCAP...10..009H",
"2017JCAP...10..020R",
"2017MNRAS.464.1168R",
"2017MNRAS.466..762Z",
"2017MNRAS.467.1940H",
"2017MNRAS.467.2... | [
"1979Natur.281..358A",
"1983ApJ...267..465D",
"1987MNRAS.227....1K",
"1990MNRAS.242P..43M",
"1993ApJ...412...64L",
"1994ApJ...426...23F",
"1996ApJ...461L..65F",
"1996ApJS..105...37S",
"1996MNRAS.282..877B",
"1998AJ....116.3040G",
"1998ApJ...496..605E",
"1998MNRAS.297..692C",
"1999ApJ...517..... |
3893390 | 1607.07308 | Constraints on the broad-line region properties and extinction in local Seyferts | We use high-spectral resolution (R > 8000) data covering 3800-13 000 Å to study the physical conditions of the broad-line region (BLR) of nine nearby Seyfert 1 galaxies. Up to six broad H I lines are present in each spectrum. A comparison - for the first time using simultaneous optical to near-infrared observations ... | [
-0.0272531658411026,
0.019185302779078484,
0.04634839668869972,
-0.006327546667307615,
0.0015617813915014267,
0.02623664028942585,
0.025516066700220108,
0.004403869621455669,
-0.01261005736887455,
0.03075310029089451,
-0.028256824240088463,
0.0035803557839244604,
-0.01360084768384695,
-0.0... | 15.470749 | 7.650501 | 2016-07-01 | 48 | 2016MNRAS.462.3570S | [
"BLR",
"gas",
"NLR",
"scheme",
"Seyfert",
"theoretical predictions",
"regions",
"photoionization calculations",
"dust",
"N",
"independent estimates",
"scales",
"the line ratios",
"our devised simple scheme",
"the emitting gas",
"N<SUB",
"case B",
"SUP>-3</SUP",
"the BLR and narro... | [
"dust",
"extinction",
"galaxies: active",
"galaxies: ISM",
"galaxies: nuclei",
"galaxies: Seyfert",
"Astrophysics - Astrophysics of Galaxies"
] | 7 | [
"10.1093/mnras/stw1865",
"10.48550/arXiv.1607.07308"
] | [
"Schnorr-Müller, Allan",
"Davies, R. I.",
"Korista, K. T.",
"Burtscher, L.",
"Rosario, D.",
"Storchi-Bergmann, T.",
"Contursi, A.",
"Genzel, R.",
"Graciá-Carpio, J.",
"Hicks, E. K. S.",
"Janssen, A.",
"Koss, M.",
"Lin, M. -Y.",
"Lutz, D.",
"Maciejewski, W.",
"Müller-Sánchez, F.",
"Or... | [
"Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr. 1, D-85741 Garching, Germany; CAPES Foundation, Ministry of Education of Brazil, 70040-020 Brasília, Brazil",
"Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr. 1, D-85741 Garching, Germany",
"Department of Physics, Western Mic... | [
"2016ApJ...832....8B",
"2017A&A...601A..32S",
"2017A&A...607A..37M",
"2017ApJ...836L...8C",
"2017MNRAS.466.4917D",
"2018A&A...615A.164V",
"2018ARA&A..56..625H",
"2018ApJ...856..154S",
"2018MNRAS.473.2930D",
"2018MNRAS.473.4582L",
"2018RNAAS...2....3D",
"2019A&A...628A..26P",
"2019AJ....158..... | [
"1970ApJ...160...25O",
"1975MNRAS.171..395N",
"1979RvMP...51..715D",
"1980MNRAS.193..563W",
"1981ApJ...249..462O",
"1981ApJ...250..478K",
"1983MNRAS.202..453B",
"1985ApJ...289...67D",
"1987ApJ...315...74W",
"1988ApJ...332..172R",
"1989ApJ...340..190G",
"1992AJ....104.2072T",
"1992ApJS...79..... |
12593903 | 1607.02141 | Bar-driven evolution and quenching of spiral galaxies in cosmological simulations | We analyse the outputs of the cosmological 'zoom-in' hydrodynamical simulation ErisBH to study a strong stellar bar which naturally emerges in the late evolution of the simulated Milky Way-type galaxy. We focus on the analysis of the formation and evolution of the bar and on its effects on the galactic structure, the g... | [
0.025187529623508453,
0.030193988233804703,
0.011280701495707035,
-0.010362204164266586,
-0.033376388251781464,
0.04545915871858597,
-0.003787185065448284,
0.029961129650473595,
-0.028538106009364128,
-0.01107371598482132,
0.026429442688822746,
0.011325979605317116,
-0.06452768296003342,
-... | 10.387046 | 6.649911 | 2016-07-01 | 74 | 2017MNRAS.465.3729S | [
"bar",
"gas inflows",
"sub-kpc scales",
"stars",
"z",
"evolution",
"buckling instability",
"bar-driven quenching",
"a strong stellar bar",
"Milky Way",
"the nuclear star formation",
"disc-dominated galaxies",
"the galactic central region",
"a clear bar",
"the central ∼2 kpc",
"the star... | [
"methods: numerical",
"galaxies: bulges",
"galaxies: evolution",
"galaxies: formation",
"galaxies: kinematics and dynamics",
"galaxies: structure",
"Astrophysics - Astrophysics of Galaxies"
] | 15 | [
"10.1093/mnras/stw2934",
"10.48550/arXiv.1607.02141"
] | [
"Spinoso, Daniele",
"Bonoli, Silvia",
"Dotti, Massimo",
"Mayer, Lucio",
"Madau, Piero",
"Bellovary, Jillian"
] | [
"Università degli Studi di Milano-Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy; Centro de estudios de fisí ca del cosmos de Aragó n, plaza San Juan, 1 planta-2 E-44001 Teruel, Spain",
"Centro de estudios de fisí ca del cosmos de Aragó n, plaza San Juan, 1 planta-2 E-44001 Teruel, Spain",
"Università d... | [
"2017ApJ...835..289S",
"2017ApJ...838..105L",
"2017MNRAS.469.2806A",
"2017MNRAS.469.3722R",
"2017PASA...34...41N",
"2018A&A...609A..60K",
"2018ApJ...868..100G",
"2018MNRAS.473.2608Z",
"2018MNRAS.473.4731K",
"2018MNRAS.474.1909F",
"2018MNRAS.474.3101J",
"2018MNRAS.476.2318S",
"2018MNRAS.478.1... | [
"1964ApJ...139.1217T",
"1976ApJ...209...53S",
"1977ApJ...217..916S",
"1978ApJ...222..850G",
"1979ApJ...233...67R",
"1979ApJ...233..857G",
"1981A&A....96..164C",
"1989Natur.338...45S",
"1992MNRAS.259..345A",
"1993A&A...271..391C",
"1993RPPh...56..173S",
"1997A&A...323..363M",
"1997ApJ...482L.... |
3481761 | 1607.01096 | Galaxy And Mass Assembly (GAMA): M_star - R_e relations of z = 0 bulges, discs and spheroids | We perform automated bulge + disc decomposition on a sample of ∼7500 galaxies from the Galaxy And Mass Assembly (GAMA) survey in the redshift range of 0.002 < z < 0.06 using Structural Investigation of Galaxies via Model Analysis, a wrapper around GALFIT3. To achieve robust profile measurements, we use a novel ap... | [
0.04623211547732353,
0.05655335262417793,
0.05710582807660103,
0.014552694745361805,
0.01140107586979866,
0.02442190796136856,
0.006924772169440985,
-0.002925606444478035,
0.013523082248866558,
0.006981275510042906,
-0.034881263971328735,
-0.022551026195287704,
-0.04683481529355049,
-0.007... | 12.01799 | 6.202541 | 2016-07-01 | 102 | 2016MNRAS.462.1470L | [
"Deep Extragalactic",
"Survey-Ultra Deep Survey",
"Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey-Ultra Deep Survey",
"simulated data",
"disc decomposition",
"elliptical relation",
"discs",
"galaxy evolution",
"∼7500 galaxies",
"Mass Assembly",
"spheroids",
"lt",
"GALFIT3",
... | [
"galaxies: elliptical and lenticular",
"cD",
"galaxies: formation",
"galaxies: fundamental parameters",
"galaxies: spiral",
"galaxies: statistics",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 37 | [
"10.1093/mnras/stw1495",
"10.48550/arXiv.1607.01096"
] | [
"Lange, Rebecca",
"Moffett, Amanda J.",
"Driver, Simon P.",
"Robotham, Aaron S. G.",
"Lagos, Claudia del P.",
"Kelvin, Lee S.",
"Conselice, Christopher",
"Margalef-Bentabol, Berta",
"Alpaslan, Mehmet",
"Baldry, Ivan",
"Bland-Hawthorn, Joss",
"Bremer, Malcolm",
"Brough, Sarah",
"Cluver, Mic... | [
"International Centre for Radio Astronomy Research, University of Western Australia, M468, 35 Stirling Highway, Crawley, WA 6009, Australia",
"International Centre for Radio Astronomy Research, University of Western Australia, M468, 35 Stirling Highway, Crawley, WA 6009, Australia",
"International Centre for Ra... | [
"2016MNRAS.462.4336M",
"2017AJ....153..111G",
"2017ApJ...849...55S",
"2017MNRAS.466.1513R",
"2017MNRAS.466.3569P",
"2017MNRAS.467..179G",
"2017MNRAS.467.1033B",
"2017MNRAS.467.2066S",
"2017MNRAS.467.3751B",
"2017MNRAS.469..968X",
"2017MNRAS.471..447S",
"2017PASA...34...47D",
"2018ApJ...863..... | [
"1926ApJ....64..321H",
"1964ApJ...139.1217T",
"1976ApJ...206..883V",
"1977egsp.conf..401T",
"1980MNRAS.193..189F",
"1994ARA&A..32..115R",
"1996A&AS..117..393B",
"1997ApJ...482..659D",
"1998ASPC..145..108S",
"1998MNRAS.295..319M",
"2000AJ....120.1579Y",
"2000ApJ...533..682C",
"2002NewA....7..... |
12436535 | 1607.06480 | Very-high energy emission from pulsars | The vast majority of pulsars detected by the Fermi Large Area Telescope (LAT) display exponentially cutoff spectra with cutoffs falling in a narrow band around a few GeV. Early spectral modelling predicted spectral cutoffs at energies of up to 100 GeV, assuming curvature radiation. It was therefore not expected that pu... | [
-0.025759393349289894,
0.022099873051047325,
0.025720462203025818,
-0.017518984153866768,
-0.008039266802370548,
0.04383638873696327,
-0.030625779181718826,
0.004052076023072004,
0.05325771123170853,
-0.04744400084018707,
0.005473060067743063,
0.024474669247865677,
-0.0690377727150917,
-0.... | 5.536493 | 4.261087 | 2016-07-01 | 2 | 2016arXiv160706480B | [
"new radiation mechanisms",
"radiation models",
"curvature radiation",
"magnetic field structures",
"spectral cutoffs",
"other pulsars",
"pulsars",
"VHE pulsar science",
"VHE pulsar",
"VHE emission",
"cutoffs",
"pulsed emission",
"VHE",
"energies",
"local environment",
"important quest... | [
"Astrophysics - High Energy Astrophysical Phenomena"
] | 6 | [
"10.48550/arXiv.1607.06480"
] | [
"Breed, M.",
"Venter, C.",
"Harding, A. K."
] | [
"-",
"-",
"-"
] | [
"2016heas.confE..40V",
"2017ASSL..446...61D"
] | [
"1969ApJ...157..869G",
"1981ApJ...245..267H",
"1982ApJ...252..337D",
"1983ApJ...266..215A",
"1986ApJ...300..522C",
"1996ApJ...470..469R",
"2000MNRAS.317...97B",
"2001ApJ...549..495H",
"2002ApJ...576..366H",
"2005AdSpR..35.1152F",
"2005ApJ...619L.167V",
"2005ApJ...622..531H",
"2008ApJ...676..... |
12407656 | 1607.03570 | Equilibrium Sequences and Gravitational Instability of Rotating Isothermal Rings | Nuclear rings at the centers of barred galaxies exhibit strong star formation activities. They are thought to undergo gravitational instability when they are sufficiently massive. We approximate them as rigidly rotating isothermal objects and investigate their gravitational instability. Using a self-consistent field me... | [
-0.006438659504055977,
0.05040371045470238,
0.03047841601073742,
-0.005323672201484442,
0.011175000108778477,
0.012757968157529831,
0.03841838240623474,
-0.019988112151622772,
-0.007267833221703768,
-0.005358221009373665,
-0.005615767557173967,
-0.02319173701107502,
-0.08950050920248032,
-... | 10.217501 | 6.905362 | 2016-07-01 | 3 | 2016ApJ...829...45K | [
"slender rings",
"ring thickness",
"smaller α",
"Rings",
"rings",
"Nuclear rings",
"young star clusters",
"strong star formation activities",
"gravitational potential energy",
"α",
"such equilibria",
"gravitational instability",
"a larger unstable range",
"non-axisymmetric modes",
"obser... | [
"galaxies: ISM",
"galaxies: kinematics and dynamics",
"galaxies: nuclei",
"galaxies: structure",
"instabilities",
"stars: formation",
"Astrophysics - Astrophysics of Galaxies"
] | 3 | [
"10.3847/0004-637X/829/1/45",
"10.48550/arXiv.1607.03570"
] | [
"Kim, Woong-Tae",
"Moon, Sanghyuk"
] | [
"Center for the Exploration of the Origin of the universe (CEOU), Department of Physics & Astronomy, Seoul National University, Seoul 151-742, Korea ; Center for Theoretical Physics (CTP), Seoul National University, Seoul 151-742, Korea",
"Center for the Exploration of the Origin of the universe (CEOU), Depar... | [
"2018MNRAS.475...63H",
"2019ApJS..241...24M",
"2021MNRAS.505.4310C"
] | [
"1953mtp..book.....M",
"1964ApJ...140.1056O",
"1964ApJ...140.1067O",
"1965MNRAS.130...97G",
"1967ApJ...147..334C",
"1968ApJ...151.1075O",
"1971ApJ...167..425B",
"1981PThPh..65.1870E",
"1985A&A...150..327C",
"1986ApJS...61..479H",
"1986ApJS...61..609B",
"1986ApJS...62..461H",
"1987PThPh..77..... |
12464733 | 1607.02606 | No need for dark matter in galaxy clusters within Galileon theory | Modified gravity theories with a screening mechanism have acquired much interest recently in the quest for a viable alternative to General Relativity on cosmological scales, given their intrinsic property of being able to pass Solar System scale tests and, at the same time, to possibly drive universe acceleration on mu... | [
0.00040361020364798605,
0.04387258365750313,
-0.015943387523293495,
-0.008317196741700172,
-0.024449041113257408,
0.002619540086016059,
-0.0008928108727559447,
-0.026408985257148743,
-0.040304481983184814,
0.024700315669178963,
-0.046812500804662704,
-0.0005029422463849187,
-0.05613479763269... | 10.367568 | 1.388186 | 2016-07-01 | 15 | 2016JCAP...10..033S | [
"general relativity",
"Solar System scale tests",
"cosmological scales",
"X-ray intra-cluster hot gas observations",
"Dark Matter",
"gravitational lensing events",
"observations",
"covariant Galileon models",
"clusters",
"Solar System",
"archival data",
"universe acceleration",
"the general ... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 3 | [
"10.1088/1475-7516/2016/10/033",
"10.48550/arXiv.1607.02606"
] | [
"Salzano, Vincenzo",
"Mota, David F.",
"Dabrowski, Mariusz P.",
"Capozziello, Salvatore"
] | [
"Institute of Physics, University of Szczecin, Wielkopolska 15, 70-451 Szczecin, Poland",
"Institute of Theoretical Astrophysics, University of Oslo, 0315 Oslo, Norway",
"Institute of Physics, University of Szczecin, Wielkopolska 15, 70-451 Szczecin, Poland; National Centre for Nuclear Research, Andrzeja Sołtan... | [
"2018ApJ...856..177C",
"2018EPJC...78..447C",
"2018IJMPD..2730003M",
"2018PDU....19..137H",
"2019arXiv190708010V",
"2020EPJC...80...24G",
"2020PhRvD.102j4063G",
"2021EPJP..136..235G",
"2021MNRAS.506..595P",
"2021arXiv210512582S",
"2022EPJC...82..652B",
"2022MNRAS.511.1878L",
"2022PhRvD.105l4... | [
"1972PhLB...39..393V",
"1974IJTP...10..363H",
"1978A&A....70..677C",
"1996ApJ...462..563N",
"2005MNRAS.358..601C",
"2006ApJ...638L..51M",
"2007PhRvD..75f3501M",
"2007PhRvD..75f3508B",
"2008GReGr..40..357C",
"2009PhRvD..79f4036N",
"2009PhRvD..79h4003D",
"2009arXiv0912.0914L",
"2010PhLB..694..... |
2073358 | 1607.07679 | Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71 | The determination of the thermodynamic properties of clusters of galaxies at intermediate and high redshift can bring new insights into the formation of large-scale structures. It is essential for a robust calibration of the mass-observable scaling relations and their scatter, which are key ingredients for precise cosm... | [
0.00045346442493610084,
0.002075859345495701,
-0.015130983665585518,
-0.010287828743457794,
0.0004154819471295923,
0.007001180667430162,
-0.006616704631596804,
0.021939925849437714,
-0.007683315314352512,
-0.01836802251636982,
0.0036153129767626524,
0.02414756268262863,
-0.07729203999042511,... | 10.628067 | 3.366452 | 2016-07-01 | 36 | 2017A&A...597A.110R | [
"intermediate redshift",
"cluster statistics",
"clusters",
"R",
"similar angular resolution",
"X-ray observations",
"new insights",
"large program",
"intermediate and high redshift",
"intermediate and high redshifts",
"PSZ1 G045.85",
"SZ-discovered clusters",
"R 0.02 R",
"data",
"the clu... | [
"galaxies: clusters: intracluster medium",
"instrumentation: high angular resolution",
"cosmology: observations",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 39 | [
"10.1051/0004-6361/201629405",
"10.48550/arXiv.1607.07679"
] | [
"Ruppin, F.",
"Adam, R.",
"Comis, B.",
"Ade, P.",
"André, P.",
"Arnaud, M.",
"Beelen, A.",
"Benoît, A.",
"Bideaud, A.",
"Billot, N.",
"Bourrion, O.",
"Calvo, M.",
"Catalano, A.",
"Coiffard, G.",
"D'Addabbo, A.",
"De Petris, M.",
"Désert, F. -X.",
"Doyle, S.",
"Goupy, J.",
"Kram... | [
"Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble Alpes, CNRS/IN2P3, 53 avenue des Martyrs, Grenoble, France",
"Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble Alpes, CNRS/IN2P3, 53 avenue des Martyrs, Grenoble, France; Laboratoire Lagrange, Université Côte d'Azu... | [
"2016sf2a.conf..439D",
"2017A&A...606A..64A",
"2017AN....338..305P",
"2017arXiv170506064P",
"2017arXiv170901255M",
"2017ehep.confE..42M",
"2018A&A...612A..39R",
"2018A&A...614A.118A",
"2018A&A...615A..18R",
"2018A&A...615A.112R",
"2018MNRAS.481..749S",
"2018arXiv180810817P",
"2019A&A...621A.... | [
"1956ZhETF..31..876K",
"1972CoASP...4..173S",
"1979AJ.....84..942W",
"1980ARA&A..18..537S",
"1992StaSc...7..457G",
"1995ApJ...450..559B",
"1998AJ....115.1693C",
"1998ApJ...502....7I",
"1999PhR...310...97B",
"2002ARA&A..40..643C",
"2004ApJ...601..599L",
"2004MNRAS.348.1401D",
"2004MNRAS.354..... |
12509796 | 1607.00745 | Results of an all-sky high-frequency Einstein@Home search for continuous gravitational waves in LIGO's fifth science run | We present results of a high-frequency all-sky search for continuous gravitational waves from isolated compact objects in LIGO's fifth science run (S5) data, using the computing power of the Einstein@Home volunteer computing project. This is the only dedicated continuous gravitational wave search that probes this high-... | [
0.016191694885492325,
0.05233548581600189,
-0.0011718949535861611,
-0.00509786419570446,
0.003624717006459832,
-0.004487283527851105,
-0.009633606299757957,
-0.00836721621453762,
-0.01197901088744402,
-0.013516769744455814,
-0.010008353739976883,
-0.0039865425787866116,
-0.05665154755115509,... | 7.113799 | 2.266396 | 2016-07-01 | 13 | 2016PhRvD..94f4061S | [
"continuous gravitational wave strain amplitudes",
"continuous gravitational waves",
"the Einstein@Home volunteer computing project",
"S5 data",
"isolated compact objects",
"rotation periods",
"objects",
"the only dedicated continuous gravitational wave search",
"90% confidence level upper limits",
... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 12 | [
"10.1103/PhysRevD.94.064061",
"10.48550/arXiv.1607.00745"
] | [
"Singh, Avneet",
"Papa, Maria Alessandra",
"Eggenstein, Heinz-Bernd",
"Zhu, Sylvia",
"Pletsch, Holger",
"Allen, Bruce",
"Bock, Oliver",
"Maschenchalk, Bernd",
"Prix, Reinhard",
"Siemens, Xavier"
] | [
"Max-Planck-Institut für Gravitationsphysik, am Mühlenberg 1, 14476 Potsdam-Golm, Germany; Max-Planck-Institut für Gravitationsphysik, Callinstraße 38, 30167 Hannover, Germany; Leibniz Universität Hannover, Welfengarten 1, 30167 Hannover, Germany",
"Max-Planck-Institut für Gravitationsphysik, am Mühlenberg 1, 144... | [
"2016PhRvD..94h2008Z",
"2016PhRvD..94j2002A",
"2016PhRvD..94l2006P",
"2017PhRvD..96h2003S",
"2017PhRvD..96l2004A",
"2017PhRvD..96l4007Z",
"2018PhRvD..97j2003A",
"2018PhRvD..98h4058D",
"2019PhRvD..99d4006S",
"2021ApJ...909...79S",
"2023APh...15302880W",
"2023PhRvD.107f2005M",
"2023PhRvD.108l2... | [
"2005PhRvD..72f3006C",
"2007PhRvD..76h2001A",
"2008PhRvD..77b2001A",
"2008PhRvD..78j2005P",
"2009PhRvL.102k1102A",
"2009RPPh...72g6901A",
"2010NIMPA.624..223A",
"2010PhRvD..82d2002P",
"2011PhRvD..84b3007P",
"2012PhRvD..85b2001A",
"2012PhRvD..85d2003W",
"2013PhRvD..87d2001A",
"2013PhRvD..88d4... |
12517024 | 1607.00059 | HI absorption spectra for supernova remnants in the VGPS survey | The set of supernova remnants (SNR) from Green's SNR catalog which are found in the VLA Galactic Plane Survey are studied here. For this set of 34 SNR, we extract and analyze HI absorption spectra in a uniform way and construct a catalog of absorption spectra and distance determinations. The results of this work will b... | [
-0.026023324579000473,
0.029287898913025856,
0.03884844109416008,
-0.03674978390336037,
-0.023598210886120796,
-0.032529156655073166,
-0.036330051720142365,
-0.07014171779155731,
0.032995522022247314,
-0.021336328238248825,
-0.03208610787987709,
0.020660094916820526,
-0.0435587540268898,
-... | 4.064715 | 5.117086 | 2016-07-01 | 0 | 2016sros.confE..86L | [
"HI absorption spectra",
"absorption spectra and distance determinations",
"the VLA Galactic Plane Survey",
"SNR",
"Greens SNR catalog",
"supernova remnants",
"Green",
"a uniform way",
"a catalog",
"34 SNR",
"this work",
"The results",
"The set",
"this set",
"34",
"we",
"which"
] | [
"Astrophysics - Astrophysics of Galaxies"
] | 2 | [
"10.48550/arXiv.1607.00059"
] | [
"Leahy, D.",
"Ranasinghe, S."
] | [
"University of Calgary, Canada;",
"-"
] | null | null |
2323953 | 1607.06096 | The missing magnetic morphology term in stellar rotation evolution | <BR /> Aims: This study examines the relationship between magnetic field complexity and mass and angular momentum losses. Observations of open clusters have revealed a bimodal distribution of the rotation periods of solar-like stars that has proven difficult to explain under the existing rubric of magnetic braking. Rec... | [
0.029225660488009453,
0.04416952654719353,
0.012295585125684738,
-0.010001986287534237,
0.007732031401246786,
0.05116855353116989,
0.02906014397740364,
-0.009109373204410076,
0.007318237796425819,
0.002457639202475548,
-0.023349789902567863,
0.015274900011718273,
-0.032086748629808426,
-0.... | 8.665624 | 12.045554 | 2016-07-01 | 66 | 2016A&A...595A.110G | [
"Angular momentum loss rates",
"angular momentum loss",
"Magnetic field complexity",
"magnetic field complexity",
"angular momentum",
"magnetic complexity",
"mass and angular momentum loss rates",
"geometrical complexity",
"losses",
"complexity",
"stellar rotation evolution models",
"observed ... | [
"magnetic fields",
"magnetohydrodynamics (MHD)",
"stars: activity",
"stars: rotation",
"Astrophysics - Solar and Stellar Astrophysics"
] | 10 | [
"10.1051/0004-6361/201628367",
"10.48550/arXiv.1607.06096"
] | [
"Garraffo, Cecilia",
"Drake, Jeremy J.",
"Cohen, Ofer"
] | [
"Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA, 02138, USA",
"Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA, 02138, USA",
"Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA, 02138, USA"
] | [
"2016ApJ...832...97S",
"2017ApJ...845...46F",
"2017ApJ...849...83P",
"2017ApJ...850...45R",
"2017IAUS..328..315A",
"2017MNRAS.472..876O",
"2017SoPh..292..126M",
"2018ApJ...854...78F",
"2018ApJ...856...53P",
"2018ApJ...862...90G",
"2018ApJ...862...93A",
"2018ApJ...864..125F",
"2018ApJ...868..... | [
"1962AnAp...25...18S",
"1967ApJ...148..217W",
"1967ApJ...150..551K",
"1968MNRAS.138..359M",
"1969SoPh....9..131A",
"1981ApJ...243..625E",
"1984A&A...136...98M",
"1984ApJ...280..202S",
"1987ApJ...318..337S",
"1988ApJ...333..236K",
"1993ApJ...409..624S",
"1995GeoRL..22.3301P",
"1998A&A...335..... |
12594325 | 1607.08797 | Concordance cosmology without dark energy | According to the separate universe conjecture, spherically symmetric sub-regions in an isotropic universe behave like mini-universes with their own cosmological parameters. This is an excellent approximation in both Newtonian and general relativistic theories. We estimate local expansion rates for a large number of suc... | [
0.010449189692735672,
-0.005044654011726379,
0.03305858373641968,
-0.011364677920937538,
-0.02169390767812729,
0.014281611889600754,
-0.007961587980389595,
0.0020124949514865875,
-0.03290705755352974,
0.048135723918676376,
-0.04275644198060036,
0.01649140939116478,
-0.04740333557128906,
0.... | 11.081444 | 0.903728 | 2016-07-01 | 48 | 2017MNRAS.469L...1R | [
"local scale parameters",
"cosmic microwave background observations",
"local expansion rates",
"future precision observations",
"non-linear evolution",
"such regions",
"local Hubble constant measurements",
"full consistency",
"structure",
"boundary effects",
"light propagation",
"regions",
"... | [
"methods: numerical",
"cosmological parameters",
"dark energy",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 12 | [
"10.1093/mnrasl/slx026",
"10.48550/arXiv.1607.08797"
] | [
"Rácz, Gábor",
"Dobos, László",
"Beck, Róbert",
"Szapudi, István",
"Csabai, István"
] | [
"Department of Physics of Complex Systems, Eötvös Loránd University, Pf. 32, H-1518 Budapest, Hungary",
"Department of Physics of Complex Systems, Eötvös Loránd University, Pf. 32, H-1518 Budapest, Hungary",
"Department of Physics of Complex Systems, Eötvös Loránd University, Pf. 32, H-1518 Budapest, Hungary",
... | [
"2016arXiv161207245C",
"2017A&A...598A.111R",
"2017ApJ...841...63T",
"2017CQGra..34w7001D",
"2017JCAP...02..047S",
"2017JCAP...06..025B",
"2017JCAP...12..008M",
"2017MNRAS.469..744K",
"2017MNRAS.470.4493W",
"2017PhRvD..95l4009F",
"2018A&A...610A..51R",
"2018CQGra..35b4003B",
"2018MNRAS.473L.... | [
"1994ApJ...427...51B",
"1998AJ....116.1009R",
"1999ApJ...517..565P",
"2000A&A...363L..29S",
"2000GReGr..32..105B",
"2001GReGr..33.1381B",
"2005MNRAS.364.1105S",
"2005PhRvD..71b3524K",
"2006MNRAS.365..939M",
"2006MNRAS.373..369C",
"2007NJPh....9..377W",
"2007PhRvL..99y1101W",
"2008cosm.book..... |
12408779 | 1607.05789 | The X-Ray Luminosity Function of M37 and the Evolution of Coronal Activity in Low-mass Stars | We use a 440.5 ks Chandra observation of the ≈500 Myr old open cluster M37 to derive the X-ray luminosity functions of its ≤1.2 {M}<SUB>⊙ </SUB> stars. Combining detections of 162 M37 members with upper limits for 160 non-detections, we find that its G, K, and M stars have a similar median (0.5-7 keV) X-ray luminosity ... | [
0.020198477432131767,
0.051829151809215546,
0.007523392792791128,
-0.02709141932427883,
0.053318217396736145,
0.036458130925893784,
0.04767417162656784,
-0.03636206313967705,
0.027163470163941383,
-0.002640392631292343,
-0.020138435065746307,
-0.003401438007131219,
-0.0742131918668747,
-0.... | 8.497781 | 12.220102 | 2016-07-01 | 13 | 2016ApJ...830...44N | [
"K stars",
"G stars",
"M stars",
"stars",
"G and K stars X-ray activity",
"NGC",
"-0.68 ±",
"±",
"-",
"Myr",
"the X-ray luminosity functions",
"X",
"low-mass stars",
"≈",
"the ≈500 Myr old open cluster M37",
"K",
"magnetic activity",
"activity",
"G",
"magnitude"
] | [
"open clusters and associations: individual: M37",
"stars: activity",
"stars: coronae",
"stars: low-mass",
"X-rays: individual: M37",
"Astrophysics - Solar and Stellar Astrophysics"
] | 11 | [
"10.3847/0004-637X/830/1/44",
"10.48550/arXiv.1607.05789"
] | [
"Núñez, Alejandro",
"Agüeros, Marcel A."
] | [
"Department of Astronomy, Columbia University, 550 West 120th Street, New York, NY 10027, USA",
"Department of Astronomy, Columbia University, 550 West 120th Street, New York, NY 10027, USA"
] | [
"2017ApJ...834..176N",
"2018A&A...615A...2C",
"2018ApJ...862...33A",
"2018ApJ...863...91F",
"2018PhDT........75N",
"2020ApJ...898..104E",
"2021A&A...649A..96J",
"2021A&A...653A..49B",
"2021A&A...654A.134C",
"2022MNRAS.512...41K",
"2024ApJ...960...62E",
"2024ApJ...961...26R",
"2024arXiv240613... | [
"1978ApJ...224..132B",
"1981ApJ...248..279P",
"1987ApJ...315..687M",
"1988ApJ...333..236K",
"1989A&A...213L...1M",
"1989A&AS...78...25D",
"1989NASSP.502..139C",
"1990ApJ...365..704S",
"1993A&AS...98..477M",
"1993MNRAS.263..647S",
"1994ApJS...91..625S",
"1995A&A...293..889P",
"1995AJ....110.1... |
12510330 | 1607.02356 | Post-Newtonian parameter γ for multiscalar-tensor gravity with a general potential | We compute the parametrized post-Newtonian parameter γ in the case of a static point source for multiscalar-tensor gravity with completely general nonderivative couplings and potential in the Jordan frame. Similarly to the single massive field case γ depends exponentially on the distance from the source and is determin... | [
-0.013188961893320084,
0.024904431775212288,
0.025073520839214325,
-0.014046486467123032,
-0.021727969869971275,
-0.05053353309631348,
0.025749878957867622,
-0.01677606999874115,
-0.002599747385829687,
-0.009493154473602772,
-0.06174173578619957,
0.009082508273422718,
-0.0427795834839344,
... | 10.225882 | 1.09362 | 2016-07-01 | 30 | 2016PhRvD..94l4015H | [
"scalar fields",
"nonminimal coupling",
"general hybrid metric-Palatini gravity",
"completely general nonderivative couplings",
"multiscalar-tensor gravity",
"Jordan",
"linear",
"γ",
"potential",
"two scalar fields",
"the single massive field case",
"the mass eigenvectors",
"the Jordan frame... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Phenomenology",
"High Energy Physics - Theory"
] | 3 | [
"10.1103/PhysRevD.94.124015",
"10.48550/arXiv.1607.02356"
] | [
"Hohmann, Manuel",
"Järv, Laur",
"Kuusk, Piret",
"Randla, Erik",
"Vilson, Ott"
] | [
"Institute of Physics, University of Tartu, W. Ostwaldi 1, Tartu 50411, Estonia",
"Institute of Physics, University of Tartu, W. Ostwaldi 1, Tartu 50411, Estonia",
"Institute of Physics, University of Tartu, W. Ostwaldi 1, Tartu 50411, Estonia",
"Institute of Physics, University of Tartu, W. Ostwaldi 1, Tartu... | [
"2016arXiv160903159C",
"2017PhRvD..95h4050P",
"2017PhRvD..96j4026H",
"2017PhRvL.118o1302J",
"2017SCPMA..60j0411Z",
"2017Univ....3...37J",
"2018JCAP...06..032C",
"2018NuPhB.927..219K",
"2018PDU....22..101S",
"2018PhRvD..97j4011H",
"2018PhRvD..98f4004H",
"2019EPJP..134..318L",
"2019IJMPD..2850... | [
"1970ApJ...161.1059N",
"1978GReGr...9..353S",
"1983JMP....24.2793T",
"1984PhLB..145..176W",
"1989PhRvD..39.3159M",
"1990CQGra...7..557M",
"1990CQGra...7..893G",
"1990CQGra...7.1023S",
"1992CQGra...9.2093D",
"1993tegp.book.....W",
"1994CQGra..11..269W",
"1994PhRvD..49.6442B",
"1996PhRvD..53.5... |
12473477 | 1607.05576 | The freedom to choose neutron star magnetic field equilibria: Table 1. | Our ability to interpret and glean useful information from the large body of observations of strongly magnetized neutron stars rests largely on our theoretical understanding of magnetic field equilibria. We answer the following question: is one free to arbitrarily prescribe magnetic equilibria such that fluid degrees o... | [
-0.0016572519671171904,
-0.0009663368691690266,
0.014000867493450642,
-0.018407614901661873,
0.01697227545082569,
-0.02505550906062126,
-0.010607671923935413,
-0.016947094351053238,
-0.022801773622632027,
-0.02044731006026268,
0.003962925635278225,
-0.007869192399084568,
-0.02792619168758392... | 5.332808 | 2.90859 | 2016-07-01 | 13 | 2016MNRAS.463.2542G | [
"non-axisymmetric equilibria",
"magnetic field equilibria",
"magnetic equilibria",
"general relativity",
"a magnetic field equilibrium",
"complete freedom",
"more realistic non-barotropic multifluid models",
"Newtonian gravity",
"entropy",
"freedom",
"both axi- and non-axisymmetric equilibria",
... | [
"stars: magnetic field",
"stars: neutron",
"Astrophysics - Solar and Stellar Astrophysics"
] | 1 | [
"10.1093/mnras/stw2115",
"10.48550/arXiv.1607.05576"
] | [
"Glampedakis, Kostas",
"Lasky, Paul D."
] | [
"Departamento de Física, Universidad de Murcia, Murcia, E-30100, Spain; Theoretical Astrophysics, University of Tübingen, Auf der Morgenstelle 10, Tübingen, D-72076, Germany",
"Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University, VIC 3800, Australia"
] | [
"2017PhRvD..96j3012G",
"2018MNRAS.473.4272K",
"2019MNRAS.489.4261M",
"2020MNRAS.495.1360S",
"2021MNRAS.503..875L",
"2021MNRAS.503.2764F",
"2021MNRAS.506.2985K",
"2022ASSL..465..245D",
"2022ApJ...928...53W",
"2022pas..conf..231S",
"2023MNRAS.519.1080G",
"2023MNRAS.523.4089S",
"2023PhRvD.108h4... | [
"1988ApJ...325..725M",
"1992ApJ...395..240R",
"2002A&A...393..949P",
"2004PhRvD..69d3001P",
"2007A&A...469..275B",
"2007A&A...470..303P",
"2007Ap&SS.308..181H",
"2007LRR....10....1A",
"2008JFM...607..235Y",
"2008MNRAS.385..531H",
"2008MNRAS.385.2080C",
"2009A&A...499..557R",
"2009MNRAS.397..... |
12516965 | 1607.05754 | Mechanical designs and development of TES bolometer detector arrays for the Advanced ACTPol experiment | The next generation Advanced ACTPol (AdvACT) experiment is currently underway and will consist of four Transition Edge Sensor (TES) bolometer arrays, with three operating together, totaling 5800 detectors on the sky. Building on experience gained with the ACTPol detector arrays, AdvACT will utilize various new technolo... | [
0.012005939148366451,
-0.012976692989468575,
0.028651509433984756,
0.013690482825040817,
-0.011677595786750317,
0.040343381464481354,
0.00533200753852725,
-0.027580825611948967,
0.012005939148366451,
-0.022684229537844658,
0.04959409311413765,
-0.05259200930595398,
0.010813910514116287,
-0... | 10.630923 | 2.914708 | 2016-07-01 | 5 | 2016SPIE.9914E..37W | [
"detectors",
"multichroic pixels",
"cryogenic readout electronics",
"the detector array stack assemblies",
"HF) detector array package",
"the detector array assembly",
"AdvACT",
"pre-existing ACTPol infrastructure",
"various new technologies",
"back short cavity plate",
"the ACTPol detector arra... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 5 | [
"10.1117/12.2233746",
"10.48550/arXiv.1607.05754"
] | [
"Ward, Jonathan T.",
"Austermann, Jason",
"Beall, James A.",
"Choi, Steve K.",
"Crowley, Kevin T.",
"Devlin, Mark J.",
"Duff, Shannon M.",
"Gallardo, Patricio A.",
"Henderson, Shawn W.",
"Ho, Shuay-Pwu Patty",
"Hilton, Gene",
"Hubmayr, Johannes",
"Khavari, Niloufar",
"Klein, Jeffrey",
"K... | [
"Univ. of Pennsylvania (United States)",
"NIST Quantum Devices Group (United States)",
"NIST Quantum Devices Group (United States)",
"Princeton Univ. (United States)",
"Princeton Univ. (United States)",
"Univ. of Pennsylvania (United States)",
"NIST Quantum Devices Group (United States)",
"Cornell Uni... | [
"2018JLTP..193..288V",
"2019BAAS...51c..37K",
"2019BAAS...51c..51K",
"2019arXiv190704473A",
"2022SPIE12190E..1KH"
] | [
"2010ApJ...722.1148F"
] |
12472651 | 1607.05612 | Searching in the dark: the dark mass content of the Milky Way globular clusters NGC288 and NGC6218 | We present an observational estimate of the fraction and distribution of dark mass in the innermost region of the two Galactic globular clusters NGC 6218 (M12) and NGC 288. Such an assessment has been made by comparing the dynamical and luminous mass profiles derived from an accurate analysis of the most extensive spec... | [
0.011415462009608746,
0.01818392239511013,
0.023092392832040787,
-0.00845611747354269,
0.012033477425575256,
0.009103845804929733,
0.03068685345351696,
0.010363646782934666,
-0.006465394515544176,
0.017447056248784065,
-0.006010796409100294,
0.002791469683870673,
-0.04554300010204315,
-0.0... | 9.99544 | 7.47804 | 2016-07-01 | 22 | 2016MNRAS.462.1937S | [
"M12",
"NGC 288",
"dark mass",
"tidal heating",
"dark remnants",
"non-luminous matter",
"the cluster core",
"lt",
"binaries",
"R",
"Galactic",
"these stellar systems",
"both clusters",
"the two Galactic globular clusters",
"distribution",
"a spurious consequence",
"the total mass",
... | [
"methods: data analysis",
"techniques: radial velocities",
"stars: kinematics and dynamics",
"stars: luminosity function",
"mass function",
"stars: Population II",
"globular clusters: individual: NGC6218",
"NGC288",
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Astrophysics of G... | 2 | [
"10.1093/mnras/stw1779",
"10.48550/arXiv.1607.05612"
] | [
"Sollima, A.",
"Ferraro, F. R.",
"Lovisi, L.",
"Contenta, F.",
"Vesperini, E.",
"Origlia, L.",
"Lapenna, E.",
"Lanzoni, B.",
"Mucciarelli, A.",
"Dalessandro, E.",
"Pallanca, C."
] | [
"INAF Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, Italy; Dipartimento di Astronomia, Universitá di Bologna, via Ranzani 1, I-40127 Bologna, Italy",
"Dipartimento di Astronomia, Universitá di Bologna, via Ranzani 1, I-40127 Bologna, Italy",
"Dipartimento di Astronomia, Universitá di Bolo... | [
"2016MmSAI..87..614S",
"2017ApJ...849..108G",
"2017JCAP...04..036D",
"2017MNRAS.464.2930H",
"2017MNRAS.467..412P",
"2017MNRAS.467..524B",
"2017PhRvD..96f3001G",
"2018ApJ...860...50F",
"2018MNRAS.473..909B",
"2018RAA....18..126S",
"2019MNRAS.483.1400H",
"2019MNRAS.484L.114K",
"2019MNRAS.485.5... | [
"1916MNRAS..76..572E",
"1966AJ.....71...64K",
"1969ApJ...158L.139S",
"1975ApJ...199L.143C",
"1978MNRAS.183..341W",
"1979AJ.....84..752G",
"1979PAZh....5...77O",
"1984ApJ...277..470P",
"1984sv...bookR....F",
"1985AJ.....90.1027M",
"1988Natur.336...48G",
"1989ApJ...339..178R",
"1991A&A...250..... |
12593492 | 1607.01800 | A statistical investigation of the mass discrepancy-acceleration relation | We use the mass discrepancy-acceleration relation (the correlation between the ratio of total-to-visible mass and acceleration in galaxies; MDAR) to test the galaxy-halo connection. We analyse the MDAR using a set of 16 statistics that quantify its four most important features: shape, scatter, the presence of a `charac... | [
0.03672776371240616,
0.03404159098863602,
0.015351352281868458,
0.011234227567911148,
0.026510266587138176,
0.059095799922943115,
0.012778148986399174,
-0.01905425451695919,
-0.01424675714224577,
0.038234028965234756,
-0.04842642322182655,
-0.03218386322259903,
-0.031305208802223206,
0.007... | 10.170216 | 2.174805 | 2016-07-01 | 86 | 2017MNRAS.464.4160D | [
"halo mass",
"galaxy kinematics",
"galaxy size",
"other galaxy properties",
"specific galaxy formation models",
"galaxies",
"fixed stellar mass",
"low acceleration",
"acceleration",
"halo abundance matching",
"AM mocks",
"MDAR",
"AM",
"conventional correlations",
"relations",
"concrete... | [
"galaxies: formation",
"galaxies: fundamental parameters",
"galaxies: haloes",
"galaxies: kinematics and dynamics",
"dark matter",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 5 | [
"10.1093/mnras/stw2571",
"10.48550/arXiv.1607.01800"
] | [
"Desmond, Harry"
] | [
"Kavli Institute for Particle Astrophysics and Cosmology and Physics Department, Stanford University, Stanford, CA 94305, USA; SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA"
] | [
"2016PhRvL.117t1101M",
"2016arXiv160906642M",
"2017A&A...603A..11P",
"2017A&A...603A..65T",
"2017A&A...607A.108H",
"2017ApJ...836..152L",
"2017ApJ...837..179D",
"2017IJMPD..2650118C",
"2017MNRAS.469.1630H",
"2017MNRAS.471.1841N",
"2017MNRAS.471L..11D",
"2017MNRAS.472..765T",
"2017MNRAS.472L.... | [
"1983ApJ...270..365M",
"1983ApJ...270..371M",
"1983ApJ...270..384M",
"1986ApJ...301...27B",
"1990A&ARv...2....1S",
"1998ApJ...499...41M",
"1998MNRAS.295..319M",
"1999ASPC..182..528M",
"1999ApJ...522...82K",
"1999MNRAS.310.1147M",
"2000ApJ...534..146V",
"2003MNRAS.341.1109B",
"2004ApJ...609..... |
5251088 | 1607.03034 | Observing—and Imaging—Active Galactic Nuclei with the Event Horizon Telescope | Originally developed to image the shadow region of the central black hole in Sagittarius A* and in the nearby galaxy M87, the Event Horizon Telescope (EHT) provides deep, very high angular resolution data on other active galactic nucleus (AGN) sources too. The challenges of working with EHT data have spurred the develo... | [
-0.056411925703287125,
-0.005315972957760096,
0.03019983321428299,
-0.00866847112774849,
-0.0570441298186779,
0.03447935730218887,
-0.009130464866757393,
0.04537269473075867,
-0.02881385013461113,
-0.031780339777469635,
0.02776828408241272,
-0.018844502046704292,
-0.0540776401758194,
-0.02... | 8.905908 | 3.682015 | 2016-07-01 | 60 | 2016Galax...4...54F | [
"other active galactic nucleus",
"other wavelengths",
"AGN sources",
"novel imaging techniques",
"better reconstructions",
"EHT data",
"sources",
"AGN",
"emphasis",
"EHT",
"Sagittarius A",
"M87",
"the Event Horizon Telescope",
"deep, very high angular resolution data",
"the central black... | [
"galaxies: jets",
"galaxy: center",
"techniques: high angular resolution",
"techniques: image processing",
"techniques: interferometric",
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 12 | [
"10.3390/galaxies4040054",
"10.48550/arXiv.1607.03034"
] | [
"Fish, Vincent L.",
"Akiyama, Kazunori",
"Bouman, Katherine L.",
"Chael, Andrew A.",
"Johnson, Michael D.",
"Doeleman, Sheperd S.",
"Blackburn, Lindy",
"Wardle, John F. C.",
"Freeman, William T.",
"the Event Horizon Telescope Collaboration"
] | [
"Massachusetts Institute of Technology, Haystack Observatory, Westford, MA 01886, USA",
"Massachusetts Institute of Technology, Haystack Observatory, Westford, MA 01886, USA; Japan Society for the Promotion of Science, Chiyoda (Tokyo) 102-0083, Japan",
"Massachusetts Institute of Technology, Computer Science an... | [
"2017A&A...601A..52B",
"2017A&ARv..25....2P",
"2017A&ARv..25....4B",
"2017ApJ...850..172J",
"2017CaJPh..95.1299M",
"2017JETPL.106..637D",
"2017JPhCS.934a2044D",
"2017arXiv170504776A",
"2018A&A...613A...2B",
"2018AJ....156...15M",
"2018PhLB..781..651D",
"2018PhRvD..97f4021T",
"2018PhRvD..97f4... | [
"1958MNRAS.118..276J",
"1974A&AS...15..417H",
"1974ApJ...193..293R",
"1980A&A....89..377C",
"1984AJ.....89.1076S",
"1985A&A...143...77C",
"1986ARA&A..24..127N",
"1990SPIE.1351..714H",
"1994A&AS..108..585S",
"1994ApJ...427..718R",
"1994IAUS..158...91B",
"2004SPIE.5491..886L",
"2005AJ....130.1... |
12619768 | 1607.04278 | Dark gamma-ray bursts | Many theories of dark matter (DM) predict that DM particles can be captured by stars via scattering on ordinary matter. They subsequently condense into a DM core close to the center of the star and eventually annihilate. In this work, we trace DM capture and annihilation rates throughout the life of a massive star and ... | [
0.0012201586505398154,
0.04495353624224663,
-0.014057212509214878,
0.01146610639989376,
-0.0564257986843586,
0.03658321872353554,
0.04121151193976402,
0.0057607488706707954,
-0.006382368039339781,
0.0074471221305429935,
0.010001299902796745,
0.04894174635410309,
-0.055441051721572876,
-0.0... | 8.148736 | -1.078547 | 2016-07-01 | 10 | 2017PhRvD..95e5031B | [
"DM annihilation",
"DM particles",
"more DM particles",
"DM",
"DM capture",
"s -wave annihilation",
"annihilation rates",
"gamma rays",
"standard model particles",
"dark matter",
"stars",
"ordinary matter",
"particles",
"stellar evolution",
"the DM annihilation products",
"dark photons... | [
"High Energy Physics - Phenomenology",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 8 | [
"10.1103/PhysRevD.95.055031",
"10.48550/arXiv.1607.04278"
] | [
"Brdar, Vedran",
"Kopp, Joachim",
"Liu, Jia"
] | [
"PRISMA Cluster of Excellence and Mainz Institute for Theoretical Physics, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany",
"PRISMA Cluster of Excellence and Mainz Institute for Theoretical Physics, Johannes Gutenberg-Universität Mainz, 55099 Mainz, Germany",
"PRISMA Cluster of Excellence and Mainz ... | [
"2017JCAP...02..042H",
"2017PhRvD..95g5001A",
"2018JCAP...04..025B",
"2019JCAP...11..011N",
"2021MNRAS.503..458H",
"2022JCAP...05..042G",
"2022JHEP...10..186L",
"2023PhRvD.107k5016N",
"2024EPJC...84..136L",
"2024arXiv240201839L"
] | [
"1931AnP...403..257S",
"1965TrAlm...5...87E",
"1985ApJ...299.1001K",
"1985PhRvL..55..257S",
"1987ApJ...321..560G",
"1987ApJ...321..571G",
"1987NuPhB.279..804S",
"1990ApJ...356..302G",
"1996PhR...267..195J",
"1998ASPC..131...76L",
"2003JHEP...05..067B",
"2003PhRvL..90v5002K",
"2004PhRvD..69j1... |
2878662 | 1607.06561 | LZIFU: an emission-line fitting toolkit for integral field spectroscopy data | We present lzifu (LaZy-IFU), an idl toolkit for fitting multiple emission lines simultaneously in integral field spectroscopy (IFS) data. lzifu is useful for the investigation of the dynamical, physical and chemical properties of gas in galaxies. lzifu has already been applied to many world-class IFS instruments and la... | [
-0.029873691499233246,
0.041172076016664505,
0.010703371837735176,
-0.010033128783106804,
0.014444421976804733,
-0.03392250835895538,
-0.022788263857364655,
0.021693989634513855,
-0.0074684228748083115,
0.03933916613459587,
0.01821966841816902,
-0.020859606564044952,
-0.02308919094502926,
... | 11.932857 | 6.765119 | 2016-07-01 | 90 | 2016Ap&SS.361..280H | [
"emission line",
"fitting multiple emission lines",
"IFS data",
"large IFS surveys",
"multiple distinct kinematic components",
"other IFS instruments",
"integral field",
"IFS",
"kinematic maps",
"Multi Unit Spectroscopic Explorer",
"flux uncertainties",
"complex, skewed line profiles",
"SAMI... | [
"Integral field spectroscopy",
"Data analysis",
"Emission line fitting",
"Astrophysics - Astrophysics of Galaxies"
] | 16 | [
"10.1007/s10509-016-2865-2",
"10.48550/arXiv.1607.06561"
] | [
"Ho, I. -Ting",
"Medling, Anne M.",
"Groves, Brent",
"Rich, Jeffrey A.",
"Rupke, David S. N.",
"Hampton, Elise",
"Kewley, Lisa J.",
"Bland-Hawthorn, Joss",
"Croom, Scott M.",
"Richards, Samuel",
"Schaefer, Adam L.",
"Sharp, Rob",
"Sweet, Sarah M."
] | [
"Institute for Astronomy, University of Hawaii, Honolulu, HI, USA; Research School of Astronomy and Astrophysics, Australian National University, Weston, ACT, Australia",
"Research School of Astronomy and Astrophysics, Australian National University, Weston, ACT, Australia",
"Research School of Astronomy and As... | [
"2016ApJ...827..103K",
"2016MNRAS.462.1616D",
"2016MNRAS.463..170C",
"2017A&A...601A..61V",
"2017ApJ...834..174K",
"2017ApJ...846...39H",
"2017ApJS..232...11T",
"2017MNRAS.464..121S",
"2017MNRAS.468.3965F",
"2017MNRAS.470.1991B",
"2017MNRAS.470.3395H",
"2017MNRAS.470.4573Z",
"2017MNRAS.470.4... | [
"1999lssu.conf..105C",
"2000AJ....120.1579Y",
"2001MNRAS.326...23B",
"2002ApJ...571..545P",
"2003MNRAS.342..345C",
"2003SPIE.4834..161D",
"2004PASP..116..138C",
"2005MNRAS.357..945G",
"2005MNRAS.358..363C",
"2006MNRAS.365...46O",
"2006MNRAS.366.1151S",
"2006MNRAS.371..829S",
"2006NewAR..49..... |
12516930 | 1607.05497 | The QACITS pointing sensor: from theory to on-sky operation on Keck/NIRC2 | Small inner working angle coronagraphs are essential to benefit from the full potential of large and future extremely large ground-based telescopes, especially in the context of the detection and characterization of exoplanets. Among existing solutions, the vortex coronagraph stands as one of the most effective and pro... | [
-0.01918681338429451,
0.046274080872535706,
0.009572245180606842,
-0.010432830080389977,
-0.014460649341344833,
0.04466577246785164,
-0.025549499318003654,
0.012683047913014889,
-0.023080607876181602,
-0.009212492033839226,
0.024886425584554672,
-0.01721169985830784,
-0.024914640933275223,
... | 14.392312 | 10.692685 | 2016-07-01 | 4 | 2016SPIE.9909E..20H | [
"shared risk mode",
"vortex mode",
"science",
"Small inner working angle coronagraphs",
"exoplanets",
"mechanical flexures",
"existing solutions",
"error",
"errors",
"Coronagraphic Images",
"QACITS",
"a vortex phase mask",
"temperature and/or gravity variations",
"characterization",
"ins... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 7 | [
"10.1117/12.2233274",
"10.48550/arXiv.1607.05497"
] | [
"Huby, Elsa",
"Absil, Olivier",
"Mawet, Dimitri",
"Baudoz, Pierre",
"Femenıa Castellã, Bruno",
"Bottom, Michael",
"Ngo, Henry",
"Serabyn, Eugene"
] | [
"Univ. de Liège (Belgium)",
"Univ. de Liège (Belgium)",
"California Institute of Technology (United States)",
"LESIA, Observatoire de Paris, CNRS, UPMC, Univ. Paris-Diderot (France)",
"W. M. Keck Observatory (United States)",
"California Institute of Technology (United States)",
"California Institute of... | [
"2016SPIE.9909E..22F",
"2017AJ....153...43S",
"2022JATIS...8b9006V",
"2023arXiv231206806B"
] | [
"2005ApJ...633.1191M",
"2010ApJ...709...53M",
"2012A&A...539A.126M",
"2012SPIE.8442E..04M",
"2012SPIE.8446E..8KD",
"2013A&A...552L..13M",
"2014SPIE.9151E..19F",
"2015A&A...584A..74H",
"2015PASP..127..890J"
] |
12608612 | 1607.07989 | Nuclear Physics Meets the Sources of the Ultra-High Energy Cosmic Rays | The determination of the injection composition of cosmic ray nuclei within astrophysical sources requires sufficiently accurate descriptions of the source physics and the propagation - apart from controlling astrophysical uncertainties. We therefore study the implications of nuclear data and models for cosmic ray astro... | [
-0.026270892471075058,
0.008871370926499367,
0.013973136432468891,
-0.03199510648846626,
0.007998776622116566,
0.022640902549028397,
0.003487466834485531,
0.0024083589669317007,
0.003420567838475108,
-0.013763713650405407,
-0.02429301291704178,
0.04069777578115463,
-0.021663596853613853,
-... | 6.042072 | 0.387415 | 2016-07-01 | 33 | 2017NatSR...7.4882B | [
"cosmic ray sources",
"cosmic ray nuclei",
"astrophysical sources",
"non-thermal radiation fields",
"astrophysical environments",
"cosmic ray astrophysics",
"astrophysical uncertainties",
"nuclear model uncertainties",
"propagation",
"environments",
"nuclear models",
"the most precise cosmic r... | [
"Astrophysics - High Energy Astrophysical Phenomena",
"High Energy Physics - Phenomenology",
"Nuclear Experiment",
"Nuclear Theory"
] | 4 | [
"10.1038/s41598-017-05120-7",
"10.48550/arXiv.1607.07989"
] | [
"Boncioli, Denise",
"Fedynitch, Anatoli",
"Winter, Walter"
] | [
"DESY, Platanenallee 6, D-15738, Zeuthen, Germany",
"DESY, Platanenallee 6, D-15738, Zeuthen, Germany",
"DESY, Platanenallee 6, D-15738, Zeuthen, Germany"
] | [
"2017EPJWC.14107001B",
"2017JCAP...01..033B",
"2017JCAP...11..009A",
"2017PhRvD..95l3001L",
"2018A&A...611A.101B",
"2018APh...102...39H",
"2018ApJ...854...54R",
"2018MNRAS.476.1191B",
"2018NPNew..28...12R",
"2018NatSR...810828B",
"2018PhRvD..98d3001S",
"2019ApJ...872..110B",
"2019ApJ...873..... | [
"1948PhRv...74.1046G",
"1976ApJ...205..638P",
"1996PhDT........59R",
"2000CoPhC.124..290M",
"2005AIPC..769..199K",
"2005AIPC..769.1303F",
"2005APh....23..191K",
"2006RPPh...69.2259M",
"2008APh....29....1A",
"2008JCAP...10..033A",
"2008PhRvD..78b3005M",
"2010ApJ...721..630H",
"2010PhRvD..81l3... |
12510090 | 1607.07347 | Cosmological dynamics of spatially flat Einstein-Gauss-Bonnet models in various dimensions: Low-dimensional Λ -term case | In this paper we perform a systematic study of spatially flat [(3 +D )+1 ] -dimensional Einstein-Gauss-Bonnet cosmological models with the Λ -term. We consider models that topologically are the product of two flat isotropic subspaces with different scale factors. One of these subspaces is three-dimensional and represen... | [
-0.002163405530154705,
0.0075449515134096146,
0.02687177248299122,
-0.023983238264918327,
0.016683991998434067,
0.015209759585559368,
-0.01950061321258545,
-0.03933682292699814,
-0.01848183572292328,
0.03384740650653839,
-0.04492212459445,
-0.02231723628938198,
-0.04139835014939308,
0.0315... | 10.227494 | 0.255524 | 2016-07-01 | 25 | 2016PhRvD..94h4019P | [
"D =",
"different scale factors",
"extra dimensions",
"Λ ≤1",
"Λ",
"different dynamics",
"lt;0",
"=",
"an anisotropic exponential regime",
"substantial differences",
"the extra-dimensional part",
"motion",
"all possible regimes",
"physically viable regimes",
"study",
"Λ <0",
"equa... | [
"High Energy Physics - Theory",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology"
] | 4 | [
"10.1103/PhysRevD.94.084019",
"10.48550/arXiv.1607.07347"
] | [
"Pavluchenko, Sergey A."
] | [
"Programa de Pós-Graduação em Física, Universidade Federal do Maranhão (UFMA), 65085-580 São Luís, Maranhão, Brazil"
] | [
"2017EPJC...77...89E",
"2017EPJC...77..402E",
"2017EPJC...77..503P",
"2017GrCo...23..359C",
"2017MPLA...3250202E",
"2018EPJC...78..100I",
"2018EPJC...78..373P",
"2018EPJC...78..551P",
"2018EPJC...78..611P",
"2018EPJWC.16802003T",
"2018GReGr..50..119I",
"2018GrCo...24...28C",
"2018Parti...1..... | [
"1913AnP...347..533N",
"1916AnP...354..769E",
"1921AmJM...43..217K",
"1926Natur.118..516K",
"1926ZPhy...37..895K",
"1932ZPhy...73..147L",
"1969PhRv..177.2309V",
"1970PhLB...33..361S",
"1971JMP....12..498L",
"1974NuPhB..81..118S",
"1977PhLA...64....8T",
"1985NuPhB.258...46C",
"1985PhLB..156..... |
12434660 | 1607.02424 | Study of baryon acoustic oscillations with SDSS DR12 data and measurement of $\Omega_\textrm{DE}(a)$ | We define Baryon Acoustic Oscillation (BAO) distances $\hat{d}_\alpha(z, z_c)$, $\hat{d}_z(z, z_c)$, and $\hat{d}_/(z, z_c)$ that do not depend on cosmological parameters. These BAO distances are measured as a function of redshift $z$ with the Sloan Digital Sky Survey (SDSS) data release DR12. From these BAO distances ... | [
0.011674957349896431,
0.02430669218301773,
0.036220844835042953,
-0.007312510162591934,
-0.025445712730288506,
0.057497743517160416,
-0.03635752573609352,
-0.011982493102550507,
-0.02037707343697548,
-0.02861218899488449,
-0.012996220961213112,
-0.01574126072227955,
-0.07348959147930145,
-... | 12.153745 | 2.335181 | 2016-07-01 | 2 | 2016arXiv160702424H | [
"several scenarios",
"constant dark energy density",
"cosmological parameters",
"flat space",
"DR12",
"agreement",
"z_c)$",
"\\Omega_\\textrm{DE}(a)$.",
"SDSS",
"Baryon Acoustic Oscillation",
"the Sloan Digital Sky Survey",
"(SDSS) data release",
"the cosmological parameters",
"BAO",
"CM... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.48550/arXiv.1607.02424"
] | [
"Hoeneisen, B."
] | [
"-"
] | [
"2016arXiv160808486H",
"2017IJAA....7...11H"
] | [
"2000astro.ph..9071H",
"2007ApJ...664..660E",
"2008PhRvD..77d3525S",
"2010deot.book..246B",
"2013PhR...530...87W",
"2015ApJS..219...12A"
] |
12613181 | 1607.04202 | Theory of Gravitational Waves | The existence of gravitational radiation is a natural prediction of any relativistic description of the gravitational interaction. In this chapter, we focus on gravitational waves, as predicted by Einstein's general theory of relativity. First, we introduce those mathematical concepts that are necessary to properly for... | [
-0.004811108577996492,
0.052687179297208786,
-0.021772900596261024,
-0.014943881891667843,
-0.018131477758288383,
0.0032551297917962074,
-0.003419912187382579,
-0.009724869392812252,
-0.04845145717263222,
0.017050936818122864,
-0.02928266115486622,
0.04551238566637039,
-0.06331970542669296,
... | 9.083855 | 1.579996 | 2016-07-01 | 5 | 2017ogw..book....1L | [
"laser interferometers",
"powerful gravitational wave sources",
"Gravitational waves",
"gravitational waves",
"relativistic speeds",
"curvature",
"gravitational radiation",
"flat spacetime",
"nonspherical compact objects",
"matter",
"spacetime",
"connection",
"Einstein",
"tensor",
"vecto... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 24 | [
"10.1142/9789813141766_0001",
"10.48550/arXiv.1607.04202"
] | [
"Le Tiec, Alexandre",
"Novak, Jérôme"
] | [
"LUTH, Observatoire de Paris, PSL Research University, CNRS, Université Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon Cedex, France",
"LUTH, Observatoire de Paris, PSL Research University, CNRS, Université Paris Diderot, Sorbonne Paris Cité, 5 place Jules Janssen, 92195 Meudon Cedex, Fra... | [
"2016PhRvD..94h4018A",
"2018AnPhy.394..225V",
"2018arXiv181004477B",
"2023arXiv230900772A",
"2024EPJC...84..406D"
] | [
"1972gcpa.book.....W",
"1973grav.book.....M",
"1984ucp..book.....W",
"2003gieg.book.....H",
"2004sgig.book.....C",
"2007tste.book.....K",
"2008LRR....11....8L",
"2008PhRvL.100d1101S",
"2009fcgr.book.....S",
"2011ApJ...743..102G",
"2011gwpa.book.....C",
"2013RvMP...85.1401A",
"2013gere.book..... |
746093 | 1403.4240 | Multi-epoch spectropolarimetry of SN 2009ip: direct evidence for aspherical circumstellar material | We present spectropolarimetry of SN 2009ip throughout the evolution of its 2012 explosion. During the 2012a phase, when the spectrum exhibits broad P-Cygni lines, we measure a V-band polarization of P ≈ 0.9 per cent at a position angle of θ ≈ 166°, indicating substantial asphericity for the 2012a outflow. Near the subs... | [
0.008550683967769146,
0.009820587001740932,
-0.007117972243577242,
-0.0035752668045461178,
-0.011832896620035172,
0.0338640958070755,
0.009338675066828728,
-0.031024720519781113,
-0.011663575656712055,
-0.015108596533536911,
0.004920062143355608,
-0.025515293702483177,
-0.0049037812277674675... | 14.093406 | -0.531925 | 2014-03-01 | 91 | 2014MNRAS.442.1166M | [
"P ≈",
"strong CSM interaction",
"CSM",
"interstellar polarization",
"polarization",
"substantial asphericity",
"θ",
"SN 2009ip",
"intense interaction",
"2012a",
"2012b",
"circumstellar material",
"significant variations",
"SN",
"asphericity",
"spherical symmetry",
"the required expl... | [
"circumstellar matter",
"stars: evolution",
"supernovae: general",
"supernovae: individual: SN 2009ip",
"stars: winds",
"outflows",
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 8 | [
"10.1093/mnras/stu730",
"10.48550/arXiv.1403.4240"
] | [
"Mauerhan, Jon",
"Williams, G. Grant",
"Smith, Nathan",
"Smith, Paul S.",
"Filippenko, Alexei V.",
"Hoffman, Jennifer L.",
"Milne, Peter",
"Leonard, Douglas C.",
"Clubb, Kelsey I.",
"Fox, Ori D.",
"Kelly, Patrick L."
] | [
"Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA; Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA",
"Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA; MMT Observatory, Tucson, AZ 85721-0065, USA",
"Steward... | [
"2014A&A...571A..89Q",
"2014ApJ...789..104O",
"2014MNRAS.441.2230H",
"2015A&A...578A.100W",
"2015AJ....149....9M",
"2015ApJ...803L..26M",
"2015EAS....71..163H",
"2015IAUS..305..269H",
"2015MNRAS.447..598S",
"2015MNRAS.447..772F",
"2015MNRAS.447.1922M",
"2015MNRAS.449.1876S",
"2015MNRAS.450..... | [
"1975ApJ...196..261S",
"1986A&A...163..119Z",
"1988igbo.conf..157M",
"1990MNRAS.244..269S",
"1992AJ....104.1563S",
"1992ApJ...398L..57S",
"1993ApJ...414L..21T",
"1994A&A...285L..13B",
"1994ApJ...420..268C",
"1994ApJ...431L..95L",
"1994ApJ...432L.115V",
"1994MNRAS.268..173C",
"1995AJ....110.2... |
485723 | 1403.3689 | 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses | The 3D-HST and CANDELS programs have provided WFC3 and ACS spectroscopy and photometry over ≈900 arcmin<SUP>2</SUP> in five fields: AEGIS, COSMOS, GOODS-North, GOODS-South, and the UKIDSS UDS field. All these fields have a wealth of publicly available imaging data sets in addition to the Hubble Space Telescope (HST) da... | [
-0.011784059926867485,
-0.0011385672260075808,
0.028836840763688087,
-0.024156147614121437,
-0.0029048530850559473,
-0.01793482154607773,
-0.020545661449432373,
-0.006850514095276594,
-0.00020746325026266277,
-0.033917393535375595,
-0.00807949062436819,
-0.010190507397055626,
-0.016558839008... | 12.778493 | 5.980173 | 2014-03-01 | 821 | 2014ApJS..214...24S | [
"stellar population parameters",
"WFC3",
"account",
"photometric redshifts",
"publicly available imaging data sets",
"the UKIDSS UDS field",
"Objects",
"objects",
"derived data products",
"wavelengths",
"SEDs",
"ACS",
"the ancillary imaging data",
"http://3dhst.research.yale.edu",
"the F... | [
"catalogs",
"galaxies: evolution",
"galaxies: general",
"methods: data analysis",
"techniques: photometric",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 68 | [
"10.1088/0067-0049/214/2/24",
"10.48550/arXiv.1403.3689"
] | [
"Skelton, Rosalind E.",
"Whitaker, Katherine E.",
"Momcheva, Ivelina G.",
"Brammer, Gabriel B.",
"van Dokkum, Pieter G.",
"Labbé, Ivo",
"Franx, Marijn",
"van der Wel, Arjen",
"Bezanson, Rachel",
"Da Cunha, Elisabete",
"Fumagalli, Mattia",
"Förster Schreiber, Natascha",
"Kriek, Mariska",
"L... | [
"South African Astronomical Observatory, PO Box 9, Observatory, Cape Town 7935, South Africa ; Department of Astronomy, Yale University, 260 Whitney Avenue, New Haven, CT 06511, USA;",
"Astrophysics Science Division, Goddard Space Flight Center, Greenbelt, MD 20771, USA",
"Department of Astronomy, Yale Universi... | [
"2014ApJ...788...11L",
"2014ApJ...788...28V",
"2014ApJ...788...86P",
"2014ApJ...789..164T",
"2014ApJ...789L..31W",
"2014ApJ...789L..40W",
"2014ApJ...790..113Z",
"2014ApJ...791...17M",
"2014ApJ...791...45V",
"2014ApJ...792L...6V",
"2014ApJ...793..115B",
"2014ApJ...793L..31V",
"2014ApJ...795..... | [
"1968adga.book.....S",
"1971ApJ...170..193O",
"1980ApJS...43..305K",
"1996A&AS..117..393B",
"1997A&A...326..950F",
"1998ApJ...500..525S",
"1999PASP..111...63F",
"2000AJ....120.2747C",
"2000ApJ...533..682C",
"2000ApJ...538...29C",
"2001AJ....121.2895C",
"2001AJ....122..598D",
"2003AJ....125.1... |
526921 | 1403.6245 | The Stagger-grid: A grid of 3D stellar atmosphere models - V. Fe line shapes, shifts and asymmetries | We present a theoretical study of the effects and signatures of realistic velocity field and atmospheric inhomogeneities associated with convective motions at the surface of cool late-type stars on the emergent profiles of iron spectral lines for a large range in stellar parameters. We compute 3D spectral line flux pro... | [
0.02296307682991028,
-0.005928834434598684,
0.035292502492666245,
-0.048119183629751205,
0.033048469573259354,
0.019176272675395012,
-0.009996142238378525,
-0.05370376259088516,
-0.012029795907437801,
0.014751959592103958,
-0.011041657067835331,
-0.0028114148881286383,
-0.015720972791314125,... | 8.49339 | 10.749544 | 2014-03-01 | 10 | 2014arXiv1403.6245M | [
"line profiles",
"3D spectral line flux profiles",
"iron spectral lines",
"Line shifts",
"line strength",
"convective velocities",
"Theoretical line shifts",
"velocity fields",
"stellar parameters",
"different stellar parameters",
"realistic velocity field",
"cool stars",
"atmospheric inhomo... | [
"Astrophysics - Solar and Stellar Astrophysics"
] | 7 | [
"10.48550/arXiv.1403.6245"
] | [
"Magic, Zazralt",
"Collet, Remo",
"Asplund, Martin"
] | [
"-",
"-",
"-"
] | [
"2015A&A...573A..90M",
"2016AJ....152..167T",
"2017A&A...597A...6N",
"2017A&A...597A..52M",
"2017A&A...605A..90D",
"2017A&A...607A...6M",
"2017A&A...607A.124M",
"2018A&A...611A..11C",
"2021A&A...649A..16D",
"2021arXiv210406072M"
] | [
"1958ZA.....46..108B",
"1965ApJ...142..841H",
"1981A&A....96..345D",
"1982A&A...107....1N",
"1988ApJ...331..815M",
"1989A&A...213..371S",
"1990A&A...228..155N",
"1991ApJ...370..295C",
"1994A&A...291..635A",
"1998ApJ...499..914S",
"2000A&A...359..729A",
"2000A&A...359..743A",
"2000ApJ...536..... |
621082 | 1403.1186 | Constraints on the symmetry energy using the mass-radius relation of neutron stars | The nuclear symmetry energy is intimately connected with nuclear astrophysics. This contribution focuses on the estimation of the symmetry energy from experiment and how it is related to the structure of neutron stars. The most important connection is between the radii of neutron stars and the pressure of neutron star ... | [
0.0353178009390831,
0.0004002322384621948,
0.061600297689437866,
-0.01296321302652359,
0.03841117024421692,
0.035918671637773514,
-0.027239438146352768,
-0.016601813957095146,
0.04039181396365166,
-0.0028513504657894373,
-0.0574609711766243,
-0.00896297674626112,
-0.03705364838242531,
0.00... | 4.410195 | 1.895929 | 2014-03-01 | 249 | 2014EPJA...50...40L | [
"neutron star matter",
"neutron star radii",
"individual neutron star radii",
"nuclear experiment",
"nuclear experiments",
"neutron star interiors",
"neutron stars",
"neutron star",
"nuclear astrophysics",
"pure neutron matter",
"higher precision",
"SUB",
"s</SUB",
"photospheric radius exp... | [
"Nuclear Theory",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Solar and Stellar Astrophysics"
] | 6 | [
"10.1140/epja/i2014-14040-y",
"10.48550/arXiv.1403.1186"
] | [
"Lattimer, James M.",
"Steiner, Andrew W."
] | [
"Dept. of Physics & Astronomy, Stony Brook University",
"Institute for Nuclear Theory"
] | [
"2014MNRAS.442.3777P",
"2014MNRAS.445.4218K",
"2014NuPhA.928..296L",
"2014PhRvC..90b7301M",
"2014PhRvC..90d5801H",
"2014PhRvC..90e4317A",
"2014PhRvC..90e4327S",
"2014PhRvD..90f3010Y",
"2014PhRvD..90l4023C",
"2014arXiv1410.8707D",
"2015A&A...584A.103S",
"2015Ap&SS.359...58B",
"2015EPJC...75..... | [
"1966NucPh..81....1M",
"1969AnPhy..55..395M",
"1979PhRvC..19.1855R",
"1989PhR...175..103L",
"1990ARA&A..28..215D",
"1990AnPhy.204..401M",
"1994NuPhA.567..521K",
"1994PhRvC..49.2118S",
"1999PhRvL..82.3216K",
"2000ApJ...542..914W",
"2001ApJ...550..426L",
"2001PhRvL..87h2501T",
"2003NuPhA.727..... |
437446 | 1403.0463 | Molecular observations of comets C/2012 S1 (ISON) and C/2013 R1 (Lovejoy): HNC/HCN ratios and upper limits to PH<SUB>3</SUB> | We present molecular observations carried out with the IRAM 30 m telescope at wavelengths around 1.15 mm towards the Oort cloud comets C/2012 S1 (ISON) and C/2013 R1 (Lovejoy) when they were at ~0.6 and ~1 au, respectively, from the Sun. We detect HCN, HNC, and CH<SUB>3</SUB>OH in both comets, together with the ion HCO... | [
0.01746404357254505,
0.022674880921840668,
0.0076292334124445915,
-0.03982936963438988,
0.021720420569181442,
0.003924250602722168,
0.02840164303779602,
-0.01807025447487831,
0.015168179757893085,
-0.02644112892448902,
-0.03510865941643715,
-0.01577439159154892,
-0.010073425248265266,
-0.0... | 8.950421 | 16.974802 | 2014-03-01 | 25 | 2014A&A...564L...2A | [
"comet ISON",
"comet Lovejoy",
"ISON",
"Lovejoy",
"anonymous ftp",
"Sun",
"the Oort cloud comets",
"most previous comets",
"upper limits",
"CH<SUB>3</SUB>OH lines",
"both comets",
"the comet",
"a few weak unidentified lines",
"PH",
"HNC",
"activity",
"P",
"November",
"CDS",
"Oo... | [
"comets: general",
"comets: individual: C/2012 S1 (ISON)",
"comets:",
"individual: C/2013 R1 (Lovejoy)",
"Astrophysics - Earth and Planetary Astrophysics"
] | 9 | [
"10.1051/0004-6361/201423639",
"10.48550/arXiv.1403.0463"
] | [
"Agúndez, M.",
"Biver, N.",
"Santos-Sanz, P.",
"Bockelée-Morvan, D.",
"Moreno, R."
] | [
"Univ. Bordeaux, LAB, UMR 5804, 33270, Floirac, France",
"LESIA, Observatoire de Paris, CNRS, UPMC, Université Paris-Diderot, 5 place Jules Janssen, 92195, Meudon, France",
"Instituto de Astrofísica de Andalucía - CSIC, Glorieta de la Astronomía s/n, 18008, Granada, Spain",
"LESIA, Observatoire de Paris, CNRS... | [
"2014A&A...566L...5B",
"2014A&A...567L...1C",
"2014ApJ...790L..27A",
"2014ApJ...791..118M",
"2014ApJ...792L...2C",
"2014ApJ...796L...6B",
"2015A&A...575A..52S",
"2015A&A...584A.121O",
"2015AJ....149...19K",
"2016A&A...588A..72W",
"2016ApJ...820...34D",
"2016IAUFM..29A.228B",
"2016Icar..266..... | [
"1994Icar..107..164B",
"1996Natur.383..418I",
"1997Sci...275.1915B",
"1997ssis.book.....K",
"1998ApJ...497L.117L",
"1998Natur.393..547I",
"2000A&A...353.1101B",
"2001MNRAS.323...84R",
"2002EM&P...89...53B",
"2004A&A...418.1141C",
"2004ApJ...615.1054M",
"2005JMoSp.229..170I",
"2006A&A...449.1... |
1922567 | 1403.5888 | Stellar statistics along the ecliptic and the impact on the K2 mission concept | K2 is the mission concept for a repurposed Kepler mission that uses two reaction wheels to maintain the satellite attitude and provide ~81 days of coverage for ten 105 deg<SUP>2</SUP> fields along the ecliptic in the first 2.5 years of operation. We examine stellar populations based on the updated Besançon model of the... | [
0.0019633343908935785,
0.03359982743859291,
0.06791926175355911,
-0.05161752924323082,
-0.015208489261567593,
0.0455285981297493,
0.004916119854897261,
0.002805751748383045,
-0.00900884997099638,
0.012655289843678474,
-0.018972555175423622,
-0.04555627331137657,
-0.028285851702094078,
-0.0... | 6.897971 | 13.299354 | 2014-03-01 | 3 | 2015IJAsB..14..165P | [
"stellar occurrence rates",
"~81 days",
"> fields",
"operation",
"galactic latitude",
"first",
"stellar populations",
"orbital periods",
"SUP>2</SUP",
"deg",
"coverage",
"Transiting Exoplanet Survey Satellite",
"optimized target selection",
"spectral type and luminosity class",
"the expe... | [
"extrasolar planets",
"Kepler",
"stellar populations",
"Astrophysics - Solar and Stellar Astrophysics"
] | 4 | [
"10.1017/S1473550414000329",
"10.48550/arXiv.1403.5888"
] | [
"Prša, Andrej",
"Robin, Annie",
"Barclay, Thomas"
] | [
"Department of Astrophysics and Planetary Science, Villanova University, 800 E Lancaster Ave, Villanova, PA 19085, USA",
"Institute Utinam, CNRS UMR6213, Université de Franche-Comté, OSU THETA de Franche-Comté-Bourgogne, Besançon, France",
"NASA Ames Research Center, M/S 244-30, Moffett Field, CA 94035, USA"
] | [
"2015RAA....15.1945S",
"2016AJ....151...68K",
"2018exha.book.....P"
] | [
"1989ApJ...345..245C",
"1997A&A...324...65N",
"1999ASPC..192.....H",
"1999BaltA...8..147V",
"2003A&A...409..523R",
"2003AdSpR..31..345B",
"2005A&A...436..895G",
"2006A&A...453..635M",
"2009A&A...495..819R",
"2009A&A...503L..21M",
"2009ExA....23..329C",
"2010ApJ...725.2166H",
"2010ApJS..190..... |
256584 | 1403.7075 | Transport of the charged dust grains to the galactic halo | We develop a 3D dynamical model of dust outflows from galactic discs. The outflows are initiated by multiple SN explosions in a magnetized interstellar medium (ISM) with a gravitationally stratified density distribution. Dust grains are treated as particles in cells interacting collisionally with gas, and forced by ste... | [
-0.0015745877753943205,
0.025121008977293968,
0.0009660186478868127,
0.011685733683407307,
-0.017531616613268852,
0.007565260864794254,
-0.004413068760186434,
-0.00018409780750516802,
-0.042978402227163315,
0.03361533582210541,
-0.008240945637226105,
0.016035456210374832,
-0.0257725622504949... | 12.176749 | 8.359406 | 2014-03-01 | 3 | 2013lcdu.confE..60K | [
"galactic discs",
"Lorenz force",
"Dust grains",
"dust outflows",
"stellar radiation",
"ISM",
"multiple SN explosions",
"distances",
"Lorenz",
"the galactic plane",
"gas",
"the charged dust grains",
"the outflowing medium varies",
"the dust mass loss rate",
"cells",
"magnetic field",
... | [
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 2 | [
"10.22323/1.207.0060",
"10.48550/arXiv.1403.7075"
] | [
"Khoperskov, S.",
"Shchekinov, Y."
] | [
"-",
"-"
] | [
"2014Sci...345..791K",
"2015MmSAI..86..541Z",
"2017PhyU...60..961S"
] | null |
621860 | 1403.0655 | An analytic calculation of the growth index for dark energy model | We derive the analytic formula of the growth index for the dark energy model where the effect on the growth of matter density perturbation from modified gravity (MG) is encoded in the effective Newton coupling constant in MG (or equivalently ). Based on the analytic formula, we propose that the parameter can be directl... | [
0.04212458059191704,
0.024852391332387924,
-0.01014768984168768,
-0.007835838943719864,
-0.014860307797789574,
0.00895286351442337,
-0.019250601530075073,
0.022195987403392792,
-0.014626899734139442,
-0.0052627939730882645,
-0.008497161790728569,
0.0028592476155608892,
-0.04130209609866142,
... | 11.063164 | 1.333309 | 2014-03-01 | 11 | 2014EPJC...74.2964H | [
"MG",
"Newton",
"general relativity",
"matter density perturbation",
"modified gravity",
"the observed growth rate",
"the dark energy model",
"the growth index",
"the growth",
"the analytic formula",
"the effect",
"the prediction",
"the parameter",
"We",
"we"
] | [
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology",
"High Energy Physics - Theory"
] | 9 | [
"10.1140/epjc/s10052-014-2964-6",
"10.48550/arXiv.1403.0655"
] | [
"Huang, Qing-Guo"
] | [
"State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Science"
] | [
"2014PhRvD..90d3513R",
"2019EPJP..134..318L",
"2019IJMPD..2850132L",
"2019PhLB..795..129L",
"2019PhRvD.100h3503C",
"2020PhLB..81135985L",
"2021EPJP..136..883B",
"2022ApJ...934...13K",
"2022IJMPD..3150117L",
"2022arXiv220306741S",
"2023FoPh...53....5L"
] | [
"1980PhLB...91...99S",
"1998ApJ...508..483W",
"2000PhLB..485..208D",
"2002PhRvD..65d4023D",
"2005PhRvD..72d3529L",
"2006PhRvD..73l3504Z",
"2007APh....28..481L",
"2007JETPL..86..157S",
"2007PhLB..654....7A",
"2007PhRvD..75h3504A",
"2007PhRvD..76b3514T",
"2007PhRvD..76f4004H",
"2008PhLB..660..... |
437704 | 1403.7902 | Ubiquitous argonium (ArH<SUP>+</SUP>) in the diffuse interstellar medium: A molecular tracer of almost purely atomic gas | <BR /> Aims: We describe the assignment of a previously unidentified interstellar absorption line to ArH<SUP>+</SUP> and discuss its relevance in the context of hydride absorption in diffuse gas with a low H<SUB>2</SUB> fraction. The confidence of the assignment to ArH<SUP>+</SUP> is discussed, and the column densities... | [
-0.015310931019484997,
0.019988561049103737,
-0.03269229084253311,
0.025381894782185555,
0.025688624009490013,
0.0185954961925745,
-0.007508491165935993,
-0.01352167408913374,
0.002623179228976369,
0.022480741143226624,
-0.023375369608402252,
0.02168835699558258,
0.011444857344031334,
-0.0... | 11.885487 | 11.17517 | 2014-03-01 | 106 | 2014A&A...566A..29S | [
"atomic diffuse gas",
"diffuse gas",
"dense molecular gas",
"gas",
"determined column densities",
"interstellar matter",
"ArH",
"different H<SUB>2</SUB",
"several lines",
"multiple velocity components",
"gt;99.9% atomic",
"ISM",
"chemical models",
"H<SUB>2</SUB",
"cosmic ray ionization",... | [
"astrochemistry",
"line: identification",
"molecular processes",
"ISM: abundances",
"ISM: molecules",
"ISM: structure",
"Astrophysics - Astrophysics of Galaxies"
] | 26 | [
"10.1051/0004-6361/201423727",
"10.48550/arXiv.1403.7902"
] | [
"Schilke, P.",
"Neufeld, D. A.",
"Müller, H. S. P.",
"Comito, C.",
"Bergin, E. A.",
"Lis, D. C.",
"Gerin, M.",
"Black, J. H.",
"Wolfire, M.",
"Indriolo, N.",
"Pearson, J. C.",
"Menten, K. M.",
"Winkel, B.",
"Sánchez-Monge, Á.",
"Möller, T.",
"Godard, B.",
"Falgarone, E."
] | [
"I. Physikalisches Institut der Universität zu Köln, Zülpicher Str. 77, 50937, Köln, Germany",
"The Johns Hopkins University, Baltimore, MD, 21218, USA",
"I. Physikalisches Institut der Universität zu Köln, Zülpicher Str. 77, 50937, Köln, Germany",
"I. Physikalisches Institut der Universität zu Köln, Zülpiche... | [
"2014A&A...566L...6M",
"2014A&A...567A..53K",
"2014A&A...569L...5M",
"2014ApJ...789....8N",
"2014FaDi..168....9V",
"2014RSCAd...462030J",
"2014sf2a.conf...17D",
"2015A&A...577A..49N",
"2015A&A...582L...4M",
"2015ARA&A..53..199G",
"2015ApJ...800...40I",
"2015ApJ...801..141O",
"2015ApJ...812..... | [
"1965PPS....86..467K",
"1976S&T....52..327C",
"1978ApJS...36..595D",
"1982ApJS...48...95S",
"1982JChPh..76.3529V",
"1982JChPh..77..693W",
"1982PhyS...25..268B",
"1983JChPh..79.2093B",
"1984JMoSp.106..124J",
"1985JMoSp.113..451R",
"1987JChPh..87.2442L",
"1988JMoSp.127..279F",
"1988JMoSp.128..... |
437599 | 1403.6715 | Ionization structure of multiple-shell planetary nebulae. I. NGC 2438 | Context. In recent times an increasing number of extended haloes and multiple shells around planetary nebulae have been discovered. These faint extensions to the main nebula trace the mass-loss history of the star, modified by the subsequent evolution of the nebula. Integrated models predict that some haloes may be rec... | [
-0.008778403513133526,
-0.008256587199866772,
-0.0013532546581700444,
-0.007615876384079456,
-0.0054559530690312386,
0.015509174205362797,
0.03091266378760338,
-0.01820412464439869,
-0.016354648396372795,
0.03577414155006409,
0.028349818661808968,
0.01936665177345276,
-0.03759719803929329,
... | 10.158763 | 10.336473 | 2014-03-01 | 13 | 2014A&A...565A..87O | [
"archival VLA observations",
"HST archive",
"VLA",
"multiple shells",
"m",
"telescope",
"ESO",
"observations",
"ionization equilibrium",
"SAAO",
"extended haloes",
"the main nebula",
"haloes",
"UV radiation",
"data",
"the inner nebula",
"3.6 m telescope",
"ionization",
"membershi... | [
"planetary nebulae: general",
"planetary nebulae: individual: NGC 2438",
"stars: AGB and post-AGB",
"Astrophysics - Solar and Stellar Astrophysics"
] | 5 | [
"10.1051/0004-6361/201323205",
"10.48550/arXiv.1403.6715"
] | [
"Öttl, S.",
"Kimeswenger, S.",
"Zijlstra, A. A."
] | [
"Institute for Astro and Particle Physics, Leopold Franzens Universität Innsbruck, Technikerstrasse 25, 6020, Innsbruck, Austria",
"Instituto de Astronomía, Universidad Católica del Norte, 0610 Avenida Angamos, Antofagasta, Chile ; Institute for Astro and Particle Physics, Leopold Franzens Universität Innsbruck, ... | [
"2015Ap&SS.357...21A",
"2015ApJ...812..133S",
"2015RMxAA..51..221Z",
"2016ApJS..226...22R",
"2016MNRAS.455.1459F",
"2018A&A...620A..84B",
"2018Galax...6...84B",
"2018MNRAS.480.1626B",
"2020A&A...640A..10W",
"2020A&A...644A..63A",
"2020MNRAS.493.2238A",
"2022A&A...658A..17S",
"2022ApJ...939..... | [
"1977RMxAA...2..181T",
"1983ApJ...271..188K",
"1983ApJS...51..211A",
"1985A&A...142..441O",
"1987ApJS...64..529C",
"1988A&A...202..253K",
"1988ApJ...334..862M",
"1989A&AS...79..329Z",
"1989ApJ...343..811S",
"1989SSRv...51..339K",
"1990ApJ...359..392K",
"1991A&A...249..223G",
"1992A&A...255..... |
482820 | 1403.1135 | Transient Spirals as Superposed Instabilities | We present evidence that recurrent spiral activity, long manifested in simulations of disk galaxies, results from the superposition of a few transient spiral modes. Each mode lasts between 5 and 10 rotations at its corotation radius where its amplitude is greatest. The scattering of stars as each wave decays takes plac... | [
-0.005924372002482414,
0.018111834302544594,
0.02671399712562561,
-0.017447179183363914,
-0.007950290106236935,
0.057876065373420715,
0.057262539863586426,
-0.0026857792399823666,
-0.029628250747919083,
0.036070287227630615,
-0.01264121662825346,
0.0011711339466273785,
-0.04373937472701073,
... | 10.025497 | 6.798583 | 2014-03-01 | 115 | 2014ApJ...785..137S | [
"disk galaxies",
"subsequent traveling waves",
"waves",
"new locations",
"spiral activity",
"further activity",
"new standing-wave instabilities",
"angular momentum",
"other recent simulations",
"abrupt changes",
"narrow ranges",
"low-mass disks",
"random motion",
"simulations",
"particl... | [
"galaxies: kinematics and dynamics",
"galaxies: spiral",
"galaxies: structure",
"instabilities",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 14 | [
"10.1088/0004-637X/785/2/137",
"10.48550/arXiv.1403.1135"
] | [
"Sellwood, J. A.",
"Carlberg, R. G."
] | [
"Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854, USA",
"Department of Astronomy and Astrophysics, University of Toronto, Toronto, ON M5S 3H4, Canada"
] | [
"2014ApJ...792..122L",
"2014ApJ...794..173V",
"2014AstL...40..724O",
"2014MNRAS.443.2757K",
"2014MNRAS.443L...1D",
"2014MNRAS.444.3756M",
"2014PASA...31...35D",
"2014hpcn.conf...54B",
"2015AJ....149..116M",
"2015ApJ...799..213B",
"2015ApJ...800..106W",
"2015ApJ...802L..13D",
"2015ApJ...806..... | [
"1964ApJ...139.1217T",
"1965MNRAS.130..125G",
"1966ApJ...146..810J",
"1966PNAS...55..229L",
"1969ApJ...158..899T",
"1972ASSL...31...22R",
"1972MNRAS.157....1L",
"1974ApJ...193..539M",
"1974MNRAS.167..351H",
"1976ApJS...31..313S",
"1977ApJ...212..637K",
"1977ApJ...212..645M",
"1978PhDT.......... |
813545 | 1403.3289 | Primordial tensor modes from quantum corrected inflation | We analyze quantum corrections on the naive ϕ<SUP>4</SUP> inflation. These typically lead to an inflaton potential which carries a noninteger power of the field. We consider both minimal and nonminimal couplings to gravity. For the latter case we also study unitarity of inflaton-inflaton scattering. Finally we confront... | [
-0.031085768714547157,
0.017919758334755898,
-0.010200746357440948,
0.005205234978348017,
0.00892492476850748,
-0.0011862518731504679,
0.009000658057630062,
0.043249767273664474,
-0.04539361223578453,
0.005819843150675297,
-0.0012729086447507143,
0.02649514190852642,
-0.013550505973398685,
... | 11.120042 | -0.675024 | 2014-03-01 | 38 | 2014PhRvD..90d3509J | [
"sizable quantum departures",
"primordial tensor modes",
"quantum corrections",
"gravity",
"quantum",
"the main distinctive features",
"inflaton-inflaton scattering",
"unitarity",
"the ϕ<SUP>4</SUP>-inflation model",
"a noninteger power",
"the naive ϕ<SUP>4</SUP> inflation",
"an inflaton poten... | [
"98.80.Cq",
"Particle-theory and field-theory models of the early Universe",
"High Energy Physics - Phenomenology",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 4 | [
"10.1103/PhysRevD.90.043509",
"10.48550/arXiv.1403.3289"
] | [
"Joergensen, Jakob",
"Sannino, Francesco",
"Svendsen, Ole"
] | [
"CP-Origins and The Danish IAS, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark",
"CP-Origins and The Danish IAS, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark",
"CP-Origins and The Danish IAS, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denm... | [
"2014GReGr..46.1786N",
"2014JCAP...06..045K",
"2014JCAP...07..020C",
"2014JCAP...08..040D",
"2014JHEP...06..080S",
"2014PhLB..734...41G",
"2014PhRvD..89j3524K",
"2014PhRvD..89j3525C",
"2014PhRvD..90b3525B",
"2014PhRvD..90d3505B",
"2014PhRvD..90d7303C",
"2014PhRvD..90l4061B",
"2014SCPMA..57.1... | [
"1973PhRvD...7.1888C",
"1976PhRvD..13.3333G",
"1979JETPL..30..682S",
"1979PZETF..30..719S",
"1980PhLB...91...99S",
"1981JETPL..33..532M",
"1981PZETF..33..549M",
"1981PhRvD..23..347G",
"1982PhLB..108..389L",
"1982PhRvL..48.1220A",
"1982PhRvL..49.1110G",
"2008PhLB..659..703B",
"2010PhRvD..82d3... |
437538 | 1403.6186 | Correlations between the stellar, planetary, and debris components of exoplanet systems observed by Herschel | Context. Stars form surrounded by gas- and dust-rich protoplanetary discs. Generally, these discs dissipate over a few (3-10) Myr, leaving a faint tenuous debris disc composed of second-generation dust produced by the attrition of larger bodies formed in the protoplanetary disc. Giant planets detected in radial velocit... | [
0.009051639586687088,
0.017641067504882812,
0.010457532480359077,
-0.005013709422200918,
0.0311479102820158,
0.07046155631542206,
0.011028876528143883,
0.020696798339486122,
-0.01895066536962986,
0.01208811067044735,
-0.028425998985767365,
0.014290034770965576,
-0.001334474771283567,
-0.05... | 9.028565 | 13.17443 | 2014-03-01 | 57 | 2014A&A...565A..15M | [
"dust temperature",
"cold debris discs",
"dust emission",
"dust",
"fractional luminosities",
"lower planet masses",
"upper limits",
"Stars form",
"planet formation",
"flux density levels",
"Giant planets",
"a faint tenuous debris disc",
"the debris disc systems",
"larger bodies",
"the du... | [
"infrared: stars",
"infrared: planetary systems",
"circumstellar matter",
"planet-disk interactions",
"Astrophysics - Earth and Planetary Astrophysics"
] | 12 | [
"10.1051/0004-6361/201323058",
"10.48550/arXiv.1403.6186"
] | [
"Marshall, J. P.",
"Moro-Martín, A.",
"Eiroa, C.",
"Kennedy, G.",
"Mora, A.",
"Sibthorpe, B.",
"Lestrade, J. -F.",
"Maldonado, J.",
"Sanz-Forcada, J.",
"Wyatt, M. C.",
"Matthews, B.",
"Horner, J.",
"Montesinos, B.",
"Bryden, G.",
"del Burgo, C.",
"Greaves, J. S.",
"Ivison, R. J.",
... | [
"Depto. de Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, 28049, Madrid, Spain ; School of Physics, University of New South Wales, Sydney, NSW, 2052, Australia",
"Department of Astrophysics, Center for Astrobiology, Ctra. de Ajalvir, km 4, Torrejon de Ardoz, 28850, Madrid, Spain; Space Telescope Sci... | [
"2014A&A...567A.127S",
"2014A&A...570A.114M",
"2014ApJ...791..114W",
"2014MNRAS.445.3315N",
"2014sf2a.conf..181F",
"2015A&A...579A..20M",
"2015AJ....149...86W",
"2015Ap&SS.357..103W",
"2015ApJ...799..182P",
"2015ApJ...801..143M",
"2015MNRAS.449.3121K",
"2016A&A...593A..51M",
"2016ApJ...826..... | [
"1969SoPh...10..330E",
"1993prpl.conf.1253B",
"1995ApJ...450L..35B",
"1995Natur.378..355M",
"1996ApJ...464L.147M",
"1996ApJ...464L.153B",
"1997ApJ...474L.115B",
"1997ApJ...483..457C",
"1997ApJ...483L.111N",
"1997GeoRL..24.3125G",
"1998A&A...338L..67D",
"1998ApJ...505L.147M",
"1998Natur.392..... |
484071 | 1403.7463 | The Rest-frame Ultraviolet Structure of 0.5 < z < 1.5 Galaxies | We present the rest-frame UV wavelength dependence of the Petrosian-like half-light radius (r <SUB>50</SUB>), and the concentration parameter for a sample of 198 star-forming galaxies at 0.5 < z < 1.5. We find a ~5% decrease in r <SUB>50</SUB> from 1500 Å to 3000 Å, with half-light radii at 3000 Å ranging from 0.... | [
0.007504705805331469,
0.01784251444041729,
0.024039169773459435,
0.03614314645528793,
0.0010654270881786942,
0.034238338470458984,
0.02161596529185772,
0.0005786761175841093,
-0.007372092921286821,
0.017830457538366318,
-0.04094133526086807,
0.011248016729950905,
-0.03194774314761162,
-0.0... | 12.623739 | 6.503448 | 2014-03-01 | 12 | 2014ApJ...791...18B | [
"lt",
"large galaxies",
"different UV colors",
"higher redshifts",
"z",
"z <",
"SUB>50</SUB",
"r <",
"SUB>3000</SUB",
"clumpy star formation",
"concentration",
"0.6 kpc",
"6 kpc",
"disk-like galaxies",
"bulges",
"more dust",
"length scales",
"C",
"the rest-frame UV wavelength d... | [
"cosmology: observations",
"galaxies: formation",
"galaxies: high-redshift",
"galaxies: structure",
"Astrophysics - Astrophysics of Galaxies"
] | 6 | [
"10.1088/0004-637X/791/1/18",
"10.48550/arXiv.1403.7463"
] | [
"Bond, Nicholas A.",
"Gardner, Jonathan P.",
"de Mello, Duilia F.",
"Teplitz, Harry I.",
"Rafelski, Marc",
"Koekemoer, Anton M.",
"Coe, Dan",
"Grogin, Norman",
"Gawiser, Eric",
"Ravindranath, Swara",
"Scarlata, Claudia"
] | [
"Cosmology Laboratory (Code 665), NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA",
"Cosmology Laboratory (Code 665), NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA",
"Physics Department, The Catholic University of America, Washington, DC 20064 USA",
"IPAC, California Institute of Techn... | [
"2014MNRAS.445..175G",
"2015A&A...576A..51G",
"2015AJ....150...31R",
"2015ApJ...814...97S",
"2016ApJ...817...79H",
"2016arXiv161001163H",
"2017ApJ...836..136F",
"2017ApJ...839...71F",
"2018MNRAS.474.3976G",
"2019A&A...632A.128B",
"2019ApJ...875..152B",
"2019arXiv191007043B"
] | [
"1976ApJ...209L...1P",
"1985ApJS...59..115K",
"1996A&AS..117..393B",
"2000ApJ...536..571B",
"2000ApJS..131..441K",
"2003ApJS..147....1C",
"2003SPIE.4854...81F",
"2003hstc.conf..337K",
"2004A&A...428.1043L",
"2004ApJ...600L.107F",
"2004ApJS..150....1B",
"2004ApJS..155..271S",
"2005A&A...434..... |
871001 | 1403.2246 | The Present and Future of Planetary Nebula Research. A White Paper by the IAU Planetary Nebula Working Group | We present a summary of current research on planetary nebulae and their central stars, and related subjects such as atomic processes in ionized nebulae, AGB and post-AGB evolution. Future advances are discussed that will be essential to substantial improvements in our knowledge in the field. | [
-0.026158995926380157,
0.010611778125166893,
0.04758090153336525,
-0.01286947913467884,
0.0020141375716775656,
-0.006096376106142998,
0.03497977927327156,
-0.01533136423677206,
0.027325766161084175,
0.023872124031186104,
-0.006364732980728149,
0.0207101758569479,
-0.07275980710983276,
-0.0... | 10.078562 | 10.017478 | 2014-03-01 | 32 | 2014RMxAA..50..203K | [
"post-AGB evolution",
"atomic processes",
"related subjects",
"AGB",
"planetary nebulae",
"substantial improvements",
"current research",
"Future advances",
"their central stars",
"the field",
"our knowledge",
"a summary",
"We",
"that"
] | [
"ISM: abundances",
"planetary nebulae: general",
"stars: AGB and post-AGB",
"stars: evolution",
"Astrophysics - Solar and Stellar Astrophysics"
] | 53 | [
"10.48550/arXiv.1403.2246"
] | [
"Kwitter, K. B.",
"Méndez, R. H.",
"Peña, M.",
"Stanghellini, L.",
"Corradi, R. L. M.",
"De Marco, O.",
"Fang, X.",
"Henry, R. B. C.",
"Karakas, A. I.",
"Liu, X. -W.",
"López, J. A.",
"Manchado, A.",
"Parker, Q. A."
] | [
"Department of Astronomy, Williams College, Williamstown, MA, USA.",
"-",
"-",
"-",
"-",
"-",
"-",
"-",
"-",
"-",
"-",
"-",
"-"
] | [
"2015A&A...579A..86W",
"2015ASPC..493...83M",
"2015ApJ...815...69F",
"2015RMxAA..51..221Z",
"2015arXiv151204129M",
"2016A&A...588A..25M",
"2016ApJ...832..125H",
"2016ApJS..223....6Y",
"2016MNRAS.457.3409A",
"2017BAAA...59...43M",
"2017NatAs...1E.117J",
"2017PASA...34....1D",
"2017PASP..129h2... | [
"1971BOTT....6...29P",
"1976IAUS...73...75P",
"1978ApJ...219..914B",
"1982MNRAS.198..111Z",
"1982MNRAS.198..127M",
"1985ApJ...290L..25A",
"1986A&AS...64..545N",
"1989ApJ...345L..51K",
"1993ApJ...413..641V",
"1993MNRAS.263..256L",
"1994A&A...282..999S",
"1994A&A...283..593P",
"1994MNRAS.271..... |
747125 | 1403.7525 | The life and death of cosmic voids | We investigate the formation, growth, merger history, movement, and destruction of cosmic voids detected via the watershed transform code VIDE in a cosmological N-body dark matter Λ cold dark matter simulation. By adapting a method used to construct halo merger trees, we are able to trace individual voids back to their... | [
0.00308843026868999,
0.06751403212547302,
0.051631681621074677,
-0.016766265034675598,
0.0006484651239588857,
-0.0043494077399373055,
0.017972875386476517,
-0.02850966714322567,
-0.01720120571553707,
0.043185409158468246,
0.013890044763684273,
-0.0012451934162527323,
-0.06661608815193176,
... | 11.290302 | 2.639526 | 2014-03-01 | 35 | 2014MNRAS.445.1235S | [
"cold dark matter simulation",
"dark energy",
"void destruction",
"void sizes",
"cosmological initial conditions",
"scale factor",
"merger history",
"halo merger trees",
"individual voids",
"cosmic voids",
"high redshift",
"little radical dynamical evolution",
"the median initial void size",... | [
"cosmology: theory",
"large-scale structure of Universe",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 4 | [
"10.1093/mnras/stu1845",
"10.48550/arXiv.1403.7525"
] | [
"Sutter, P. M.",
"Elahi, Pascal",
"Falck, Bridget",
"Onions, Julian",
"Hamaus, Nico",
"Knebe, Alexander",
"Srisawat, Chaichalit",
"Schneider, Aurel"
] | [
"Sorbonne Universités, UPMC Univ Paris 06, UMR7095, Institut d'Astrophysique de Paris, F-75014 Paris, France; CNRS, UMR7095, Institut d'Astrophysique de Paris, F-75014 Paris, France; Center for Cosmology and AstroParticle Physics, Ohio State University, Columbus, OH 43210, USA",
"Sydney Institute for Astronomy, U... | [
"2014JCAP...12..013H",
"2014MNRAS.443.2983S",
"2014arXiv1409.8661A",
"2015JCAP...11..036H",
"2015MNRAS.450.3239F",
"2015PhRvD..92h3531P",
"2016IAUS..308..493V",
"2016IAUS..308..524S",
"2016MNRAS.456.4425C",
"2016MNRAS.458.4431W",
"2016MNRAS.461.4013C",
"2016PhRvD..93j3519P",
"2017CMPh...2013... | [
"1979Natur.281..358A",
"1987ApJ...313..505W",
"1993ApJ...410..458D",
"1993MNRAS.263..481V",
"1994ApJ...431...20S",
"1995ApJ...452...25R",
"1996MNRAS.282..641S",
"2003MNRAS.344..715G",
"2004ApJ...605....1G",
"2004MNRAS.350..517S",
"2004ogci.conf...58V",
"2005MNRAS.364.1105S",
"2006MNRAS.366..... |
800084 | 1403.5716 | The challenge for single field inflation with BICEP2 result | The detection of B-mode power spectrum by the BICEP2 collaboration constrains the tensor-to-scalar ratio r=0.20-0.05+0.07 for the lensed-ΛCDM model. The consistency of this big value with the Planck results requires a large running of the spectral index. The large values of the tensor-to-scalar ratio and the running of... | [
0.046530090272426605,
0.009976843371987343,
0.008070673793554306,
-0.04198460653424263,
-0.004967038054019213,
0.018695125356316566,
-0.007343640550971031,
0.011968545615673065,
-0.04227786511182785,
-0.02339945361018181,
-0.01681339368224144,
0.011828026734292507,
-0.049022771418094635,
-... | 11.414172 | -0.708225 | 2014-03-01 | 50 | 2014PhLB..734...41G | [
"single field inflation",
"scalar",
"the spectral index",
"a large running",
"an upper limit",
"The large values",
"r=0.20",
"the absolute value",
"BICEP2",
"the chaotic inflation",
"the natural inflation",
"this big value",
"the running",
"the lensed-ΛCDM model",
"the larger the value",... | [
"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Theory"
] | 4 | [
"10.1016/j.physletb.2014.05.018",
"10.48550/arXiv.1403.5716"
] | [
"Gao, Qing",
"Gong, Yungui"
] | [
"MOE Key Laboratory of Fundamental Quantities Measurement, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, PR China",
"MOE Key Laboratory of Fundamental Quantities Measurement, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, PR China"
] | [
"2014JCAP...07..020C",
"2014JCAP...08..040D",
"2014JCAP...10..025H",
"2014JCAP...10..048G",
"2014JCAP...11..003L",
"2014JHEP...07..026H",
"2014JHEP...10..137M",
"2014MPLA...2950197F",
"2014PTEP.2014j3C01K",
"2014PhLB..737..191H",
"2014PhLB..737..374B",
"2014PhLB..738..206L",
"2014PhLB..738..... | [
"1982PhRvL..48.1220A",
"1983PhLB..129..177L",
"1990PhRvL..65.3233F",
"2005JCAP...07..010B",
"2010JCAP...09..007B",
"2012JCAP...02..008H",
"2014A&A...571A..16P",
"2014A&A...571A..22P",
"2014JCAP...02..025A",
"2014JCAP...07..014C",
"2014NuPhB.882..386C",
"2014PhLB..733..283H",
"2014PhLB..734..... |
643722 | 1403.0127 | Complex Investigation of SBS Galaxies in Seven Selected Fields | It is known that the main criterion for the selection of active objects in the First Byurakan, otherwise Markarian survey was the presence of signs of UV-excess in their low-dispersion spectra. Using the presence of emission lines as the second criteria became real during the Second Byurakan survey because of its impro... | [
-0.0017409658757969737,
0.025845663622021675,
0.01602712646126747,
-0.018280142918229103,
-0.028418708592653275,
-0.021275628358125687,
0.011636309325695038,
-0.0285723228007555,
-0.0014161349972710013,
0.030671723186969757,
-0.019304240122437477,
-0.04042625427246094,
-0.006093380507081747,... | 14.737309 | 6.737109 | 2014-03-01 | 3 | 2014IAUS..304...36H | [
"lt",
"active objects",
"objects",
"SBS galaxies",
"used criteria",
"individual galaxies",
"2.6.m telescope",
"SUB",
"galaxies",
"Byurakan",
"multipupil spectrographs MPFS",
"extended version",
"SAO Russia",
"the Second Byurakan survey",
"VAGR",
"different stages",
"spectral classifi... | [
"Astrophysics - Astrophysics of Galaxies"
] | 1 | [
"10.1017/S1743921314003238",
"10.48550/arXiv.1403.0127"
] | [
"Hakopian, Susanna"
] | [
"Byurakan Astrophysical Observatory (BAO), Armenia"
] | [
"2016ASPC..505..183H",
"2021Ap.....64....8H",
"2022Ap.....65..297H"
] | [
"1967Ap......3...24M",
"1968ApJ...151..393S",
"1970ApJ...162L.155S",
"1974ApJ...192..581K",
"1980A&A....87..142H",
"1983Ap.....19..354M",
"1985ApJS...57..503F",
"1987A&AS...70..281B",
"1987ApJS...63..295V",
"1990ApJS...72..567G",
"1993ApJ...404..551O",
"1997A&A...319...52V",
"1999IAUS..194..... |