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437733 | 1403.6308 | Nonlinear Kalman filters for calibration in radio interferometry | The data produced by the new generation of interferometers are affected by a wide variety of partially unknown complex effects such as pointing errors, phased array beams, ionosphere, troposphere, Faraday rotation, or clock drifts. Most algorithms addressing direction-dependent calibration solve for the effective Jones... | [
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-0.036496929824352264... | 11.210581 | 3.6295 | 2014-03-01 | 93 | 2014A&A...566A.127T | [
"conditioning",
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"array beams",
"calibration",
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"instrumentation: interferometers",
"methods: data analysis",
"techniques: interferometric",
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 7 | [
"10.1051/0004-6361/201423503",
"10.48550/arXiv.1403.6308"
] | [
"Tasse, C."
] | [
"GEPI, Observatoire de Paris, CNRS, Université Paris Diderot, 5 place Jules Janssen, 92190, Meudon, France ; SKA South Africa, 3rd Floor, The Park, Park Road, 7405, Pinelands, South Africa; Department of Physics & Electronics, Rhodes University, PO Box 94, 6140, Grahamstown, South Africa"
] | [
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483204 | 1403.4627 | The Stellar Halos of Massive Elliptical Galaxies. III. Kinematics at Large Radius | We present a two-dimensional kinematic analysis out to ~2-5 effective radii (R<SUB>e</SUB> ) of 33 massive elliptical galaxies with stellar velocity dispersions σ > 150 km s<SUP>-1</SUP>. Our observations were taken using the Mitchell Spectrograph (formerly VIRUS-P), a spectrograph with a large 107 × 107 arcsec<SUP>... | [
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-0.0... | 11.156897 | 6.656718 | 2014-03-01 | 41 | 2014ApJ...786...23R | [
"elliptical galaxy formation",
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"e</SUB",
"kinematic decoupling",
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"outer accretion-dominated halos",
"the stellar angular momentum",
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"galaxies: elliptical and lenticular",
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"Astrophysics - Astrophysics of Galaxies"
] | 6 | [
"10.1088/0004-637X/786/1/23",
"10.48550/arXiv.1403.4627"
] | [
"Raskutti, Sudhir",
"Greene, Jenny E.",
"Murphy, Jeremy D."
] | [
"Department of Astrophysics, Princeton University, Princeton, NJ 08540, USA",
"Department of Astrophysics, Princeton University, Princeton, NJ 08540, USA; Department of Astronomy, UT Austin, 1 University Station C1400, Austin, TX 71712, USA",
"Department of Astrophysics, Princeton University, Princeton, NJ 0854... | [
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477511 | 1403.3141 | Clustering of Local Group Distances: Publication Bias or Correlated Measurements? I. The Large Magellanic Cloud | The distance to the Large Magellanic Cloud (LMC) represents a key local rung of the extragalactic distance ladder yet the galaxy's distance modulus has long been an issue of contention, in particular in view of claims that most newly determined distance moduli cluster tightly—and with a small spread—around the "canonic... | [
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-0.0... | 7.628262 | 9.42493 | 2014-03-01 | 156 | 2014AJ....147..122D | [
"LMC distance moduli",
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"distance estimates",
"the individual distance moduli",
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"a given distance tracer",
"a general distance scale",
"the LMC distances",
"LMC",
"the extragalactic distance ladder",
"a slightly adjusted... | [
"astronomical databases: miscellaneous",
"distance scale",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 15 | [
"10.1088/0004-6256/147/5/122",
"10.48550/arXiv.1403.3141"
] | [
"de Grijs, Richard",
"Wicker, James E.",
"Bono, Giuseppe"
] | [
"Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, China; Department of Astronomy, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, China",
"National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, ... | [
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745666 | 1403.6552 | The circulation of dust in protoplanetary discs and the initial conditions of planet formation | We examine the consequences of a model for the circulation of solids in a protoplanetary nebula in which aerodynamic drag is counterbalanced by the recycling of material to the outer disc by a protostellar outflow or a disc wind. This population of circulating dust eventually becomes unstable to the formation of planet... | [
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-0.013869... | 9.674417 | 13.688652 | 2014-03-01 | 15 | 2014MNRAS.440.3545H | [
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"planets and satellites: formation",
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] | 2 | [
"10.1093/mnras/stu471",
"10.48550/arXiv.1403.6552"
] | [
"Hansen, Bradley M. S."
] | [
"Department of Physics & Astronomy, University of California Los Angeles, Los Angeles, CA 90095, USA"
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"2014ApJ...794...11I",
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800016 | 1403.6078 | Higgs inflation at the critical point | Higgs inflation can occur if the Standard Model (SM) is a self-consistent effective field theory up to inflationary scale. This leads to an upper bound on the top Yukawa coupling, ytphys<ytcrit and thus on the mass of the top quark m<SUB>t</SUB>. If m<SUB>t</SUB> is more than a few hundred of MeV below the critical ... | [
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... | [
"High Energy Physics - Phenomenology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Theory"
] | 17 | [
"10.1016/j.physletb.2014.05.074",
"10.48550/arXiv.1403.6078"
] | [
"Bezrukov, Fedor",
"Shaposhnikov, Mikhail"
] | [
"CERN, CH-1211 Genève 23, Switzerland",
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818322 | 1403.4885 | Experimental Demonstration of an Inertial Collimation Mechanism in Nested Outflows | Interaction between a central outflow and a surrounding wind is common in astrophysical sources powered by accretion. Understanding how the interaction might help to collimate the inner central outflow is of interest for assessing astrophysical jet formation paradigms. In this context, we studied the interaction betwee... | [
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"astrophysical jet formation paradigms",
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"a dedicated phase plate",
"two nested supersonic plasma flows",
"a solid target",
"strongly collimated jets",
"a long-pulse high... | [
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"X-ray and gamma-ray measurements",
"Jets outflows and bipolar flows",
"Astrophysics - High Energy Astrophysical Phenomen... | 2 | [
"10.1103/PhysRevLett.112.155001",
"10.48550/arXiv.1403.4885"
] | [
"Yurchak, R.",
"Ravasio, A.",
"Pelka, A.",
"Pikuz, S.",
"Falize, E.",
"Vinci, T.",
"Koenig, M.",
"Loupias, B.",
"Benuzzi-Mounaix, A.",
"Fatenejad, M.",
"Tzeferacos, P.",
"Lamb, D. Q.",
"Blackman, E. G."
] | [
"LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France",
"LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France",
"LULI, Ecole Polytechnique, CNRS, CEA, UPMC, Route de Saclay, 91128 Palaiseau, France",
"Joint Institute for High Temperatures RAS, 13... | [
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524282 | 1403.1372 | Kepler-9 revisited 60% the mass with six times more data | Kepler-9 was the first case where transit timing variations have been used to confirm the planets in this system. Following predictions of dramatic TTVs - larger than a week - we re-analyse the system based on the full Kepler data set. We re-processed all available data for Kepler-9 removing short and long term trends,... | [
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-0.... | 7.219191 | 13.881907 | 2014-03-01 | 14 | 2014arXiv1403.1372D | [
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] | 16 | [
"10.48550/arXiv.1403.1372"
] | [
"Dreizler, Stefan",
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"-"
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437638 | 1403.1199 | Time delays between Fermi-LAT and GBM light curves of gamma-ray bursts | <BR /> Aims: Most gamma-ray bursts (GRBs) detected by the Fermi Gamma-ray Space Telescope exhibit a delay of up to about 10 seconds between the trigger time of the hard X-ray signal as measured by the Fermi Gamma-ray Burst Monitor (GBM) and the onset of the MeV-GeV counterpart detected by the Fermi Large Area Telescope... | [
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"time lags",
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... | [
"cosmology: observations",
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] | 7 | [
"10.1051/0004-6361/201322636",
"10.48550/arXiv.1403.1199"
] | [
"Castignani, G.",
"Guetta, D.",
"Pian, E.",
"Amati, L.",
"Puccetti, S.",
"Dichiara, S."
] | [
"SISSA-ISAS, via Bonomea 265, 34136, Trieste, Italy",
"Osservatorio Astronomico di Roma, via Frascati 33, 00040, Monteporzio Catone, Italy; Department of Physics and Optical Engineering, ORT Braude, PO Box 78, Carmiel, Israel",
"INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna, via Gobetti 101, ... | [
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814707 | 1403.3225 | Cusps and pseudocusps in strings with Y-junctions | We study the occurrence of cuspy events on a light string stretched between two Y-junctions with fixed heavy strings. We first present an analytic study and give a solid criterion to discriminate between cuspy and noncuspy string configurations. We then describe a numerical code, built to test this analysis. Our numeri... | [
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0.0240... | 10.358698 | -1.711409 | 2014-03-01 | 6 | 2014PhRvD..90l3517E | [
"fixed heavy strings",
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"the string networks parameters",
"the strings root-mean-square velocity",
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"98.80.Cq",
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"Particle-theory and field-theory models of the early Universe",
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"High Energy Physics - Theory",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology"
] | 2 | [
"10.1103/PhysRevD.90.123517",
"10.48550/arXiv.1403.3225"
] | [
"Elghozi, Thomas",
"Nelson, William",
"Sakellariadou, Mairi"
] | [
"Department of Physics, King's College London, University of London, Strand, London WC2R 2LS, United Kingdom",
"Institute for Mathematics, Astrophysics and Particle Physics, Radboud University, Heyendaalsweg 135, Nijmegen 6525-AJ, Netherlands",
"Department of Physics, King's College London, University of London... | [
"2017PhRvD..96b3533S",
"2017PhRvD..96j4046B",
"2020JCAP...04..034A",
"2020JCAP...07..032G",
"2023JHEP...12..115F",
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653139 | 1403.3539 | Scintillating bolometers: A key for determining WIMP parameters | In the last decade direct detection Dark Matter (DM) experiments have increased enormously their sensitivity and ton-scale setups have been proposed, especially using germanium and xenon targets with double readout and background discrimination capabilities. In light of this situation, we study the prospects for determ... | [
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"29.40.Vj",
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"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Phenomenology"
] | 6 | [
"10.1142/S0217751X1443009X",
"10.48550/arXiv.1403.3539"
] | [
"Cerdeño, D. G.",
"Marcos, C.",
"Peiró, M.",
"Fornasa, M.",
"Cuesta, C.",
"García, E.",
"Ginestra, C.",
"Martínez, M.",
"Ortigoza, Y.",
"Puimedón, J.",
"Sarsa, M. L."
] | [
"Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Madrid, Spain",
"Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Madrid, Spain",
"Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Madrid, Spain",
"School of Physics and Astronomy, University of N... | [
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471967 | 1403.2015 | Challenges in nucleosynthesis of trans-iron elements | Nucleosynthesis beyond Fe poses additional challenges not encountered when studying astrophysical processes involving light nuclei. Astrophysical sites and conditions are not well known for some of the processes involved. On the nuclear physics side, different approaches are required, both in theory and experiment. The... | [
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"astrophysical processes",
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"Astrophysics - High Energy Astrophysical Phenomena",
"Nuclear Experiment",
"Nuclear Theory"
] | 7 | [
"10.1063/1.4868239",
"10.48550/arXiv.1403.2015"
] | [
"Rauscher, T."
] | [
"Centre for Astrophysics Research, School of Physics, Astronomy and Mathematics, Hatfield AL10 9AB, United Kingdom and Department of Physics, University of Basel, CH-4056 Basel, Switzerland"
] | [
"2014AIPA....4d0901B",
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746395 | 1403.1293 | A no-go theorem for direct collapse black holes without a strong ultraviolet background. | Explaining the existence of supermassive black holes larger than ∼10<SUP>9</SUP> M<SUB>⊙</SUB> at redshifts z ≳ 6 remains an open theoretical question. One possibility is that gas collapsing rapidly in pristine atomic cooling haloes (T<SUB>vir</SUB> ≳ 10<SUP>4</SUP> K) produces 10<SUP>4</SUP>-10<SUP>6</SUP> M<SUB>⊙</SU... | [
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"quasars: supermassive black holes",
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] | 7 | [
"10.1093/mnrasl/slu063",
"10.48550/arXiv.1403.1293"
] | [
"Visbal, E.",
"Haiman, Z.",
"Bryan, G. L."
] | [
"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",
"Department of Astronomy, Columbia University, 550 West 120th Street, New York, NY 10027, USA"
] | [
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437569 | 1403.1400 | IGR J17488-2338: a newly discovered giant radio galaxy | We present the discovery of a large-scale radio structure associated with IGR J17488-2338, a source recently discovered by INTEGRAL and optically identified as a broad-line AGN at redshift 0.24. At low frequencies, the source properties are those of an intermediate-power FR II radio galaxy with a linear size of 1.4 Mpc... | [
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-0.04567387327551842... | 15.340584 | 5.767642 | 2014-03-01 | 16 | 2014A&A...565A...2M | [
"radio galaxies",
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"IGR J17488",
"useful laboratories",
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"other properties",
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"gamma rays: galaxies",
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] | 2 | [
"10.1051/0004-6361/201423609",
"10.48550/arXiv.1403.1400"
] | [
"Molina, M.",
"Bassani, L.",
"Malizia, A.",
"Bird, A. J.",
"Bazzano, A.",
"Ubertini, P.",
"Venturi, T."
] | [
"IASF/INAF, via Gobetti 101, 40129, Bologna, Italy",
"IASF/INAF, via Gobetti 101, 40129, Bologna, Italy",
"IASF/INAF, via Gobetti 101, 40129, Bologna, Italy",
"School of Physics and Astronomy, University of Southampton, SO17 1, BJ Southampton, UK",
"IAPS/INAF, via Fosso del Cavaliere 100, 00133, Roma, Italy... | [
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527220 | 1403.6827 | Statistics of Dark Matter Substructure: I. Model and Universal Fitting Functions | We present a new, semi-analytical model describing the evolution of dark matter subhaloes. The model uses merger trees constructed using the method of Parkinson et al. (2008) to describe the masses and redshifts of subhaloes at accretion, which are subsequently evolved using a simple model for the orbit-averaged mass l... | [
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"halo dynamical times",
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"redshifts",
"the average subhalo mass and velocity functions",
"an a... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 8 | [
"10.48550/arXiv.1403.6827"
] | [
"Jiang, Fangzhou",
"van den Bosch, Frank C."
] | [
"-",
"-"
] | [
"2014MNRAS.445.1713V",
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693822 | 1403.2918 | Higgsphobic and fermiophobic Z' as a single dark matter candidate | A spin-1 Z' particle as a single dark matter candidate is investigated by assuming that it does not directly couple to the Higgs boson and standard model fermions and does not mix with the photon and Z boson. The remaining dominant vertices are quartic Z <SUP>'</SUP> Z <SUP>'</SUP> ZZ and Z <SUP>'</SUP> Z <SUP>'</SUP> ... | [
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0.027... | 8.380244 | -1.811694 | 2014-03-01 | 10 | 2014JHEP...05..088C | [
"Z boson",
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"Z",
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"standard-model gauge-boson loops",
"a dark Z",
"the Higgs boson",
"W",
"a single dark matter candidate",
"A spin-1 Z particle",
"the cosmological thermal relic density",
"direct ... | [
"Beyond Standard Model",
"Cosmology of Theories beyond the SM",
"High Energy Physics - Phenomenology",
"Astrophysics - High Energy Astrophysical Phenomena",
"High Energy Physics - Experiment"
] | 2 | [
"10.1007/JHEP05(2014)088",
"10.48550/arXiv.1403.2918"
] | [
"Chen, Nan",
"Zhang, Ying",
"Wang, Qing",
"Cacciapaglia, Giacomo",
"Deandrea, Aldo",
"Panizzi, Luca"
] | [
"Department of Physics, Tsinghua University",
"School of Science, Xi'an Jiaotong University",
"Department of Physics, Tsinghua University; Center for High Energy Physics, Tsinghua University",
"Université de Lyon; , Université Lyon 1, Villeurbanne, CNRS/IN2P3, UMR5822, Institut de Physique Nucléaire de Lyon",... | [
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483876 | 1403.2129 | Fermi Bubbles Inflated by Winds Launched from the Hot Accretion Flow in Sgr A* | A pair of giant gamma-ray Bubbles has been revealed by Fermi-LAT. In this paper we investigate their formation mechanism. Observations have indicated that the activity of the supermassive black hole located at the Galactic center, Sgr A*, was much stronger than at the present time. Specifically, one possibility is that... | [
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... | 7.757503 | 4.439316 | 2014-03-01 | 80 | 2014ApJ...790..109M | [
"hot accretion flows",
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"SUP>7</SUP",
"CMZ gas",
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"Galactic",
"recent magnetohydrodynamic numerical simulations",
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"the hot accretion regime",
"years ago",
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"the past ~10",
"the wind orientation",
"Observatio... | [
"accretion",
"accretion disks",
"black hole physics",
"galaxies: active",
"galaxies: jets",
"Galaxy: nucleus",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Astrophysics of Galaxies"
] | 14 | [
"10.1088/0004-637X/790/2/109",
"10.48550/arXiv.1403.2129"
] | [
"Mou, Guobin",
"Yuan, Feng",
"Bu, Defu",
"Sun, Mouyuan",
"Su, Meng"
] | [
"Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China; University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing 100049, China;",
"Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China",
"Shanghai Astron... | [
"2015ApJ...799L...7F",
"2015ApJ...802...91T",
"2015ApJ...804..101Y",
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745538 | 1403.0589 | The Herschel Fornax Cluster Survey II: FIR properties of optically selected Fornax cluster galaxies | The Herschel Fornax Cluster Survey is a deep, far-infrared (FIR) survey of the Fornax cluster. The survey is in five Herschel bands (100-500 μm) and covers an area of 16 deg<SUP>2</SUP> centred on NGC 1399. This paper presents photometry, detection rates, dust masses, and temperatures using an optically selected sample... | [
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-0.... | 10.476242 | 7.690213 | 2014-03-01 | 11 | 2014MNRAS.440.1571F | [
"dust masses",
"galaxies",
"Fornax",
"NGC",
"temperature",
"temperatures",
"FIR",
"The Herschel Fornax Cluster Survey",
"little effect",
"E/S0",
"a mean dust mass",
"stars",
"the Herschel Virgo Cluster Survey",
"Herschel",
"the Fornax Cluster Catalogue",
"the Fornax cluster",
"detect... | [
"galaxies: clusters: individual: Fornax",
"galaxies: ISM",
"galaxies: photometry",
"infrared: galaxies",
"Astrophysics - Astrophysics of Galaxies"
] | 9 | [
"10.1093/mnras/stu369",
"10.48550/arXiv.1403.0589"
] | [
"Fuller, C.",
"Davies, J. I.",
"Auld, R.",
"Smith, M. W. L.",
"Baes, M.",
"Bianchi, S.",
"Bocchio, M.",
"Boselli, A.",
"Clemens, M.",
"Davis, T. A.",
"De Looze, I.",
"di Serego Alighieri, S.",
"Grossi, M.",
"Hughes, T. M.",
"Viaene, S.",
"Serra, P."
] | [
"School of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3AA, UK",
"School of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3AA, UK",
"School of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3AA, UK",
"School of Physics and Astronomy, Cardiff U... | [
"2014MNRAS.442.1286H",
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573768 | 1403.7360 | Does the energy of type IIP supernovae depend on the stellar mass? | The oxygen density in the central zone of the ejecta of nine type IIP supernovae (SNe IIP) at the nebular phase has been determined from the [O I] 6300, 6364 Å doublet lines. In combination with the known estimates for two supernovae, the results of measurements show that the oxygen densities on day 300 are distributed... | [
0.011007408611476421,
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0.0... | 2.902444 | 4.865455 | 2014-03-01 | 10 | 2014AstL...40..291C | [
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"Analysis",
"combination",
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"supernovae and supernova remnants",
"stars-structure and evolution",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Solar and Stellar Astrophysics"
] | 7 | [
"10.1134/S1063773714050016",
"10.48550/arXiv.1403.7360"
] | [
"Chugai, N. N.",
"Utrobin, V. P."
] | [
"Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia; Institute for Theoretical and Experimental Physics, Moscow, Russia",
"Institute of Astronomy, Russian Academy of Sciences, Moscow, Russia; Institute for Theoretical and Experimental Physics, Moscow, Russia"
] | [
"2015MNRAS.453..287M",
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"2019MNRAS.489..641M",
"2020MNRAS.495.3751C",
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678189 | 1403.0898 | Probing non-standard gravity with the growth index: a background independent analysis | Measurements of the growth index of linear matter density fluctuations γ(z) provide a clue as to whether Einstein's field equations encompass gravity also on large cosmic scales, those where the expansion of the universe accelerates. We show that the information encoded in this function can be satisfactorily parameteri... | [
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-... | 11.188595 | 1.51499 | 2014-03-01 | 40 | 2014JCAP...05..042S | [
"various cosmological models",
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"parameterized post-Friedmann cosmological models",
"alternatives model",
"models",
"different growth rate histories",
"growth data",
"relevant cosmological scenarios",
"gravity",
"γ",
"predictions",
"most dark energy and dark gravity... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 5 | [
"10.1088/1475-7516/2014/05/042",
"10.48550/arXiv.1403.0898"
] | [
"Steigerwald, Heinrich",
"Bel, Julien",
"Marinoni, Christian"
] | [
"Aix Marseille Université, Université de Toulon, CNRS, CPT UMR 7332, 13288, Marseille, France",
"INAF — Osservatorio Astronomico di Brera, Via Brera 28, Milano, via Bianchi 46, 23807 Merate, Italy",
"Aix Marseille Université, Université de Toulon, CNRS, CPT UMR 7332, 13288, Marseille, France; Institut Universit... | [
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481738 | 1403.2586 | Remote sensing of clouds and aerosols with cosmic rays | Remote sensing of atmosphere is conventionally done via a study of extinction/scattering of light from natural (Sun, Moon) or artificial (laser) sources. Cherenkov emission from extensive air showers generated by cosmic rays provides one more natural light source distributed throughout the atmosphere. We show that Cher... | [
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"atmosphere",
"scattering phase function",
"Cherenkov light",
"cosmic rays",
"one more natural light source",
"Cherenkov telescopes",
"light",
"cloud/aerosol particles",
"atmospheric science",
"extensive air showers",
"Cherenkov emission",
"Moon",
"aerosols",
"astronomical gamma-ray observ... | [
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - High Energy Astrophysical Phenomena",
"Physics - Atmospheric and Oceanic Physics"
] | 5 | [
"10.1016/j.astropartphys.2014.03.005",
"10.48550/arXiv.1403.2586"
] | [
"Neronov, Andrii",
"Malyshev, Denys",
"Dmytriiev, Anton"
] | [
"ISDC Data Centre for Astrophysics, Astronomy Department, Geneva University, Ch. d'Ecogia 16, Versoix 1290, Switzerland",
"ISDC Data Centre for Astrophysics, Astronomy Department, Geneva University, Ch. d'Ecogia 16, Versoix 1290, Switzerland",
"Physics Department, Taras Shevchenko National University of Kyiv, G... | null | [
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] |
484688 | 1403.7195 | The Gemini NICI Planet-Finding Campaign: The Orbit of the Young Exoplanet β Pictoris b | We present new astrometry for the young (12-21 Myr) exoplanet β Pictoris b taken with the Gemini/NICI and Magellan/MagAO instruments between 2009 and 2012. The high dynamic range of our observations allows us to measure the relative position of β Pic b with respect to its primary star with greater accuracy than previou... | [
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-0.03653755784034729... | 8.234223 | 13.086057 | 2014-03-01 | 40 | 2014ApJ...794..158N | [
"semi-major axis",
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"previous observations",
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"P.A.",
"the warped inner disk P.A.",
"greater accuracy",
"NICIs semi-transparent focal plane mask",
"an orbital semi-major axis",
"higher precision determination",
"β Pictoris ... | [
"planetary systems",
"planet-disk interactions",
"planets and satellites: detection",
"stars: individual: β Pic",
"Astrophysics - Earth and Planetary Astrophysics"
] | 7 | [
"10.1088/0004-637X/794/2/158",
"10.48550/arXiv.1403.7195"
] | [
"Nielsen, Eric L.",
"Liu, Michael C.",
"Wahhaj, Zahed",
"Biller, Beth A.",
"Hayward, Thomas L.",
"Males, Jared R.",
"Close, Laird M.",
"Morzinski, Katie M.",
"Skemer, Andrew J.",
"Kuchner, Marc J.",
"Rodigas, Timothy J.",
"Hinz, Philip M.",
"Chun, Mark",
"Ftaclas, Christ",
"Toomey, Dougl... | [
"Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA",
"Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA",
"European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile",
"Institute for Astron... | [
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"2016A&A...587A..55V",
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"2016A&A...593A..74S",
"2016A&A...595A.... | [
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526370 | 1403.5229 | Redshift and redshift-drift in $\Lambda = 0$ quasi-spherical Szekeres cosmological models and the effect of averaging | Since the advent of the accelerated expanding homogeneous universe model, some other explanations for the supernova Ia dimming have been explored, among which there are inhomogeneous models constructed with exact $\Lambda = 0$ solutions of Einstein's equations. They have been used either as one patch or to build Swiss-... | [
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... | 11.194542 | 1.527693 | 2014-03-01 | 10 | 2014arXiv1403.5229M | [
"spherical LTB models",
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"homogeneous universe model",
"dark energy",
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"an unphysical QSS model",
"Swiss-cheese models",
"a QSS model",
"this QSS model",
"non spherical voids",
"a physical model",
"(BSQSS model",
"the BSQSS model",... | [
"Astrophysics - Cosmology and Extragalactic Astrophysics"
] | 3 | [
"10.48550/arXiv.1403.5229"
] | [
"Mishra, Priti",
"Célérier, Marie-Noëlle"
] | [
"-",
"-"
] | [
"2014PhRvD..90l3536P",
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"2021OJAp....4E...9F",
"2021PhRvD.103b3537H",
"2022CQGra..39a5011G",
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746131 | 1403.2409 | Satellite abundances around bright isolated galaxies - II. Radial distribution and environmental effects | We use the Eighth Data Release of the Sloan Digital Sky Survey (SDSS/DR8) galaxy sample to study the radial distribution of satellite galaxies around isolated primaries, comparing to semi-analytic models of galaxy formation based on the Millennium and Millennium-II simulations. SDSS satellites behave differently around... | [
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-0.02... | 10.885924 | 6.039719 | 2014-03-01 | 79 | 2014MNRAS.442.1363W | [
"blue satellites",
"satellite profiles",
"satellite galaxies",
"most satellites",
"SDSS satellites",
"isolated primaries",
"strong environmental effects",
"primaries",
"environmental effects",
"current semi-analytic simulations",
"semi-analytic models",
"galaxy formation",
"the few blue sate... | [
"galaxies: abundances",
"galaxies: evolution",
"galaxies: haloes",
"dark matter",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 12 | [
"10.1093/mnras/stu988",
"10.48550/arXiv.1403.2409"
] | [
"Wang, Wenting",
"Sales, Laura V.",
"Henriques, Bruno M. B.",
"White, Simon D. M."
] | [
"Max Planck Institut fur Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching b. München, Germany; Key Laboratory for Research in Galaxies and Cosmology of Chinese Academy of Sciences, Max-Panck-Institute Partner Group, Shanghai Astronomical Observatory, Nandan Road 80, Shanghai 200030, China; Institute for Com... | [
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483088 | 1403.3063 | Major Cluster Mergers and the Location of the Brightest Cluster Galaxy | Using a large N-body cosmological simulation combined with a subgrid treatment of galaxy formation, merging, and tidal destruction, we study the formation and evolution of the galaxy and cluster population in a comoving volume (100 Mpc)<SUP>3</SUP> in a ΛCDM universe. At z = 0, our computational volume contains 1788 cl... | [
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-0.00186... | 12.418479 | 5.537112 | 2014-03-01 | 41 | 2014ApJ...786...79M | [
"clusters",
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"galaxies",
"the brightest cluster galaxy",
"major mergers",
"high-cluster mass",
"high-mass clusters",
"low-mass clusters",
"BCG",
"SUB>⊙</SUB",
"18 massive clusters",
"only massive clusters",
"the whole cluster",
"radial velocity",
... | [
"galaxies: clusters: general",
"galaxies: general",
"methods: numerical",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 21 | [
"10.1088/0004-637X/786/2/79",
"10.48550/arXiv.1403.3063"
] | [
"Martel, Hugo",
"Robichaud, Fidèle",
"Barai, Paramita"
] | [
"Département de physique, Génie Physique et Optique, Université Laval, Québec, QC, G1V 0A6, Canada; Centre de Recherche en Astrophysique du Québec, QC, H3C 3J7, Canada;",
"Département de physique, Génie Physique et Optique, Université Laval, Québec, QC, G1V 0A6, Canada; Centre de Recherche en Astrophysique du Qué... | [
"2014ApJ...789L..31W",
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653142 | 1403.3580 | Analysis of the <SUP>40</SUP>K contamination in NaI(Tl) crystals from different providers in the frame of the ANAIS project | NaI(Tl) large crystals are applied in the search for galactic dark matter particles through their elastic scattering off the target nuclei in the detector by measuring the scintillation signal produced. However, energies deposited in the form of nuclear recoils are small, which added to the low efficiency to convert th... | [
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... | 7.302722 | -2.760785 | 2014-03-01 | 21 | 2014IJMPA..2943010C | [
"electron equivalent energy",
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"scintillation events",
"dark matter search project",
"nonbulk NaI(Tl",
"large sodium iodide detectors",
"large crystals",
"NaI(Tl",
"radioactive backgrounds",
"events",
"scintillation",
"crystals",
"detectors",
"the ANAIS dark matter search experi... | [
"Sodium iodide",
"scintillation",
"potassium",
"dark matter search",
"annual modulation",
"29.40.Mc",
"29.40.Wk",
"95.35.+d",
"Scintillation detectors",
"Solid-state detectors",
"Dark matter",
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - Cosmology and Nongal... | 7 | [
"10.1142/S0217751X14430106",
"10.48550/arXiv.1403.3580"
] | [
"Cuesta, C.",
"Amaré, J.",
"Cebrián, S.",
"García, E.",
"Ginestra, C.",
"Martínez, M.",
"Oliván, M. A.",
"Ortigoza, Y.",
"Ortiz de Solórzano, A.",
"Pobes, C.",
"Puimedón, J.",
"Sarsa, M. L.",
"Villar, J. A.",
"Villar, P."
] | [
"Laboratorio Subterráneo de Canfranc, Paseo de los Ayerbe s.n., 22880 Canfranc Estación, Huesca, Spain",
"Laboratorio Subterráneo de Canfranc, Paseo de los Ayerbe s.n., 22880 Canfranc Estación, Huesca, Spain",
"Laboratorio Subterráneo de Canfranc, Paseo de los Ayerbe s.n., 22880 Canfranc Estación, Huesca, Spain... | [
"2014EPJC...74.3150C",
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] |
746917 | 1403.1585 | The evolution of the star-forming sequence in hierarchical galaxy formation models | It has been argued that the specific star formation rates of star-forming galaxies inferred from observational data decline more rapidly below z = 2 than is predicted by hierarchical galaxy formation models. We present a detailed analysis of this problem by comparing predictions from the GALFORM semi-analytic model wit... | [
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-0.00... | 11.950542 | 6.658822 | 2014-03-01 | 58 | 2014MNRAS.444.2637M | [
"hierarchical galaxy formation models",
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"star formation",
"galaxy haloes",
"stellar mass assembly histories",
"observational data",
"star-forming galaxies",
"data",
"the predicted star formation rates",
"the average star formation rates",
"the specific sta... | [
"galaxies: evolution",
"galaxies: formation",
"galaxies: star formation",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 5 | [
"10.1093/mnras/stu1639",
"10.48550/arXiv.1403.1585"
] | [
"Mitchell, Peter D.",
"Lacey, Cedric G.",
"Cole, Shaun",
"Baugh, Carlton M."
] | [
"Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK",
"Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK",
"Institute for Computational Cosmology, Department of Physics, University of... | [
"2014ApJ...795..104W",
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480937 | 1403.1066 | Star Formation Rates in Nearby Markarian Galaxies | The star formation rates for the 230 nearest Markarian galaxies with radial velocities V<SUB>LG</SUB> < 3500 km/s have been determined from their far ultraviolet fluxes obtained with the GALEX satellite. We briefly discuss the observed relationship between the star formation rate and other integral parameters of the... | [
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] | 5 | [
"10.1007/s10511-014-9310-4",
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] | [
"Karachentseva, V. E.",
"Melnyk, O. V.",
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] | [
"Main Astronomical Observatory, National Academy of Sciences of Ukraine, Kiev, Ukraine",
"Astronomical Observatory of Taras Shevchenko Kiev National University, Kiev, Ukraine; Institut d'Astrophysique et de Geophysique, Universite de Liege, Liege, Belgium",
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483610 | 1403.6470 | Evidence of Very Low Metallicity and High Ionization State in a Strongly Lensed, Star-forming Dwarf Galaxy at z= 3.417 | We investigate the gas-phase metallicity and Lyman continuum (LyC) escape fraction of a strongly gravitationally lensed, extreme emission-line galaxy at z = 3.417, J1000+0221S, recently discovered by the CANDELS team. We derive ionization- and metallicity-sensitive emission-line ratios from H+K band Large Binocular Tel... | [
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"galaxies: abundances",
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"galaxies: high-redshift",
"galaxies: starburst",
"gravitational lensing: strong",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 6 | [
"10.1088/2041-8205/788/1/L4",
"10.48550/arXiv.1403.6470"
] | [
"Amorín, R.",
"Grazian, A.",
"Castellano, M.",
"Pentericci, L.",
"Fontana, A.",
"Sommariva, V.",
"van der Wel, A.",
"Maseda, M.",
"Merlin, E."
] | [
"INAF—Osservatorio Astronomico di Roma, via Frascati 33, I-00040 Monteporzio Catone, Roma, Italy; ASTRODEEP fellow.;",
"INAF—Osservatorio Astronomico di Roma, via Frascati 33, I-00040 Monteporzio Catone, Roma, Italy",
"INAF—Osservatorio Astronomico di Roma, via Frascati 33, I-00040 Monteporzio Catone, Roma, Ita... | [
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12359417 | 1403.6745 | Instabilities in the Envelopes and Winds of Very Massive Stars | The high luminosity of Very Massive Stars (VMS) means that radiative forces play an important, dynamical role both in the structure and stability of their stellar envelope, and in driving strong stellar-wind mass loss. Focusing on the interplay of radiative flux and opacity, with emphasis on key distinctions between co... | [
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] | 5 | [
"10.1007/978-3-319-09596-7_5",
"10.48550/arXiv.1403.6745"
] | [
"Owocki, Stanley P."
] | [
"Department of Physics & Astronomy, University of Delaware"
] | [
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12311653 | 1403.1299 | Radiogenic and muon-induced backgrounds in the LUX dark matter detector | The Large Underground Xenon (LUX) dark matter experiment aims to detect rare low-energy interactions from Weakly Interacting Massive Particles (WIMPs). The radiogenic backgrounds in the LUX detector have been measured and compared with Monte Carlo simulation. Measurements of LUX high-energy data have provided direct co... | [
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"10.1016/j.astropartphys.2014.07.009",
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"Akerib, D. S.",
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"Carmona-Benitez, M. C.",
"Chan, C.",
"Chapman, J. J.",
"Chiller, A. A.",
"Chiller, C.",
"Coffey, T.",
"Currie, A.",
"de Viveiros... | [
"Case Western Reserve University, Dept. of Physics, 10900 Euclid Ave, Cleveland, OH 44106, USA",
"Imperial College London, High Energy Physics, Blackett Laboratory, London SW7 2BZ, UK",
"South Dakota School of Mines and Technology, 501 East St Joseph St., Rapid City, SD 57701, USA",
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437571 | 1403.1250 | The supernova remnant W44: Confirmations and challenges for cosmic-ray acceleration | The middle-aged supernova remnant (SNR) W44 has recently attracted attention because of its relevance regarding the origin of Galactic cosmic-rays. For the first time for a SNR, the gamma-ray missions AGILE and Fermi have established the spectral continuum below 200 MeV, which can be attributed to a neutral pion emissi... | [
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... | [
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] | 7 | [
"10.1051/0004-6361/201322685",
"10.48550/arXiv.1403.1250"
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"Cardillo, M.",
"Tavani, M.",
"Giuliani, A.",
"Yoshiike, S.",
"Sano, H.",
"Fukuda, T.",
"Fukui, Y.",
"Castelletti, G.",
"Dubner, G."
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"INAF/IAPS, 00133, Roma, Italy ; Dip. di Fisica, Univ. Tor Vergata, 00133, Roma, Italy",
"INAF/IAPS, 00133, Roma, Italy; Dip. di Fisica, Univ. Tor Vergata, 00133, Roma, Italy; CIFS-Torino, 10133, Torino, Italy",
"CIFS-Torino, 10133, Torino, Italy; INAF/IASF-Milano, 20133, Milano, Italy",
"Department of Physic... | [
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595817 | 1403.2190 | The Hantzsche-Wendt manifold in cosmic topology | The Hantzsche-Wendt space is one of the 17 multiply connected spaces of the three-dimensional Euclidean space ${{\mathbb{E}}^{3}}$ E 3 . It is a compact and orientable manifold which can serve as a model for a spatial finite universe. Since it possesses much fewer matched back-to-back circle pairs on the cosmic microwa... | [
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0.0... | 12.47508 | 0.684897 | 2014-03-01 | 10 | 2014CQGra..31p5009A | [
"matched circle pairs",
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] | 10 | [
"10.1088/0264-9381/31/16/165009",
"10.48550/arXiv.1403.2190"
] | [
"Aurich, R.",
"Lustig, S."
] | [
"Institut für Theoretische Physik, Universität Ulm, Albert-Einstein-Allee 11, D-89069 Ulm, Germany",
"Institut für Theoretische Physik, Universität Ulm, Albert-Einstein-Allee 11, D-89069 Ulm, Germany"
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12404269 | 1403.7898 | A note on the puzzling spindown behavior of the Galactic center magnetar SGR J1745-2900 | SGR J1745-2900 is a magnetar near the Galactic center. X-ray observations of this source found a decreasing X-ray luminosity accompanied by an enhanced spindown rate. This negative correlation between X-ray luminosity and spindown rate is hard to understand. The wind braking model of magnetars is employed to explain th... | [
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0... | 5.338708 | 4.091697 | 2014-03-01 | 9 | 2015RAA....15.1467T | [
"X-ray luminosity",
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"Astrophysics - High Energy Astrophysical Phenomena"
] | 9 | [
"10.1088/1674-4527/15/9/003",
"10.48550/arXiv.1403.7898"
] | [
"Tong, Hao"
] | [
"Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, China"
] | [
"2014arXiv1406.6458T",
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800089 | 1403.1536 | X-ray line signal from 7 keV axino dark matter decay | Recently a weak X-ray emission around E<SUB>γ</SUB>≃3.5 keV was detected in the Andromeda galaxy and various galaxy clusters including the Perseus galaxy cluster but its source has been unidentified. Axino, the superpartner of axion, with a mass 2E<SUB>γ</SUB> is suggested as a possible origin of the line with R-parity... | [
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"High Energy Physics - Phenomenology",
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"Astrophysics - Astrophysics of Galaxies",
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] | 5 | [
"10.1016/j.physletb.2014.04.037",
"10.48550/arXiv.1403.1536"
] | [
"Park, Jong-Chul",
"Kong, Kyoungchul",
"Park, Seong Chan"
] | [
"Department of Physics and Astronomy, University of Kansas, Lawrence, KS 66045, USA",
"Department of Physics and Astronomy, University of Kansas, Lawrence, KS 66045, USA",
"Department of Physics, Sungkyunkwan University, Suwon 440-746, Republic of Korea"
] | [
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812382 | 1403.1193 | Primordial magnetic helicity from stochastic electric currents | We study the possibility that primordial magnetic fields generated in the transition between inflation and reheating posses magnetic helicity, H<SUB>M</SUB>. The fields are induced by stochastic currents of scalar charged particles created during the mentioned transition. We estimate the rms value of the induced magnet... | [
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0... | 12.036351 | -0.793186 | 2014-03-01 | 7 | 2014PhRvD..89h3012C | [
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"structure formation",
"scalar charged particles",
"random fields",
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] | 3 | [
"10.1103/PhysRevD.89.083012",
"10.48550/arXiv.1403.1193"
] | [
"Calzetta, Esteban",
"Kandus, Alejandra"
] | [
"Departamento de Física and IFIBA, FCEyN—UBA, Ciudad Universitaria, C1428EGA Ciudad Autónoma de Buenos Aires, Argentina",
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482807 | 1403.1470 | Intensity Enhancement of O VI Ultraviolet Emission Lines in Solar Spectra due to Opacity | Opacity is a property of many plasmas. It is normally expected that if an emission line in a plasma becomes optically thick, then its intensity ratio to that of another transition that remains optically thin should decrease. However, radiative transfer calculations undertaken both by ourselves and others predict that u... | [
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0.01... | 11.563137 | 13.503696 | 2014-03-01 | 8 | 2014ApJ...784L..39K | [
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"Solar",
"the intensity ratio",
"the I(1032 Å)/I(1038 Å) intensity ... | [
"opacity",
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] | 3 | [
"10.1088/2041-8205/784/2/L39",
"10.48550/arXiv.1403.1470"
] | [
"Keenan, F. P.",
"Doyle, J. G.",
"Madjarska, M. S.",
"Rose, S. J.",
"Bowler, L. A.",
"Britton, J.",
"McCrink, L.",
"Mathioudakis, M."
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"Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK",
"Armagh Observatory, College Hill, Armagh BT61 9DG, UK",
"Armagh Observatory, College Hill, Armagh BT61 9DG, UK",
"Physics Department, Imperial College, London SW7 2BZ, UK",
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813541 | 1403.4852 | Relic neutrinos, thermal axions, and cosmology in early 2014 | We present up-to-date cosmological bounds on the sum of active neutrino masses as well as on extended cosmological scenarios with additional thermal relics, as thermal axions or sterile neutrino species. Our analyses consider all the current available cosmological data in the beginning of year 2014, including the very ... | [
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"10.1103/PhysRevD.90.043507",
"10.48550/arXiv.1403.4852"
] | [
"Giusarma, Elena",
"Di Valentino, Eleonora",
"Lattanzi, Massimiliano",
"Melchiorri, Alessandro",
"Mena, Olga"
] | [
"Physics Department and INFN, Università di Roma \"La Sapienza\", Ple Aldo Moro 2, 00185 Rome, Italy",
"Physics Department and INFN, Università di Roma \"La Sapienza\", Ple Aldo Moro 2, 00185 Rome, Italy",
"Dipartimento di Fisica e Science della Terra, Università di Ferrara and INFN, sezione di Ferrara, Polo Sc... | [
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746266 | 1403.4255 | The highest frequency detection of a radio relic: 16 GHz AMI observations of the `Sausage' cluster. | We observed the cluster CIZA J2242.8+5301 with the Arcminute Microkelvin Imager at 16 GHz and present the first high radio-frequency detection of diffuse, non-thermal cluster emission. This cluster hosts a variety of bright, extended, steep-spectrum synchrotron-emitting radio sources, associated with the intracluster m... | [
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... | 14.461491 | 4.748972 | 2014-03-01 | 33 | 2014MNRAS.441L..41S | [
"radio relics",
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] | 6 | [
"10.1093/mnrasl/slu045",
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"Stroe, A.",
"Rumsey, C.",
"Harwood, J. J.",
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"Saunders, R. D. E.",
"Sobral, D.",
"Perrott, Y. C.",
"Schammel, M. P."
] | [
"Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands",
"Astrophysics Group, Cavendish Laboratory, JJ Thomson Avenue, Cambridge CB3 0HE, UK",
"School of Physics, Astronomy and Mathematics, University of Hertfordshire, College Lane, Hatfield, Hertfordshire AL10 9AB, UK",
"Harv... | [
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697477 | 1403.4241 | WFIRST Ultra-Precise Astrometry I: Kuiper Belt Objects | I show that the WFIRST microlensing survey will enable detection and precision orbit determination of Kuiper Belt Objects (KBOs) down to H_=28.2 over an effective area of about 17 sq.deg. Typical fractional period errors will be about 1.5% x 10^(0.4(H-28.2)) with similar errors in other parameters for roughly 5000 KBOs... | [
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-0... | 7.726035 | 16.258226 | 2014-03-01 | 8 | 2014JKAS...47..279G | [
"KBO mass measurements",
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"Astrophysics - Earth and Planetary Astrophysics"
] | 8 | [
"10.5303/JKAS.2014.47.6.279",
"10.48550/arXiv.1403.4241"
] | [
"Gould, Andrew"
] | [
"Department of Astronomy, Ohio State University, 140W 18th Ave., Columbus, OH 43210, USA"
] | [
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745971 | 1403.4288 | On characterizing non-locality and anisotropy for the magnetorotational instability | The extent to which angular momentum transport in accretion discs is primarily local or non-local and what determines this is an important avenue of study for understanding accretion engines. Taking a step along this path, we analyse simulations of the magnetorotational instability (MRI) by calculating energy and stres... | [
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0.034... | 11.059539 | 13.637585 | 2014-03-01 | 17 | 2014MNRAS.441.1855N | [
"accretion discs",
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"accretion",
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] | 5 | [
"10.1093/mnras/stu706",
"10.48550/arXiv.1403.4288"
] | [
"Nauman, Farrukh",
"Blackman, Eric G."
] | [
"Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA",
"Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA"
] | [
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872556 | 1403.1652 | Variable-delay polarization modulators for cryogenic millimeter-wave applications | We describe the design, construction, and initial validation of the variable-delay polarization modulator (VPM) designed for the PIPER cosmic microwave background polarimeter. The VPM modulates between linear and circular polarization by introducing a variable phase delay between orthogonal linear polarizations. Each V... | [
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-0.... | 10.656876 | 2.824199 | 2014-03-01 | 7 | 2014RScI...85f4501C | [
"orthogonal linear polarizations",
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"VPM",
"a variable phase delay",
"the variable-delay polarization modulator",
"linear and circular polarization",
"construction",
"PIPER",
"initial validation",
"mec... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 7 | [
"10.1063/1.4879499",
"10.48550/arXiv.1403.1652"
] | [
"Chuss, D. T.",
"Eimer, J. R.",
"Fixsen, D. J.",
"Hinderks, J.",
"Kogut, A. J.",
"Lazear, J.",
"Mirel, P.",
"Switzer, E.",
"Voellmer, G. M.",
"Wollack, E. J."
] | [
"NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA",
"Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland 21218, USA",
"NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA",
"NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA",
"NA... | [
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12390023 | 1403.6244 | The Short Bursts in SGR 1806-20, 1E 1048-5937, and SGR 0501+4516 | We analyzed temporal and spectral properties, focusing on the short bursts, for three anomalous X-ray pulsars (AXPs) and soft gamma repeaters (SGRs), including SGR 1806-20, 1E 1048-5937 and SGR 0501+4516. Using the data from XMM-Newton, we located the short bursts by Bayesian blocks algorithm. The short bursts' duratio... | [
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-0.... | 5.26944 | 4.115597 | 2014-03-01 | 2 | 2015PASP..127..211Q | [
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"Astrophysics - High Energy Astrophysical Phenomena"
] | 10 | [
"10.1086/680484",
"10.48550/arXiv.1403.6244"
] | [
"Qu, Zhijie",
"Li, Zhaosheng",
"Chen, Yupeng",
"Dai, Shi",
"Ji, Long",
"Xu, Renxin",
"Zhang, Shu"
] | [
"-",
"-",
"-",
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746135 | 1403.6591 | Statistical properties of filaments in weak gravitational lensing | We study the weak lensing properties of filaments that connect clusters of galaxies through large cosmological N-body simulations. We select 4639 halo pairs with masses higher than 10<SUP>14</SUP> h<SUP>-1</SUP> M<SUB>⊙</SUB> from the simulations and investigate dark matter distributions between two haloes with ray-tra... | [
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0.01... | 12.214155 | 4.716266 | 2014-03-01 | 10 | 2014MNRAS.441..745H | [
"straight filaments",
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"convergence profiles",
"large cosmological N-body simulations",
"ray-tracing simulations",
"profile",
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"gravitational lensing: weak",
"large-scale structure of Universe",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 6 | [
"10.1093/mnras/stu583",
"10.48550/arXiv.1403.6591"
] | [
"Higuchi, Yuichi",
"Oguri, Masamune",
"Shirasaki, Masato"
] | [
"Department of Astronomy, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan; Optical and Infrared Astronomy Division, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan",
"Department of Physics, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japa... | [
"2014JCAP...07..058F",
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716623 | 1403.6628 | Large Scale Anisotropy of Cosmic Rays and Directional Neutrino Signals from Galactic Sources | We investigate the neutrino leftrightharpoons cosmic ray connection for sources in the Galaxy in terms of two observables: the shape of the energy spectrum and the distribution of arrival directions. We also study the associated gamma ray emission from these sources. | [
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... | 6.114816 | 0.611271 | 2014-03-01 | 3 | 2014JPhCS.531a2009A | [
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"the shape",
"the Galaxy",
"the neutrino leftrightharpoons",
"We",
"two"
] | [
"Astrophysics - High Energy Astrophysical Phenomena"
] | 4 | [
"10.1088/1742-6596/531/1/012009",
"10.48550/arXiv.1403.6628"
] | [
"Anchordoqui, Luis A.",
"Goldberg, Haim",
"Olinto, Angela V.",
"Paul, Thomas C.",
"Vlcek, Brian J.",
"Weiler, Thomas J."
] | [
"Department of Physics, University of Wisconsin-Milwaukee, Milwaukee, WI, 53201, USA",
"Department of Physics, Northeastern University, Boston, MA 02115, USA",
"Department of Astronomy and Astrophysics, Enrico Fermi Institute, Chicago, Il 60637, USA; Kavli Institute for Cosmological Physics, University of Chica... | [
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483117 | 1403.1008 | Satellite Alignment. I. Distribution of Substructures and their Dependence on Assembly History from N-body Simulations | Observations have shown that the spatial distribution of satellite galaxies is not random, but aligned with the major axes of central galaxies. This alignment is dependent on galaxy properties, such that red satellites are more strongly aligned than blue satellites. Theoretical work conducted to interpret this phenomen... | [
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] | 3 | [
"10.1088/0004-637X/786/1/8",
"10.48550/arXiv.1403.1008"
] | [
"Wang, Y. O.",
"Lin, W. P.",
"Kang, X.",
"Dutton, Aaron",
"Yu, Yu",
"Macciò, Andrea V."
] | [
"Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Science, 80 Nandan Road, Shanghai 200030, China ; Graduate School, University of the Chinese Academy of Sciences, 19A, Yuquan Road, Beijing, China;",
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437943 | 1403.1839 | The low-high-low trend of type III radio burst starting frequencies and solar flare hard X-rays | <BR /> Aims: Using simultaneous X-ray and radio observations from solar flares, we investigate the link between the type III radio burst starting frequency and hard X-ray spectral index. For a proportion of events the relation derived between the starting height (frequency) of type III radio bursts and the electron bea... | [
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"10.48550/arXiv.1403.1839"
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"Reid, Hamish A. S.",
"Vilmer, Nicole",
"Kontar, Eduard P."
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"LESIA, Observatoire de Paris, CNRS, UPMC, Université Paris-Diderot, 5 place Jules Janssen, 92195, Meudon Cedex, France ; SUPA School of Physics and Astronomy, University of Glasgow, G12 8QQ, UK",
"LESIA, Observatoire de Paris, CNRS, UPMC, Université Paris-Diderot, 5 place Jules Janssen, 92195, Meudon Cedex, Fran... | [
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12372041 | 1403.7132 | Simulating the H<SUB>2</SUB> content of high-redshift galaxies | We introduce a sub-grid model for the non-equilibrium abundance of molecular hydrogen in cosmological simulations of galaxy formation. We improve upon previous work by accounting for the unresolved structure of molecular clouds in a phenomenological way which combines both observational and numerical results on the pro... | [
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... | [
"methods: numerical",
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] | 8 | [
"10.1093/mnras/stu2273",
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"Tomassetti, Matteo",
"Porciani, Cristiano",
"Romano-Díaz, Emilio",
"Ludlow, Aaron D."
] | [
"Argelander Institut für Astronomie, Auf Dem Hügel 71, D-53121 Bonn, Germany",
"Argelander Institut für Astronomie, Auf Dem Hügel 71, D-53121 Bonn, Germany",
"Argelander Institut für Astronomie, Auf Dem Hügel 71, D-53121 Bonn, Germany",
"Argelander Institut für Astronomie, Auf Dem Hügel 71, D-53121 Bonn, Germ... | [
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628174 | 1403.7418 | A digital method to calculate the true areas of sunspot groups | The areas of sunspots are the most prominent feature of the development of sunspot groups. Since the size of sunspot areas depend on the strength of the magnetic field, accurate measurements of these areas are important. In this study, a method which allows to measure true areas of the sunspots is introduced. A Stonyhu... | [
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] | 5 | [
"10.1007/s10686-014-9381-6",
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"Çakmak, H."
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"Faculty of Science, Department of Astronomy and Space Sciences, Istanbul University, Istanbul, Turkey"
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747309 | 1403.5137 | Heating cold clumps by jet-inflated bubbles in cooling flow clusters | We simulate the evolution of dense-cool clumps embedded in the intracluster medium (ICM) of cooling flow clusters of galaxies in response to multiple jet-activity cycles, and find that the main heating process of the clumps is mixing with the hot shocked jets' gas, the bubbles, while shocks have a limited role. We use ... | [
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0... | 14.267425 | 5.294149 | 2014-03-01 | 25 | 2014MNRAS.445.4161H | [
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"radiative cooling",
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"galaxies: clusters: general",
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] | 3 | [
"10.1093/mnras/stu2047",
"10.48550/arXiv.1403.5137"
] | [
"Hillel, Shlomi",
"Soker, Noam"
] | [
"Department of Physics, Technion - Israel Institute of Technology, Haifa 32000, Israel",
"Department of Physics, Technion - Israel Institute of Technology, Haifa 32000, Israel"
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813180 | 1403.5301 | Revealing the high-density equation of state through binary neutron star mergers | We present a novel method for revealing the equation of state of high-density neutron star matter through gravitational waves emitted during the postmerger phase of a binary neutron star system. The method relies on a small number of detections of the peak frequency in the postmerger phase for binaries of different (re... | [
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0.... | 6.154749 | 2.268913 | 2014-03-01 | 119 | 2014PhRvD..90b3002B | [
"typical neutron star masses",
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"10.1103/PhysRevD.90.023002",
"10.48550/arXiv.1403.5301"
] | [
"Bauswein, A.",
"Stergioulas, N.",
"Janka, H. -T."
] | [
"Department of Physics, Aristotle University of Thessaloniki, GR-54124 Thessaloniki, Greece",
"Department of Physics, Aristotle University of Thessaloniki, GR-54124 Thessaloniki, Greece",
"Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany"
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481745 | 1403.7597 | Surrounding material effect on measurement of thunderstorm-related neutrons | Observations of strong flux of low-energy neutrons were made by 3He counters during thunderstorms (Gurevich et al., 2012) [11]. How the unprecedented enhancements were produced remains elusive. To better elucidate the mechanism, a simulation study of surrounding material impacts on measurement by 3He counters was perfo... | [
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... | 6.520535 | -0.584857 | 2014-03-01 | 5 | 2014APh....57...33T | [
"gamma rays",
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"thick materials",
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"little gamma-ray contamination",
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"al.",
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"Gurevich et al",
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"Astrophysics - Earth and Planetary Astrophysics",
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] | 5 | [
"10.1016/j.astropartphys.2014.03.009",
"10.48550/arXiv.1403.7597"
] | [
"Tsuchiya, H."
] | [
"High-energy Astrophysics Laboratory, RIKEN Nishina Center, 2-1, Hirosawa, Wako, Saitama 351-0198, Japan"
] | [
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678375 | 1403.0654 | Cosmological observables in multi-field inflation with a non-flat field space | Using δN formalism, in the context of a generic multi-field inflation driven on a non-flat field space background, we revisit the analytic expressions of the various cosmological observables such as scalar/tensor power spectra, scalar/tensor spectral tilts, non-Gaussianity parameters, tensor-to-scalar ratio, and the va... | [
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"non-Gaussianity parameters",
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"observables",
"large volume scenarios",
"a non-flat field space background",
"scalar/tensor power spectra",
"scalar/tensor spectral tilts",
"a generic multi-field inflation",
"the various cosmological observables",
"the leading order slow-roll exp... | [
"High Energy Physics - Theory",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology"
] | 4 | [
"10.1088/1475-7516/2014/10/008",
"10.48550/arXiv.1403.0654"
] | [
"Gao, Xin",
"Li, Tianjun",
"Shukla, Pramod"
] | [
"State Key Laboratory of Theoretical Physics and Kavli Institute for Theoretical Physics China (KITPC), Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, P.R. China; Department of Physics, Robeson Hall, 0435, Virginia Tech, 850 West Campus Drive, Blacksburg, VA 24061, U.S.A.",
"State ... | [
"2014JCAP...10..048G",
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"2019ForPh..6700072D",
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812867 | 1403.1072 | Blocking the Hawking radiation | Some severe constraints on asymmetric dark matter are based on the scenario that certain types of weakly interacting massive particles can form mini-black holes inside neutron stars that can lead to their destruction. A crucial element for the realization of this scenario is that the black hole grows after its formatio... | [
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... | 8.908866 | -0.537206 | 2014-03-01 | 5 | 2014PhRvD..89l3519A | [
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"asymmetric dark matter",
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"Kouvaris, Chris"
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812771 | 1403.1843 | Practical, covariant puncture for second-order self-force calculations | Accurately modeling an extreme-mass-ratio inspiral requires knowledge of the second-order gravitational self-force on the inspiraling small object. Recently, numerical puncture schemes have been formulated to calculate this force, and their essential analytical ingredients have been derived from first principles. Howev... | [
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813004 | 1403.5717 | keV photon emission from light nonthermal dark matter | We propose a possible explanation for the recent claim of an excess at 3.5 keV in the x-ray spectrum within a minimal extension of the standard model that explains dark matter and baryon abundance of the Universe. The dark matter mass in this model is O(GeV) and its relic density has a nonthermal origin. The model incl... | [
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"Allahverdi, Rouzbeh",
"Dutta, Bhaskar",
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"Mitchell Institute of Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, Texas 77843-4242, USA",
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825627 | 1403.0074 | Atmospheres and radiating surfaces of neutron stars | The early 21st century is witnessing a breakthrough in the study of the thermal radiation of neutron stars. Observations with modern space telescopes have provided a wealth of valuable information, which, when properly interpreted, can elucidate the physics of superdense matter in the interior of these stars. This inte... | [
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"École Normale Supérieure de Lyon, France; Ioffe Physical Technical Institute, Russian Academy of Sciences, St. Petersburg, Russian Federation; Central Astronomical Observatory, Russian Academy of Sciences, Pulkovo, St.Petersburg, Russian Federation; Centre de Recherche Astrophysique de Lyon, Lyon, France; Universi... | [
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818554 | 1403.6786 | Electroweak Vacuum Stability in Light of BICEP2 | We consider the effect of a period of inflation with a high energy density upon the stability of the Higgs potential in the early Universe. The recent measurement of a large tensor-to-scalar ratio, r<SUB>T</SUB>∼0.16, by the BICEP2 experiment possibly implies that the energy density during inflation was very high, comp... | [
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746730 | 1403.3395 | Turbulence and cooling in galaxy cluster cores | We study the interplay between turbulent heating, mixing, and radiative cooling in an idealized model of cool cluster cores. Active galactic nuclei (AGN) jets are expected to drive turbulence and heat cluster cores. Cooling of the intracluster medium (ICM) and stirring by AGN jets are tightly coupled in a feedback loop... | [
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"Banerjee, Nilanjan",
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483303 | 1403.3676 | Spitzer IRS Observations of the XA Region in the Cygnus Loop Supernova Remnant | We report on spectra of two positions in the XA region of the Cygnus Loop supernova remnant obtained with the InfraRed Spectrograph on the Spitzer Space Telescope. The spectra span the 10-35 μm wavelength range, which contains a number of collisionally excited forbidden lines. These data are supplemented by optical spe... | [
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4520306 | 1403.6115 | Two-dimensional Core-collapse Supernova Models with Multi-dimensional Transport | We present new two-dimensional (2D) axisymmetric neutrino radiation/hydrodynamic models of core-collapse supernova (CCSN) cores. We use the CASTRO code, which incorporates truly multi-dimensional, multi-group, flux-limited diffusion (MGFLD) neutrino transport, including all relevant {O}(v/c) terms. Our main motivation ... | [
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"Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA",
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482852 | 1403.1029 | The Corona of HD 189733 and its X-Ray Activity | Testing whether close-in massive exoplanets (hot Jupiters) can enhance the stellar activity in their host primary is crucial for the models of stellar and planetary evolution. Among systems with hot Jupiters, HD 189733 is one of the best studied because of its proximity, strong activity, and the presence of a transitin... | [
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"2003ApJ...588.1... |
12410188 | 1403.0675 | Notes on Born-Infeld-like modified gravity | We investigate the modified F(R) gravity theory with the function F(R) = (1-√{1-2λ R-σ(λ R)<SUP>2</SUP>})/λ. The action is converted into Einstein-Hilbert action at small values of λ and σ. The local tests give a bound on the parameters, λ(1+σ)≤2×10^{-6} cm<SUP>2</SUP>. The Jordan and Einstein frames are considered, th... | [
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... | 10.223453 | 1.026263 | 2014-03-01 | 6 | 2016Ap&SS.361...73K | [
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"(1-√{1-2λ R-σ(λ R)<SUP>2</SUP>... | [
"modified gravity",
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"Ricci scalar",
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"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High E... | 5 | [
"10.1007/s10509-016-2665-8",
"10.48550/arXiv.1403.0675"
] | [
"Kruglov, S. I."
] | [
"Department of Chemical and Physical Sciences, University of Toronto, Mississauga, Ontario, Canada"
] | [
"2016IJMPA..3150058K",
"2017CQGra..34d5006B",
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5213591 | 1403.5266 | The old nuclear star cluster in the Milky Way: dynamics, mass, statistical parallax, and black hole mass | We derive new constraints on the mass, rotation, orbit structure, and statistical parallax of the Galactic old nuclear star cluster and the mass of the supermassive black hole. We combine star counts and kinematic data from Fritz et al., including 2500 line-of-sight velocities and 10 000 proper motions obtained with VL... | [
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0... | 8.874838 | 6.307974 | 2014-03-01 | 150 | 2015MNRAS.447..948C | [
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"the Galactic old nuclear star cluster",
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"galaxy: centre",
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] | 16 | [
"10.1093/mnras/stu2452",
"10.48550/arXiv.1403.5266"
] | [
"Chatzopoulos, S.",
"Fritz, T. K.",
"Gerhard, O.",
"Gillessen, S.",
"Wegg, C.",
"Genzel, R.",
"Pfuhl, O."
] | [
"Max Planck Institut fur Extraterrestrische Physic, Postfach 1312, D-85741 Garching Germany",
"Department of Astronomy, University of Virginia, 530 McCormick Road, Charlottesville, VA 22904-4325, USA",
"Max Planck Institut fur Extraterrestrische Physic, Postfach 1312, D-85741 Garching Germany",
"Max Planck In... | [
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745823 | 1403.2994 | Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts | We present a comparison of the physical properties of a rest-frame 250-μm-selected sample of massive, dusty galaxies from 0 < z < 5.3. Our sample comprises 29 high-redshift submillimetre galaxies (SMGs) from the literature and 843 dusty galaxies at z < 0.5 from the Herschel-Astrophysical TeraHertz Large Area S... | [
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... | 12.888306 | 7.49229 | 2014-03-01 | 59 | 2014MNRAS.441.1017R | [
"dust mass",
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"dust",
"lt",
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"low-redshift galaxies",
"SMGs",
"SMGs originates",
"z",
"their bursty star formation histories",
"molecular gas",
"CO",
"an average star formation rate",
"massi... | [
"dust",
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"galaxies: high-redshift",
"galaxies: ISM",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 7 | [
"10.1093/mnras/stu510",
"10.48550/arXiv.1403.2994"
] | [
"Rowlands, K.",
"Dunne, L.",
"Dye, S.",
"Aragón-Salamanca, A.",
"Maddox, S.",
"da Cunha, E.",
"Smith, D. J. B.",
"Bourne, N.",
"Eales, S.",
"Gomez, H. L.",
"Smail, I.",
"Alpaslan, M.",
"Clark, C. J. R.",
"Driver, S.",
"Ibar, E.",
"Ivison, R. J.",
"Robotham, A.",
"Smith, M. W. L.",
... | [
"School of Physics and Astronomy, The University of Nottingham, University Park Campus, Nottingham NG7 2RD, UK; (SUPA) School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK",
"Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchu... | [
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745597 | 1403.0958 | Broad absorption line variability in radio-loud quasars | We investigate C IV broad absorption line (BAL) variability within a sample of 46 radio-loud quasars (RLQs), selected from Sloan Digital Sky Survey (SDSS)/Faint Images of the Radio Sky at Twenty-Centimeters (FIRST) data to include both core-dominated (39) and lobe-dominated (7) objects. The sample consists primarily of... | [
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0... | 16.377176 | 7.236541 | 2014-03-01 | 23 | 2014MNRAS.440.2474W | [
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"RLQs",
"equivalent width measurements",
"equivalent widths",
"RQQs",
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... | [
"galaxies: active",
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] | 6 | [
"10.1093/mnras/stu402",
"10.48550/arXiv.1403.0958"
] | [
"Welling, C. A.",
"Miller, B. P.",
"Brandt, W. N.",
"Capellupo, D. M.",
"Gibson, R. R."
] | [
"Department of Physics and Astronomy, Dickinson College, Carlisle, PA 17013, USA",
"Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, USA; Department of Physics and Astronomy, Macalester College, 1600 Grand Ave, Saint Paul, MN 55105, USA",
"Department of Astronomy and Astr... | [
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12363341 | 1403.3056 | Stellar scattering and the formation of hot Jupiters in binary systems | Hot Jupiters (HJs) are usually defined as giant Jovian-size planets with orbital periods P<=10 days. Although they lie close to the star, several have finite eccentricities and significant misalignment angle with respect to the stellar equator, leading to ~20% of HJs in retrograde orbits. More than half, however, se... | [
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0.0... | 7.982541 | 14.255208 | 2014-03-01 | 7 | 2015IJAsB..14..313M | [
"hot planets",
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"giant Jovian-size planets",
"orbital characteristics",
"orbital periods",
"compact binary systems",
... | [
"planets",
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] | 3 | [
"10.1017/S147355041400007X",
"10.48550/arXiv.1403.3056"
] | [
"Martí, J. G.",
"Beaugé, C."
] | [
"Instituto de Astronomía Teórica y Experimental, Observatorio Astronómico, Universidad Nacional de Córdoba, Laprida 854, X5000BGR Córdoba, Argentina",
"Instituto de Astronomía Teórica y Experimental, Observatorio Astronómico, Universidad Nacional de Córdoba, Laprida 854, X5000BGR Córdoba, Argentina"
] | [
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746385 | 1403.1579 | Shocks in nova outflows - I. Thermal emission | Growing evidence for shocks in nova outflows includes (1) multiple velocity components in the optical spectra; (2) hard X-ray emission starting weeks to months after the outburst; (3) an early radio flare on time-scales of months, in excess of that predicted from the freely expanding photoionized gas; and, perhaps most... | [
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"radio emission",
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"shocks",
"rays",
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"times",
"multiple velocity components",
"the early radio maximum",
"the lat... | [
"radiation mechanisms: thermal",
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"Astrophysics - High Energy Astrophysical Phenomena",
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] | 15 | [
"10.1093/mnras/stu844",
"10.48550/arXiv.1403.1579"
] | [
"Metzger, Brian D.",
"Hascoët, Romain",
"Vurm, Indrek",
"Beloborodov, Andrei M.",
"Chomiuk, Laura",
"Sokoloski, J. L.",
"Nelson, Thomas"
] | [
"Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA",
"Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA",
"Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA; Tartu Observatory, Tõravere, Tartumaa EE-61602, Estonia",
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527066 | 1403.6673 | Further considerations on layer-oriented adaptive optics for solar telescopes | The future generation of telescopes will be equipped with multi-conjugate adaptive optics (MCAO) systems in order to obtain high angular resolution over large fields of view. MCAO comes in two flavors: star- and layer-oriented. Existing solar MCAO systems rely exclusively on the star-oriented approach. Earlier we have ... | [
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0.02... | 14.221319 | 10.503874 | 2014-03-01 | 0 | 2014arXiv1403.6673K | [
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"the Shack-Hartmann sub-aperture images",
"MCAO",
"a layer-oriented s... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 8 | [
"10.48550/arXiv.1403.6673"
] | [
"Kellerer, Aglae"
] | [
"-"
] | null | [
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] |
483228 | 1403.1115 | Spatial and Kinematic Distributions of Transition Populations in Intermediate Redshift Galaxy Clusters | We analyze the spatial and velocity distributions of confirmed members in five massive clusters of galaxies at intermediate redshift (0.5 < z < 0.9) to investigate the physical processes driving galaxy evolution. Based on spectral classifications derived from broad- and narrow-band photometry, we define four dist... | [
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0.010... | 12.344986 | 5.951982 | 2014-03-01 | 16 | 2014ApJ...786...30C | [
"GV galaxies",
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"galaxy-galaxy interactions",
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"star formation",
"RS) galaxies",
"the RS galaxies",
"four distinct galaxy populations",
"eac... | [
"galaxies: distances and redshifts",
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] | 2 | [
"10.1088/0004-637X/786/1/30",
"10.48550/arXiv.1403.1115"
] | [
"Crawford, Steven M.",
"Wirth, Gregory D.",
"Bershady, Matthew A."
] | [
"SAAO, P.O. Box 9, Observatory 7935, Cape Town, South Africa",
"W. M. Keck Observatory, 65-1120 Mamalahoa Highway, Kamuela, HI 96743, USA",
"Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706, USA"
] | [
"2014arXiv1412.4739R",
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788323 | 1403.0325 | Exploring the intergalactic magnetic field by means of Faraday tomography | Unveiling the intergalactic magnetic field (IGMF) in filaments of galaxies is a very important and challenging subject in modern astronomy. In order to probe the IGMF from rotation measures (RMs) of extragalactic radio sources, we need to separate RMs due to other origins such as the source, intervening galaxies, and o... | [
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... | 14.910365 | 4.390663 | 2014-03-01 | 34 | 2014PASJ...66...65A | [
"extragalactic radio sources",
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"m",
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"(Faraday RM synt... | [
"large-scale structure of universe",
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] | 4 | [
"10.1093/pasj/psu033",
"10.48550/arXiv.1403.0325"
] | [
"Akahori, Takuya",
"Kumazaki, Kohei",
"Takahashi, Keitaro",
"Ryu, Dongsu"
] | [
"Sydney Institute for Astronomy, School of Physics, The University of Sydney, NSW 2006, Australia",
"University of Nagoya, Furo-cho, Chikusa-ku, Nagoya 464-8601",
"University of Kumamoto, 2-39-1, Kurokami, Kumamoto 860-8555",
"Department of Physics, UNIST, Ulsan 689-798, Republic of Korea"
] | [
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438252 | 1403.2927 | The extended ROSAT-ESO Flux Limited X-ray Galaxy Cluster Survey (REFLEX II). IV. X-ray luminosity function and first constraints on cosmological parameters | The X-ray luminosity function that is closely related to the cluster mass function is an important statistic of the census of galaxy clusters in our Universe. It is also an important means to probe the cosmological model of our Universe. Based on our recently completed REFLEX II cluster sample comprising 910 galaxy clu... | [
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0.00806... | 13.002692 | 4.841347 | 2014-03-01 | 87 | 2014A&A...570A..31B | [
"several cosmological X-ray cluster surveys",
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"cosmological probes",
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"galaxies: clusters: general",
"cosmological parameters",
"X-rays: galaxies: clusters",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 4 | [
"10.1051/0004-6361/201323155",
"10.48550/arXiv.1403.2927"
] | [
"Böhringer, Hans",
"Chon, Gayoung",
"Collins, Chris A."
] | [
"Max-Planck-Institut für extraterrestrische Physik, 85748, Garching, Germany",
"Max-Planck-Institut für extraterrestrische Physik, 85748, Garching, Germany",
"Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool, L3 5RF, UK"
] | [
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719399 | 1403.5670 | Neutron reactions in astrophysics | The quest for the origin of matter in the Universe had been the subject of philosophical and theological debates over the history of mankind, but quantitative answers could be found only by the scientific achievements of the last century. A first important step on this way was the development of spectral analysis by Ki... | [
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... | 3.854458 | 2.483223 | 2014-03-01 | 97 | 2014JPhG...41e3101R | [
"nuclear physics",
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... | [
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Nuclear Experiment"
] | 22 | [
"10.1088/0954-3899/41/5/053101",
"10.48550/arXiv.1403.5670"
] | [
"Reifarth, R.",
"Lederer, C.",
"Käppeler, F."
] | [
"Goethe University Frankfurt, Frankfurt, Germany",
"Goethe University Frankfurt, Frankfurt, Germany",
"Karlsruhe Institute of Technology, Karlsruhe, Germany"
] | [
"2014PhRvC..90f5801M",
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746075 | 1403.2266 | High spatial resolution of the mid-infrared emission of the Compton-thick type 2 Seyfert galaxy, Markarian 3 | The mid-infrared (MIR) spectra observed with Gemini/Michelle have been used to study the nuclear region of the Compton-thick type 2 Seyfert galaxy, Markarian 3 (Mrk 3), at a spatial resolution of ∼200 pc. No polycyclic aromatic hydrocarbon emission bands were detected in the N-band spectrum of Mrk 3. However, intense [... | [
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... | 15.129188 | 8.145158 | 2014-03-01 | 10 | 2014MNRAS.441..630S | [
"Mrk",
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"MIR emission",
"Compton",
"pc",
"a theoretical torus spectral energy distribution",
"The torus model geometry",
"a silicate absorpti... | [
"techniques: spectroscopic",
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"galaxies: individual: Markarian 3",
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"Astrophysics - Galaxy Astrophysics"
] | 5 | [
"10.1093/mnras/stu468",
"10.48550/arXiv.1403.2266"
] | [
"Sales, Dinalva A.",
"Ruschel-Dutra, D.",
"Pastoriza, M. G.",
"Riffel, R.",
"Winge, Cláudia"
] | [
"Department of Physics, Rochester Institute of Technology, 84 Lomb Memorial Drive, Rochester, NY 14623, USA; Departamento de Astronomia, Universidade Federal do Rio Grande do Sul. 9500 Bento Gonçalves, Porto Alegre, 91501-970, Brazil",
"Departamento de Astronomia, Universidade Federal do Rio Grande do Sul. 9500 B... | [
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746284 | 1403.7396 | On radial anisotropy limits in stellar systems | Following earlier authors we re-examine the upper limits on the radial velocity anisotropy of general stellar systems; these constraints coming generically from phase-space density positivity, stability, and separability. Galaxy models almost always satisfy an inequality β < γ/2, i.e. the radial anisotropy is locall... | [
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0.0018... | 10.079713 | 5.614827 | 2014-03-01 | 1 | 2014MNRAS.442.3533B | [
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"methods: analytical",
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] | 2 | [
"10.1093/mnras/stu1059",
"10.48550/arXiv.1403.7396"
] | [
"Barber, Jeremy A.",
"Zhao, Hongsheng"
] | [
"Scottish Universities Physics Alliance, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK",
"Scottish Universities Physics Alliance, University of St Andrews, North Haugh, St Andrews, Fife KY16 9SS, UK"
] | [
"2023MNRAS.525.1795B"
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482911 | 1403.0055 | A Physical Model for the Evolving Ultraviolet Luminosity Function of High Redshift Galaxies and their Contribution to the Cosmic Reionization | We present a physical model for the evolution of the ultraviolet (UV) luminosity function of high-redshift galaxies, taking into account in a self-consistent way their chemical evolution and the associated evolution of dust extinction. Dust extinction is found to increase fast with halo mass. A strong correlation betwe... | [
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-0.01... | 12.951814 | 6.415932 | 2014-03-01 | 59 | 2014ApJ...785...65C | [
"z ~=",
"high z",
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"Lyman break galaxies",
"lower gas column densities",
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"halo mass",
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"Galaxies",
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... | [
"early universe",
"galaxies: evolution",
"galaxies: formation",
"galaxies: high-redshift",
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"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 8 | [
"10.1088/0004-637X/785/1/65",
"10.48550/arXiv.1403.0055"
] | [
"Cai, Zhen-Yi",
"Lapi, Andrea",
"Bressan, Alessandro",
"De Zotti, Gianfranco",
"Negrello, Mattia",
"Danese, Luigi"
] | [
"Astrophysics Sector, SISSA, Via Bonomea 265, I-34136 Trieste, Italy; Department of Astronomy and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen 361005, China;",
"Astrophysics Sector, SISSA, Via Bonomea 265, I-34136 Trieste, Italy; Dipartimento di Fisica, Università \"Tor Vergata,\" ... | [
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524676 | 1403.2044 | What could the value of the cosmological constant tell us about the future variation of the fine structure constant? | Motivated by reported claims of the measurements of a variation of the fine structure constant $\alpha$ we consider a theory where the electric charge, and consequently $\alpha$, is not a constant but depends on the Ricci scalar $R$. %We then show how this can be considered a particular case of the Bekenstein theory in... | [
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... | 9.271437 | 0.31201 | 2014-03-01 | 0 | 2014arXiv1403.2044E | [
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"the present value",
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"the cosmological constant",
"how future m... | [
"Astrophysics - Cosmology and Extragalactic Astrophysics"
] | 4 | [
"10.48550/arXiv.1403.2044"
] | [
"Enea Romano, Antonio"
] | [
"-"
] | null | [
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] |
482564 | 1403.0870 | Plasma Physical Parameters along Coronal-mass-ejection-driven Shocks. I. Ultraviolet and White-light Observations | In this work, UV and white-light (WL) coronagraphic data are combined to derive the full set of plasma physical parameters along the front of a shock driven by a coronal mass ejection. Pre-shock plasma density, shock compression ratio, speed, and inclination angle are estimated from WL data, while pre-shock plasma temp... | [
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-... | 13.286771 | 15.939953 | 2014-03-01 | 33 | 2014ApJ...784..102B | [
"shock plasma temperature",
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"plasma compression",
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"where derived post-shock plasma parameters",
"W... | [
"line: profiles",
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] | 7 | [
"10.1088/0004-637X/784/2/102",
"10.48550/arXiv.1403.0870"
] | [
"Bemporad, A.",
"Susino, R.",
"Lapenta, G."
] | [
"Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese, Torino, Italy",
"Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese, Torino, Italy",
"Center for Plasma Astrophys... | [
"2014ApJ...790...25S",
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12733 | 1403.2758 | The Local Environment of Ultraluminous X-Ray Sources Viewed by XMM-Newton's Optical Monitor | We have used XMM-Newton's Optical Monitor (OM) images to study the local environment of a sample of 27 ultraluminous X-ray sources (ULXs) in nearby galaxies. UVW1 fluxes were extracted from 100 pc regions centered on the ULX positions. We find that at least 4 ULXs (out of 10 published) have spectral types that are cons... | [
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-0... | 6.742752 | 7.085268 | 2014-03-01 | 14 | 2013ApJ...776..100B | [
"young stars",
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"young OB associations",
"young dense superclusters",
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"ULXs",
"previous literature values",
"recent star formation",
"nearby galaxies",
"clusters",
"Myr",
"SFRs",
"27 ultraluminous X-ray sources"... | [
"accretion",
"accretion disks",
"galaxies: star clusters: general",
"ultraviolet: stars",
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"Astrophysics - High Energy Astrophysical Phenomena"
] | 6 | [
"10.1088/0004-637X/776/2/100",
"10.48550/arXiv.1403.2758"
] | [
"Berghea, C. T.",
"Dudik, R. P.",
"Tincher, J.",
"Winter, L. M."
] | [
"United States Naval Observatory, Washington, DC 20392, USA",
"United States Naval Observatory, Washington, DC 20392, USA",
"St. John's College, Annapolis, MD 21401, USA",
"Atmospheric and Environmental Research, Lexington, MA 02421, USA"
] | [
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"2018MNRAS.479.3526G",
"2019ApJ...881...38E",
"2019IAUS..346..... | [
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483454 | 1403.6721 | Convective Overstability in Radially Stratified Accretion Disks under Thermal Relaxation | This paper expands the stability criterion for radially stratified, vertically unstratified accretion disks incorporating thermal relaxation. We find a linear amplification of epicyclic oscillations in these disks that depends on the effective cooling time, i.e., an overstability. The growth rates of the overstability ... | [
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0.0... | 10.584226 | 13.705351 | 2014-03-01 | 125 | 2014ApJ...788...21K | [
"thermal relaxation times",
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"amplifying vortices",
"the effective cooling time",
"vortex formation",
"t... | [
"accretion",
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"hydrodynamics",
"instabilities",
"methods: analytical",
"methods: numerical",
"planets and satellites: formation",
"turbulence",
"Astrophysics - Solar and Stellar Astrophysics"
] | 14 | [
"10.1088/0004-637X/788/1/21",
"10.48550/arXiv.1403.6721"
] | [
"Klahr, Hubert",
"Hubbard, Alexander"
] | [
"Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany",
"Department of Astrophysics, American Museum of Natural History, New York, NY 10024-5192, USA"
] | [
"2014A&A...572A..77S",
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12363349 | 1403.4809 | The Mt John University Observatory search for Earth-mass planets in the habitable zone of α Centauri | AbstractThe 'holy grail' in planet hunting is the detection of an Earth-analogue: a planet with similar mass as the Earth and an orbit inside the habitable zone. If we can find such an Earth-analogue around one of the stars in the immediate solar neighbourhood, we could potentially even study it in such great detail to... | [
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678337 | 1403.1271 | SCoPE: an efficient method of Cosmological Parameter Estimation | Markov Chain Monte Carlo (MCMC) sampler is widely used for cosmological parameter estimation from CMB and other data. However, due to the intrinsic serial nature of the MCMC sampler, convergence is often very slow. Here we present a fast and independently written Monte Carlo method for cosmological parameter estimation... | [
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872279 | 1403.6667 | A cryogenic infrared calibration target | A compact cryogenic calibration target is presented that has a peak diffuse reflectance, R ⩽ 0.003, from 800 to 4800 cm<SUP>-1</SUP> (12 - 2 μm). Upon expanding the spectral range under consideration to 400-10 000 cm<SUP>-1</SUP> (25 - 1 μm) the observed performance gracefully degrades to R ⩽ 0.02 at the band edges. In... | [
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745876 | 1403.4986 | Measuring gravitational lens time delays using low-resolution radio monitoring observations | Obtaining lensing time-delay measurements requires long-term monitoring campaigns with a high enough resolution (<1 arcsec) to separate the multiple images. In the radio, a limited number of high-resolution interferometer arrays make these observations difficult to schedule. To overcome this problem, we propose a te... | [
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437652 | 1403.5272 | Grain opacity and the bulk composition of extrasolar planets. I. Results from scaling the ISM opacity | Context. The opacity due to grains in the envelope of a protoplanet κ<SUB>gr</SUB> regulates the accretion rate of gas during formation, meaning that the final bulk composition of planets with a primordial H/He envelope is a function of that opacity. Observationally, for extrasolar planets with known mass and radius it... | [
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437326 | 1403.0727 | Deep R-band counts of z ≈ 3 Lyman-break galaxy candidates with the LBT | <BR /> Aims: We present a deep multiwavelength imaging survey (UGR) in 3 different fields, Q0933, Q1623, and COSMOS, for a total area of ~1500 arcmin<SUP>2</SUP>. The data were obtained with the Large Binocular Camera on the Large Binocular Telescope. <BR /> Methods: To select our Lyman-break galaxy (LBG) candidates, w... | [
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573619 | 1403.5334 | A search for new variable stars using digitized Moscow collection plates | By digitizing astronomical photographic plates one may extract full information stored on them, something that could not be practically achieved with classical analogue methods. We are developing algorithms for variable objects search using digitized photographic images and apply them to 30cm (10x10 deg. field of view)... | [
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"Lebedev, A.",
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100208 | 1403.2208 | Effects of the angular momentum of accreting matter on the flow structure in the subsonic settling and Bondi-Hoyle accretion regimes | Previously unexplored accretion regimes associated with the rotation of accreting matter, namely the perturbations of a quasi-spherical subsonic settling flow and Bondi-Hoyle accretion in the presence of axial rotation, are considered within the framework of ideal hydrodynamics. For subsonic settling accretion, the per... | [
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"10.1134/S1063773713120013",
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"Arzamasskiy, L.",
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"Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia; Moscow Institute of Physics and Technology, Dolgoprudnyi, Moscow oblast, Russia",
"Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia; Moscow Institute of Physics and Technology, Dolgoprudnyi, Moscow oblast, Russia"
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484296 | 1403.2722 | NuSTAR Observations of the Bullet Cluster: Constraints on Inverse Compton Emission | The search for diffuse non-thermal inverse Compton (IC) emission from galaxy clusters at hard X-ray energies has been undertaken with many instruments, with most detections being either of low significance or controversial. Because all prior telescopes sensitive at E > 10 keV do not focus light and have degree-scale... | [
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483043 | 1403.4935 | Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lyα Emitters in COSMOS and GOODS-N | We use broadband photometry extending from the rest-frame UV to the near-IR to fit the individual spectral energy distributions of 63 bright (L(Lyα) > 10<SUP>43</SUP> erg s<SUP>-1</SUP>) Lyα emitting galaxies (LAEs) in the redshift range 1.9 < z < 3.6. We find that these LAEs are quite heterogeneous, with stel... | [
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"10.1088/0004-637X/786/1/59",
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"Hagen, Alex",
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"Song, Mimi",
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"Fox, Derek B.",
"Gebhardt, Henry",
"Malz, A. I.",
"Schneider, Donald ... | [
"Department of Astronomy & Astrophysics, The Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA; Also at Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA.;",
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526114 | 1403.4797 | The influence of mass-transfer variability on the growth of white dwarfs, and the implications for supernova type Ia rates | White dwarfs (WDs) can increase their mass by accretion from companion stars, provided the mass-accretion rate is high enough to avoid nova eruptions. The accretion regimes that allow growth of the WDs are usually calculated assuming constant mass-transfer rates. However, it is possible that these systems are influence... | [
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"10.48550/arXiv.1403.4797"
] | [
"Toonen, Silvia",
"Voss, Rasmus",
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482863 | 1403.1667 | The Rest-frame Submillimeter Spectrum of High-redshift, Dusty, Star-forming Galaxies | We present the average rest-frame spectrum of high-redshift dusty, star-forming galaxies from 250 to 770 GHz. This spectrum was constructed by stacking Atacama Large Millimeter/submillimeter Array (ALMA) 3 mm spectra of 22 such sources discovered by the South Pole Telescope and spanning z = 2.0-5.7. In addition to mult... | [
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] | 9 | [
"10.1088/0004-637X/785/2/149",
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"Spilker, J. S.",
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"Chapman, S. C.",
"Crawford, T. M.",
"de Breuck, C.",
"Fassnacht, C. D.",
"Gonzalez, A. H.",
"Greve, T. R.",... | [
"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA",
"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA",
"University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA",
"European Southern Observatory, Alonso d... | [
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12363173 | 1403.4873 | Ejecta transfer in the Pluto system | The small satellites of the Pluto system (Styx, Nix, Kerberos, and Hydra) have very low surface escape velocities, and impacts should therefore eject a large amount of material from their surfaces. We show that most of this material then escapes from the Pluto system, though a significant fraction collects on the surfa... | [
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"Porter, Simon B.",
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678085 | 1403.4222 | General parity-odd CMB bispectrum estimation | We develop a methodology for estimating parity-odd bispectra in the cosmic microwave background (CMB). This is achieved through the extension of the original separable modal methodology to parity-odd bispectrum domains (l<SUB>1</SUB>+l<SUB>2</SUB>+l<SUB>3</SUB> = odd). Through numerical tests of the parity-odd modal de... | [
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0.01840... | 12.570984 | 0.801893 | 2014-03-01 | 27 | 2014JCAP...05..008S | [
"parity-odd bispectrum domains",
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... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"General Relativity and Quantum Cosmology",
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] | 8 | [
"10.1088/1475-7516/2014/05/008",
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] | [
"Shiraishi, Maresuke",
"Liguori, Michele",
"Fergusson, James R."
] | [
"Dipartimento di Fisica e Astronomia ``G. Galilei'', Università degli Studi di Padova, via Marzolo 8, I-35131, Padova, Italy; INFN, Sezione di Padova, via Marzolo 8, I-35131, Padova, Italy;",
"Dipartimento di Fisica e Astronomia ``G. Galilei'', Università degli Studi di Padova, via Marzolo 8, I-35131, Padova, Ita... | [
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813221 | 1403.3402 | Cosmology with galaxy clusters: Systematic effects in the halo mass function | We investigate potential systematic effects in constraining the amplitude of primordial fluctuations σ<SUB>8</SUB> arising from the choice of halo mass function in the likelihood analysis of current and upcoming galaxy cluster surveys. We study the widely used N-body simulation fit of Tinker et al. (T08) and, as an alt... | [
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"survey selection threshold",
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] | 6 | [
"10.1103/PhysRevD.90.023520",
"10.48550/arXiv.1403.3402"
] | [
"Paranjape, Aseem"
] | [
"Institute for Astronomy, Department of Physics, ETH Zürich, Wolfgang-Pauli-Strasse 27, CH 8093 Zürich, Switzerland"
] | [
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525678 | 1403.3919 | Hint of relic gravitational waves in the Planck and WMAP data | Relic gravitational waves (RGWs) leave well-understood imprints on the anisotropies in the temperature and polarization of cosmic microwave background (CMB) radiation. In the TT and TE information channels, which have been well observed by WMAP and Planck missions, RGWs compete with density perturbations mainly at low ... | [
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0.... | 11.845944 | -0.138481 | 2014-03-01 | 15 | 2014arXiv1403.3919Z | [
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"TE",
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"Astrophysics - Cosmology and Extragalactic Astrophysics",
"General Relativity and Quantum Cosmology",
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] | 3 | [
"10.48550/arXiv.1403.3919"
] | [
"Zhao, Wen",
"Cheng, Cheng",
"Huang, Qing-Guo"
] | [
"-",
"-",
"-"
] | [
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715536 | 1403.7221 | DIRAC framework evaluation for the Fermi-LAT and CTA experiments | DIRAC (Distributed Infrastructure with Remote Agent Control) is a general framework for the management of tasks over distributed heterogeneous computing environments. It has been originally developed to support the production activities of the LHCb (Large Hadron Collider Beauty) experiment and today is extensively used... | [
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... | 7.570367 | 0.836506 | 2014-03-01 | 2 | 2014JPhCS.513c2003A | [
"DIRAC",
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"... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 6 | [
"10.1088/1742-6596/513/3/032003",
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"Arrabito, L.",
"Cohen-Tanugi, J.",
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"Longo, F.",
"Kuss, M.",
"Piron, F.",
"Renaud, M.",
"Rolland, V.",
"Sapunov, M.",
"Tsaregorodtsev, A.",
"Zimmer, S."
] | [
"Laboratoire Univers et Particules, Université de Montpellier II Place Eugène Bataillon – CC 72, CNRS/IN2P3, F-34095 Montpellier, France",
"Laboratoire Univers et Particules, Université de Montpellier II Place Eugène Bataillon – CC 72, CNRS/IN2P3, F-34095 Montpellier, France",
"University of Barcelona, Diagonal... | [
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] |
482992 | 1403.5154 | Discriminating the Progenitor Type of Supernova Remnants with Iron K-shell Emission | Supernova remnants (SNRs) retain crucial information about both their parent explosion and circumstellar material left behind by their progenitor. However, the complexity of the interaction between supernova ejecta and ambient medium often blurs this information, and it is not uncommon for the basic progenitor type (Ia... | [
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] | 26 | [
"10.1088/2041-8205/785/2/L27",
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] | [
"Yamaguchi, Hiroya",
"Badenes, Carles",
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"Nakano, Toshio",
"Castro, Daniel",
"Enoto, Teruaki",
"Hiraga, Junko S.",
"Hughes, John P.",
"Maeda, Yoshitomo",
"Nobukawa, Masayoshi",
"Safi-Harb, Samar",
"Slane, Patrick O.",
"Smith, Randall K.",
"Uchida, Hiroyuki"
] | [
"NASA Goddard Space Flight Center, Code 662, Greenbelt, MD 20771, USA; Department of Astronomy, University of Maryland, College Park, MD 20742, USA; Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA;",
"Department of Physics and Astronomy and Pittsburgh Particle Physics, Astr... | [
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12363886 | 1403.0771 | Wormhole geometries supported by quark matter at ultra-high densities | A fundamental ingredient in wormhole physics is the presence of exotic matter, which involves the violation of the null energy condition (NEC). In this context, we investigate the possibility that wormholes could be supported by quark matter at extreme densities. Theoretical and experimental investigations of the struc... | [
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... | 4.844477 | 1.800907 | 2014-03-01 | 9 | 2015IJMPD..2450006H | [
"quark matter",
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"the color superconducting quark phases",
"that strange quark matter",
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"... | [
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"Quark-gluon plasma",
"General Relativity and Quantum Cosmology",
"Astrophysics - High Energy Astrophysical Phenomena",
"High Energy Physics - Theory"
] | 8 | [
"10.1142/S0218271815500066",
"10.48550/arXiv.1403.0771"
] | [
"Harko, Tiberiu",
"Lobo, Francisco S. N.",
"Mak, M. K."
] | [
"Department of Mathematics, University College London, Gower Street, London WC1E 6BT, UK",
"Centro de Astronomia e Astrofísica da Universidade de Lisboa, Campo Grande, Edificío C8, 1749-016 Lisboa, Portugal",
"Department of Computing and Information Management, Hong Kong Institute of Vocational Education, Chai ... | [
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746049 | 1403.6294 | On the origin of bursts in blue compact dwarf galaxies: clues from kinematics and stellar populations | Blue compact dwarf galaxies (BCDs) form stars at, for their sizes, extraordinarily high rates. In this paper, we study what triggers this starburst and what is the fate of the galaxy once its gas fuel is exhausted. We select four BCDs with smooth outer regions, indicating them as possible progenitors of dwarf elliptica... | [
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... | 11.485732 | 7.785458 | 2014-03-01 | 22 | 2014MNRAS.441..452K | [
"dwarf elliptical galaxies",
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"the star formation regions",
"possible progenitors",
"smooth outer regions",
"the same galaxy",
"the star formation",
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"galaxies: dwarf",
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"galaxies: kinematics and dynamics",
"galaxies: star formation",
"galaxies: stellar content",
"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.1093/mnras/stu556",
"10.48550/arXiv.1403.6294"
] | [
"Koleva, M.",
"De Rijcke, S.",
"Zeilinger, W. W.",
"Verbeke, R.",
"Schroyen, J.",
"Vermeylen, L."
] | [
"Sterrenkundig Observatorium, Ghent University, Krijgslaan 281, S9, B-9000 Ghent, Belgium",
"Sterrenkundig Observatorium, Ghent University, Krijgslaan 281, S9, B-9000 Ghent, Belgium",
"Institut für Astrophysik, Universit'ät Wien Türkenschanzstrasse 17, A-1180 Wien, Austria",
"Sterrenkundig Observatorium, Ghen... | [
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483810 | 1403.3825 | Spectral Softening in the X-Ray Afterglow of GRB 130925A as Predicted by the Dust Scattering Model | Gamma-ray bursts (GRBs) usually occur in a dense star-forming region with a massive circumburst medium. The small-angle scattering of intense prompt X-ray emission off the surrounding dust grains will have observable consequences and sometimes can dominate the X-ray afterglow. In most of the previous studies, only the ... | [
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0.0... | 16.517103 | 0.807294 | 2014-03-01 | 11 | 2014ApJ...789...74Z | [
"intense prompt X-ray emission",
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"the scattered X-ray emission",
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"detailed observational data",
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"the X-ray afterglow",
"grains",
"130925A.",
"AD",
"a significant spectral softening",
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"dust",
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] | 11 | [
"10.1088/0004-637X/789/1/74",
"10.48550/arXiv.1403.3825"
] | [
"Zhao, Yi-Nan",
"Shao, Lang"
] | [
"Department of Space Science and Astronomy, Hebei Normal University, Shijiazhuang 050024, China",
"Department of Space Science and Astronomy, Hebei Normal University, Shijiazhuang 050024, China; Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 21... | [
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"2023A&A...675A..44Q",
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