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12410058 | 1607.02577 | Extensive photometry of the intermediate polar MU Cam: detection of a spin period change | Intermediate polars with known rates of spin period changes are not numerous because such tasks require measurements performed for a long time. To measure a spin period change, MU Cam is a good candidate because it has a spin oscillation with a large amplitude enabling measurements with high precision. Fortunately, in ... | [
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] | 3 | [
"10.1007/s10509-016-2859-0",
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] | [
"Kozhevnikov, V. P."
] | [
"Astronomical Observatory, Ural Federal University, Ekaterinburg, Russia"
] | [
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12593907 | 1607.01024 | Linear and non-linear bias: predictions versus measurements | We study the linear and non-linear bias parameters which determine the mapping between the distributions of galaxies and the full matter density fields, comparing different measurements and predictions. Associating galaxies with dark matter haloes in the Marenostrum Institut de Ciències de l'Espai (MICE) Grand Challeng... | [
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] | 6 | [
"10.1093/mnras/stw2876",
"10.48550/arXiv.1607.01024"
] | [
"Hoffmann, K.",
"Bel, J.",
"Gaztañaga, E."
] | [
"Institut de Ciències de l'Espai (ICE, IEEC/CSIC), E-08193 Bellaterra (Barcelona), Spain; Department of Physics, Center for Astrophysics, Tsinghua University, Beijing 100084, China",
"Aix Marseille Univ, Univ Toulon, CNRS, CPT, F-13388 Marseille, France",
"Institut de Ciències de l'Espai (ICE, IEEC/CSIC), E-081... | [
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5490440 | 1607.01738 | Measuring Collisionless Damping in Heliospheric Plasmas using Field-Particle Correlations | An innovative field-particle correlation technique is proposed that uses single-point measurements of the electromagnetic fields and particle velocity distribution functions to investigate the net transfer of energy from fields to particles associated with the collisionless damping of turbulent fluctuations in weakly c... | [
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-0... | 12.588896 | 14.420337 | 2016-07-01 | 66 | 2016ApJ...826L..30K | [
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"velocity space",
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] | 5 | [
"10.3847/2041-8205/826/2/L30",
"10.48550/arXiv.1607.01738"
] | [
"Klein, K. G.",
"Howes, G. G."
] | [
"Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI 48109, USA ; Space Science Center, University of New Hampshire, Durham, NH 03824, USA",
"Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA"
] | [
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3349576 | 1607.04601 | The many faces of LINER-like galaxies: a WISE view | We use the Sloan Digital Sky Survey (SDSS) and Wide-field Sky Survey Explorer surveys to investigate the real nature of galaxies defined as low-ionization nuclear emission-line regions (LINERs) in the BPT diagram. After establishing a mid-infrared colour W2-W3 = 2.5 as the optimal separator between galaxies with and wi... | [
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"galaxies: active",
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] | 9 | [
"10.1093/mnras/stw1742",
"10.48550/arXiv.1607.04601"
] | [
"Herpich, F.",
"Mateus, A.",
"Stasińska, G.",
"Cid Fernandes, R.",
"Vale Asari, N."
] | [
"Departamento de Física-CFM, Universidade Federal de Santa Catarina, C.P. 476, 88040-900 Florianópolis, SC, Brazil",
"Departamento de Física-CFM, Universidade Federal de Santa Catarina, C.P. 476, 88040-900 Florianópolis, SC, Brazil",
"LUTH, Observatoire de Paris, PSL, CNRS, UMPC, Univ Paris Diderot, 5 place Jul... | [
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12472933 | 1607.08872 | Propagation of ultrahigh energy cosmic rays in extragalactic magnetic fields: a view from cosmological simulations | We use the CRPROPA code to simulate the propagation of ultrahigh energy cosmic rays (with energy ≥10<SUP>18</SUP>eV and pure proton composition) through extragalactic magnetic fields that have been simulated with the cosmological ENZO code. We test both primordial and astrophysical magnetogenesis scenarios in order to ... | [
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... | 5.922693 | 0.592584 | 2016-07-01 | 41 | 2016MNRAS.462.3660H | [
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] | 2 | [
"10.1093/mnras/stw1903",
"10.48550/arXiv.1607.08872"
] | [
"Hackstein, S.",
"Vazza, F.",
"Brüggen, M.",
"Sigl, G.",
"Dundovic, A."
] | [
"Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany",
"Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany",
"Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany",
"II. Institut für Theoretische Physik, Universität Hamburg, Luruper Chausee 149, D-22761 Hamburg, Germa... | [
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12408813 | 1607.01953 | Long-lived Spiral Structure for Galaxies with Intermediate-size Bulges | Spiral structure in disk galaxies is modeled with nine collisionless N-body simulations including live disks, halos, and bulges with a range of masses. Two of these simulations make long-lasting and strong two-arm spiral wave modes that last for ∼5 Gyr with constant pattern speed. These two had a light stellar disk and... | [
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-0... | 10.23533 | 6.979313 | 2016-07-01 | 23 | 2016ApJ...826L..21S | [
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"galaxies: bulges",
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] | 9 | [
"10.3847/2041-8205/826/2/L21",
"10.48550/arXiv.1607.01953"
] | [
"Saha, Kanak",
"Elmegreen, Bruce"
] | [
"Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India",
"IBM Research Division, T. J. Watson Research Center, 1101 Kitchawan Road, Yorktown Heights, NY 10598, USA"
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12508115 | 1607.01448 | Nuclear neutrino energy spectra in high temperature astrophysical environments | Astrophysical environments that reach temperatures greater than ∼100 keV can have significant neutrino energy loss via both plasma processes and nuclear weak interactions. We find that nuclear processes likely produce the highest-energy neutrinos. The important weak nuclear interactions include both charged current cha... | [
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0.... | 4.127187 | 2.190231 | 2016-07-01 | 12 | 2016PhRvC..94e5808M | [
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] | 1 | [
"10.1103/PhysRevC.94.055808",
"10.48550/arXiv.1607.01448"
] | [
"Misch, G. Wendell",
"Fuller, George M."
] | [
"Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China and Collaborative Innovation Center of IFSA (CICIFSA), Shanghai Jiao Tong University, Shanghai 200240, China",
"Department of Physics, University of California, San Diego, La Jolla, California 92093, USA"
] | [
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12501152 | 1607.08043 | Light speed variation from gamma ray burst GRB 160509A | It is postulated in Einstein's relativity that the speed of light in vacuum is a constant for all observers. However, the effect of quantum gravity could bring an energy dependence of light speed. Even a tiny speed variation, when amplified by the cosmological distance, may be revealed by the observed time lags between... | [
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-... | 8.445044 | 0.512273 | 2016-07-01 | 66 | 2016PhLB..760..602X | [
"light speed",
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] | 8 | [
"10.1016/j.physletb.2016.07.044",
"10.48550/arXiv.1607.08043"
] | [
"Xu, Haowei",
"Ma, Bo-Qiang"
] | [
"School of Physics, State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China",
"School of Physics, State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China"
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12594662 | 1607.06097 | Detection of baryon acoustic oscillation features in the large-scale three-point correlation function of SDSS BOSS DR12 CMASS galaxies | We present the large-scale three-point correlation function (3PCF) of the Sloan Digital Sky Survey DR12 Constant stellar Mass (CMASS) sample of 777 202 Luminous Red Galaxies, the largest-ever sample used for a 3PCF or bispectrum measurement. We make the first high-significance (4.5σ) detection of baryon acoustic oscill... | [
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-0.03703787177801132... | 12.235075 | 2.483861 | 2016-07-01 | 118 | 2017MNRAS.469.1738S | [
"3PCF",
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"BAO",
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"baryon acoustic oscillations",
"DESI",
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"cosmology: observations",
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] | 7 | [
"10.1093/mnras/stx488",
"10.48550/arXiv.1607.06097"
] | [
"Slepian, Zachary",
"Eisenstein, Daniel J.",
"Brownstein, Joel R.",
"Chuang, Chia-Hsun",
"Gil-Marín, Héctor",
"Ho, Shirley",
"Kitaura, Francisco-Shu",
"Percival, Will J.",
"Ross, Ashley J.",
"Rossi, Graziano",
"Seo, Hee-Jong",
"Slosar, Anže",
"Vargas-Magaña, Mariana"
] | [
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA",
"Instituto de Física Teórica, (UAM/CSI... | [
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12593612 | 1607.08275 | MOCCA-SURVEY Database I: Is NGC 6535 a dark star cluster harbouring an IMBH? | We describe the dynamical evolution of a unique type of dark star cluster model in which the majority of the cluster mass at Hubble time is dominated by an intermediate-mass black hole (IMBH). We analysed results from about 2000 star cluster models (Survey Database I) simulated using the Monte Carlo code MOnte Carlo Cl... | [
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"10.1093/mnras/stw2573",
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"Askar, Abbas",
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"de Vita, Ruggero",
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"Kamann, Sebastian"
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"Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, PL-00-716 Warsaw, Poland",
"Max-Planck Institute for Astronomy, Koenigstuhl 17, D-69117 Heidelberg, Germany",
"School of Physics, University of Melbourne, VIC 3010, Australia",
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5060081 | 1607.07744 | The concerted impact of galaxies and QSOs on the ionization and thermal state of the intergalactic medium | We present a detailed analysis of the ionization and thermal structure of the intergalactic medium (IGM) around a high-redshift (z = 10) QSO, using a large suite of cosmological, multifrequency radiative transfer simulations, exploring the contribution from galaxies as well as the QSO, and the effect of X-rays and seco... | [
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] | 6 | [
"10.1093/mnras/stx603",
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] | [
"Kakiichi, Koki",
"Graziani, Luca",
"Ciardi, Benedetta",
"Meiksin, Avery",
"Compostella, Michele",
"Eide, Marius B.",
"Zaroubi, Saleem"
] | [
"Max Planck Institute for Astrophysics, Karl-Schwarzschild Straße 1, D-85741 Garching, Germany",
"Max Planck Institute for Astrophysics, Karl-Schwarzschild Straße 1, D-85741 Garching, Germany; INAF Osservatorio Astronomico di Roma, Via Frascati 33, I-00040 Monte Porzio Catone (RM), Italy",
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12409316 | 1607.07869 | On the Proper Use of the Reduced Speed of Light Approximation | I show that the reduced speed of light (RSL) approximation, when used properly (I.e., as originally designed—only for local sources but not for the cosmic background), remains a highly accurate numerical method for modeling cosmic reionization. Simulated ionization and star formation histories from the “Cosmic Reioniza... | [
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... | 13.513605 | 5.344818 | 2016-07-01 | 20 | 2016ApJ...833...66G | [
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] | 4 | [
"10.3847/1538-4357/833/1/66",
"10.48550/arXiv.1607.07869"
] | [
"Gnedin, Nickolay Y."
] | [
"Particle Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510, USA; Kavli Institute for Cosmological Physics, The University of Chicago, Chicago, IL 60637, USA; Department of Astronomy & Astrophysics, The University of Chicago, Chicago, IL 60637, USA"
] | [
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4756676 | 1607.02950 | Exploring high-z galaxies with the E-ELT | We present simulated observations of galaxies at z = 2 and z = 3 to probe the capabilities of next-generation telescopes (E-ELT and JWST) to measure the structural and photometrical properties of high-redshift galaxies. We carry out an extensive set of simulations of high-redshift galaxies adopting the specifications o... | [
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] | 4 | [
"10.1051/0004-6361/201628114",
"10.48550/arXiv.1607.02950"
] | [
"Gullieuszik, M.",
"Falomo, R.",
"Greggio, L.",
"Uslenghi, M.",
"Fantinel, D."
] | [
"INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122, Padova, Italy",
"INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122, Padova, Italy",
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12465105 | 1607.07058 | Hubble induced mass after inflation in spectator field models | Spectator field models such as the curvaton scenario and the modulated reheating are attractive scenarios for the generation of the cosmic curvature perturbation, as the constraints on inflation models are relaxed. In this paper, we discuss the effect of Hubble induced masses on the dynamics of spectator fields after i... | [
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0.0175... | 11.124683 | -0.947879 | 2016-07-01 | 9 | 2016JCAP...12..014F | [
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] | 8 | [
"10.1088/1475-7516/2016/12/014",
"10.48550/arXiv.1607.07058"
] | [
"Fujita, Tomohiro",
"Harigaya, Keisuke"
] | [
"Stanford Institute for Theoretical Physics and Department of Physics, Stanford University, Stanford, CA 94306, U.S.A.",
"Department of Physics, University of California, Berkeley, CA 94720, U.S.A. ; Theoretical Physics Group, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, U.S.A.;"
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4413907 | 1607.07328 | Decaying dark matter search with NuSTAR deep sky observations | We present the results of the search for decaying dark matter with particle mass in the 6-40 keV range with NuSTAR deep observations of COSMOS and ECDFS empty sky fields. We show that the main contribution to the decaying dark matter signal from the Milky Way galaxy comes through the aperture of the NuSTAR detector, ra... | [
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] | 7 | [
"10.1103/PhysRevD.94.123504",
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] | [
"Neronov, A.",
"Malyshev, D.",
"Eckert, D."
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"ISDC, Astronomy Department, University of Geneva, Ch. d'Ecogia 16, 1290 Version, Switzerland",
"Institut für Astronomie und Astrophysik Tübingen, Universität Tübingen, Sand 1, D-72076 Tübingen, Germany",
"ISDC, Astronomy Department, University of Geneva, Ch. d'Ecogia 16, 1290 Version, Switzerland"
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2524317 | 1607.02507 | How to quench a galaxy | We show how the interplay between active galactic nuclei (AGNs) and merger history determines whether a galaxy quenches star formation (SF) at high redshift. We first simulate, in a full cosmological context, a galaxy of total dynamical mass M<SUB>vir</SUB> = 10<SUP>12</SUP> M<SUB>⊙</SUB> at z = 2. Then we systematical... | [
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0.0247... | 12.173446 | 6.57976 | 2016-07-01 | 96 | 2017MNRAS.465..547P | [
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... | [
"galaxies: evolution",
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] | 15 | [
"10.1093/mnras/stw2627",
"10.48550/arXiv.1607.02507"
] | [
"Pontzen, Andrew",
"Tremmel, Michael",
"Roth, Nina",
"Peiris, Hiranya V.",
"Saintonge, Amélie",
"Volonteri, Marta",
"Quinn, Tom",
"Governato, Fabio"
] | [
"Department of Physics and Astronomy, University College London, London WC1E 6BT, UK",
"Astronomy Department, University of Washington, Seattle, WA 98195, USA",
"Department of Physics and Astronomy, University College London, London WC1E 6BT, UK",
"Department of Physics and Astronomy, University College Londo... | [
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12520421 | 1607.05111 | The Inclination of the Planetary System Relative to the Solar Equator May Be Explained by the Presence of Planet 9 | We evaluate the effects of a distant planet, commonly known as planet 9, on the dynamics of the giant planets of the solar system. We find that the dynamics of the giant planets can be decomposed into a classic Lagrange-Laplace dynamics relative to their own invariant plane and a slow precession of said plane relative ... | [
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-0.02... | 7.573224 | 16.086002 | 2016-07-01 | 46 | 2017AJ....153...27G | [
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] | 10 | [
"10.3847/1538-3881/153/1/27",
"10.48550/arXiv.1607.05111"
] | [
"Gomes, Rodney",
"Deienno, Rogerio",
"Morbidelli, Alessandro"
] | [
"Observatório Nacional Rua General José Cristino 77, CEP 20921-400, Rio de Janeiro, Brazil",
"Laboratoire Lagrange, UCA, OCA, CNRS, Nice, France ; Instituto Nacional de Pesquisas Espaciais, São José dos Campos, SP, Brazil",
"Laboratoire Lagrange, UMR7293, Université Côte dAzur, CNRS, Observatoire de la Côte dAz... | [
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2881450 | 1607.07863 | Constraining f (R ) gravity with Sunyaev-Zel'dovich clusters detected by the Planck satellite | Clusters of galaxies have the potential of providing powerful constraints on possible deviations from General Relativity. We use the catalog of Sunyaev-Zel'dovich (SZ) sources detected by Planck and consider a correction to the halo mass function for a f (R ) class of modified gravity models, which has been recently fo... | [
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0.0269... | 10.507249 | 1.532137 | 2016-07-01 | 25 | 2017PhRvD..95b3521P | [
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] | 2 | [
"10.1103/PhysRevD.95.023521",
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] | [
"Peirone, Simone",
"Raveri, Marco",
"Viel, Matteo",
"Borgani, Stefano",
"Ansoldi, Stefano"
] | [
"Astronomy Unit, Department of Physics, University of Trieste, Via Tiepolo 11, I-34131 Trieste, Italy",
"SISSA-International School for Advanced Studies, Via Bonomea 265, I-34136 Trieste, Italy; INFN, Sezione di Trieste, Via Valerio 2, I-34127 Trieste, Italy; INAF-Osservatorio Astronomico di Trieste, Via Gian Bat... | [
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1821058 | 1607.02394 | Constrained hyperbolic divergence cleaning in smoothed particle magnetohydrodynamics with variable cleaning speeds | We present an updated constrained hyperbolic/parabolic divergence cleaning algorithm for smoothed particle magnetohydrodynamics (SPMHD) that remains conservative with wave cleaning speeds which vary in space and time. This is accomplished by evolving the quantity ψ /c<SUB>h</SUB> instead of ψ. Doing so allows each part... | [
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... | 7 | [
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] | [
"Tricco, Terrence S.",
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] | [
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12406281 | 1607.00672 | New detections of embedded clusters in the Galactic halo | Context. Until recently it was thought that high Galactic latitude clouds were a non-star-forming ensemble. However, in a previous study we reported the discovery of two embedded clusters (ECs) far away from the Galactic plane (~ 5 kpc). In our recent star cluster catalogue we provided additional high and intermediate ... | [
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0.00... | 9.898826 | 9.028101 | 2016-07-01 | 18 | 2016A&A...593A..95C | [
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"10.1051/0004-6361/201628710",
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] | [
"Camargo, D.",
"Bica, E.",
"Bonatto, C."
] | [
"Universidade Federal do Rio Grande do Sul, Departamento de Astronomia, CP 15051, RS, 91501-970, Porto Alegre, Brazil",
"Universidade Federal do Rio Grande do Sul, Departamento de Astronomia, CP 15051, RS, 91501-970, Porto Alegre, Brazil",
"Universidade Federal do Rio Grande do Sul, Departamento de Astronomia, ... | [
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12594281 | 1607.04784 | Optical and ultraviolet spectroscopic analysis of SN 2011fe at late times | We present optical spectra of the nearby Type Ia supernova SN 2011fe at 100, 205, 311, 349 and 578 d post-maximum light, as well as an ultraviolet (UV) spectrum obtained with the Hubble Space Telescope at 360 d post-maximum light. We compare these observations with synthetic spectra produced with the radiative transfer... | [
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... | 2.927592 | 4.920237 | 2016-07-01 | 12 | 2017MNRAS.467.2392F | [
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"supernovae: general",
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"10.1093/mnras/stx241",
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"Friesen, Brian",
"Baron, E.",
"Parrent, Jerod T.",
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"Branch, David",
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"Hauschildt, Peter H.",
"Foley, Ryan J.",
"Wright, Darryl E.",
"Pan, Yen-Chen",
"Filippenko, Alexei V.",
"Clubb, Kelsey I.",
"Silverman, Jeffrey M.",
"Maeda, Keiichi",
"Shivvers, Isa... | [
"Homer L. Dodge Department of Physics, and Astronomy, 440 W. Brooks St., Rm 100, Norman, OK 73019, USA; NERSC, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 59R4010A, Berkeley, CA 94720",
"Homer L. Dodge Department of Physics, and Astronomy, 440 W. Brooks St., Rm 100, Norman, OK 73019, USA; Hamburge... | [
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12464577 | 1607.08755 | Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission | We perform a forecast analysis of the capability of the eLISA space-based interferometer to constrain models of early and interacting dark energy using gravitational wave standard sirens. We employ simulated catalogues of standard sirens given by merging massive black hole binaries visible by eLISA, with an electromagn... | [
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-0.... | 8.195706 | 1.967904 | 2016-07-01 | 76 | 2016JCAP...10..006C | [
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"10.1088/1475-7516/2016/10/006",
"10.48550/arXiv.1607.08755"
] | [
"Caprini, Chiara",
"Tamanini, Nicola"
] | [
"Institut de Physique Théorique, CEA-Saclay, CNRS UMR 3681, Université Paris-Saclay, Gif-sur-Yvette, F-91191 France",
"Institut de Physique Théorique, CEA-Saclay, CNRS UMR 3681, Université Paris-Saclay, Gif-sur-Yvette, F-91191 France"
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12473224 | 1607.01397 | White dwarf pollution by planets in stellar binaries | Approximately 0.2 ± 0.2 of white dwarfs (WDs) show signs of pollution by metals, which is likely due to the accretion of tidally disrupted planetary material. Models invoking planet-planet interactions after WD formation generally cannot explain pollution at cooling times of several Gyr. We consider a scenario in which... | [
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] | 9 | [
"10.1093/mnrasl/slw134",
"10.48550/arXiv.1607.01397"
] | [
"Hamers, Adrian S.",
"Portegies Zwart, Simon F."
] | [
"Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, The Netherlands",
"Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, The Netherlands"
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12406317 | 1607.08080 | Glimpses of stellar surfaces. II. Origins of the photometric modulations and timing variations of KOI-1452 | The deviations of the mid-transit times of an exoplanet from a linear ephemeris are usually the result of gravitational interactions with other bodies in the system. However, these types of transit timing variations (TTV) can also be introduced by the influences of star spots on the shape of the transit profile. Here w... | [
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-0... | 7.102705 | 13.951004 | 2016-07-01 | 2 | 2016A&A...594A..42I | [
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"Astrophysics - Earth and Planetary Astrophysics",
"Astrophysics - Solar and Stellar Astrophysics"
] | 2 | [
"10.1051/0004-6361/201628295",
"10.48550/arXiv.1607.08080"
] | [
"Ioannidis, P.",
"Schmitt, J. H. M. M."
] | [
"Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029, Hamburg, Germany",
"Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029, Hamburg, Germany"
] | [
"2019A&A...624A..15S",
"2021A&A...649A..17D"
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12408690 | 1607.08339 | Damping of the Milky Way Bar by Manifold-driven Spirals | We describe a new phenomenon of “bar damping” that may have played an important role in shaping the Milky Way bar and bulge as well as its spiral structure. We use a collisionless N-body simulation of a Milky Way-like galaxy initially composed of a dark matter halo and an exponential disk with a Toomre parameter slight... | [
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... | 10.183421 | 6.836032 | 2016-07-01 | 3 | 2016ApJ...830L..20L | [
"subsequent buckling episodes",
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"galaxies: clusters: general",
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] | 5 | [
"10.3847/2041-8205/830/1/L20",
"10.48550/arXiv.1607.08339"
] | [
"Łokas, Ewa L."
] | [
"Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00-716 Warsaw, Poland"
] | [
"2017ApJ...839...24K",
"2018A&A...615A..10M",
"2019MNRAS.484.1487E"
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2774813 | 1607.08613 | SDSS-IV MaNGA IFS Galaxy Survey—Survey Design, Execution, and Initial Data Quality | The MaNGA Survey (Mapping Nearby Galaxies at Apache Point Observatory) is one of three core programs in the Sloan Digital Sky Survey IV. It is obtaining integral field spectroscopy for 10,000 nearby galaxies at a spectral resolution of R ∼ 2000 from 3622 to 10354 Å. The design of the survey is driven by a set of scienc... | [
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... | 11.551139 | 6.744822 | 2016-07-01 | 304 | 2016AJ....152..197Y | [
"spatial resolution",
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"galaxies: evolution",
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] | 16 | [
"10.3847/0004-6256/152/6/197",
"10.48550/arXiv.1607.08613"
] | [
"Yan, Renbin",
"Bundy, Kevin",
"Law, David R.",
"Bershady, Matthew A.",
"Andrews, Brett",
"Cherinka, Brian",
"Diamond-Stanic, Aleksandar M.",
"Drory, Niv",
"MacDonald, Nicholas",
"Sánchez-Gallego, José R.",
"Thomas, Daniel",
"Wake, David A.",
"Weijmans, Anne-Marie",
"Westfall, Kyle B.",
... | [
"Department of Physics and Astronomy, University of Kentucky, 505 Rose Street, Lexington, KY 40506-0057, USA",
"Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan",
"Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA",
"Department of Astronomy, Uni... | [
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3127308 | 1607.05731 | Dissecting galaxies: spatial and spectral separation of emission excited by star formation and AGN activity | The optical spectra of Seyfert galaxies are often dominated by emission lines excited by both star formation and active galactic nucleus (AGN) activity. Standard calibrations (such as for the star formation rate) are not applicable to such composite (mixed) spectra. In this paper, we describe how integral field data ca... | [
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] | 5 | [
"10.1093/mnras/stw1754",
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"Davies, Rebecca L.",
"Groves, Brent",
"Kewley, Lisa J.",
"Dopita, Michael A.",
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"Banfield, Julie",
"Zaw, Ingyin",
"James, Bethan",
"Juneau, Stéphanie",
... | [
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2336654 | 1607.07444 | Observations of asymmetric velocity fields and gas cooling in the NGC 4636 galaxy group X-ray halo | <BR /> Aims: This study aims to probe the thermodynamic properties of the hot intragroup medium (IGM) plasma in the core regions of the NGC 4636 galaxy group by detailed measurements of several emission lines and their relative intensities. <BR /> Methods: We analyzed deep XMM-Newton Reflection Grating Spectrometer (RG... | [
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"Pinto, Ciro",
"Sanders, Jeremy",
"Kaastra, Jelle",
"de Plaa, Jelle",
"Fabian, Andrew"
] | [
"Department of PhysicsUniversity of Helsinki, 00014, Helsinki, Finland",
"Department of PhysicsUniversity of Helsinki, 00014, Helsinki, Finland",
"Institute of Astronomy, Madingley Road, CB3 0, HA Cambridge, UK",
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4247601 | 1607.00787 | Characterizing the Youngest Herschel-detected Protostars. II. Molecular Outflows from the Millimeter and the Far-infrared | We present Combined Array for Research in Millimeter-wave Astronomy (CARMA) CO (J=1\to 0) observations and Herschel PACS spectroscopy, characterizing the outflow properties toward extremely young and deeply embedded protostars in the Orion molecular clouds. The sample comprises a subset of the Orion protostars known as... | [
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12473269 | 1607.07672 | NLTE carbon abundance determination in selected A- and B-type stars and the interpretation of C I emission lines | We constructed a comprehensive model atom for C I-C II using the most up-to-date atomic data available and evaluated the non-local thermodynamic equilibrium (NLTE) line formation for C I and C II in classical 1D models representing the atmospheres of A- and late B-type stars. Our NLTE calculations predict the emission ... | [
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"Alexeeva, S. A.",
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"Institute of Astronomy of the Russian Academy of Sciences 48 Pyatnitskaya St. 119017 Moscow, Russia",
"Institute of Astronomy of the Russian Academy of Sciences 48 Pyatnitskaya St. 119017 Moscow, Russia"
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12406423 | 1607.05677 | Is there a concordance value for H<SUB>0</SUB>? | Context. We test the theoretical predictions of several cosmological models against different observables to compare the indirect estimates of the current expansion rate of the Universe determined from model fitting with the direct measurements based on Cepheids data published recently. <BR /> Aims: We perform a statis... | [
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"Luković, Vladimir V.",
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"Dipartimento di Fisica, Università di Roma \"Tor Vergata\", via della Ricerca Scientifica 1, 00133, Roma, Italy",
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12436208 | 1607.06397 | Measurements of gondola motion on a stratospheric balloon flight | Balloon experiments are an economically feasible method of conducting observations in astronomy that are not possible from the ground. The astronomical payload may include a telescope, a detector, and a pointing/stabilization system. Determining the attitude of the payload is of primary importance in such applications,... | [
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12620194 | 1607.03784 | 1 /c expansion of nonminimally coupled curvature-matter gravity models and constraints from planetary precession | The effects of a nonminimally coupled curvature-matter model of gravity on a perturbed Minkowski metric are presented. The action functional of the model involves two functions f<SUP>1</SUP>(R ) and f<SUP>2</SUP>(R ) of the Ricci scalar curvature R . This work expands upon previous results, extending the framework deve... | [
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] | 6 | [
"10.1103/PhysRevD.95.024017",
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"March, Riccardo",
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"Bertolami, Orfeu",
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"Departamento de Física e Astronomia and Centro de Física do Porto, Faculdade de Ciências da Universidade do Porto, Rua do Campo Aleg... | [
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2427974 | 1607.03267 | OGLE-2012-BLG-0950Lb: The First Planet Mass Measurement from Only Microlens Parallax and Lens Flux | We report the discovery of a microlensing planet OGLE-2012-BLG-0950Lb with a planet/host mass ratio of q≃ 2× {10}<SUP>-4</SUP>. A long term distortion detected in both MOA and OGLE light curve can be explained by the microlens parallax due to the Earth’s orbital motion around the Sun. Although the finite source effect ... | [
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] | 3 | [
"10.3847/1538-3881/153/1/1",
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"Koshimoto, N.",
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"Asakura, Y.",
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"Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan;",
"Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland;",
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12473071 | 1607.01054 | The isolation of luminous blue variables: on subdividing the sample | A debate has arisen concerning the fundamental nature of luminous blue variables (LBVs) and their role in stellar evolution. While Smith & Tombleson proposed that their isolated environments indicate that LBVs must be largely the product of binary evolution, Humphreys et al. have recently expressed the view that th... | [
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"those lower luminosity LBVs",
"et al",
"velocities",
"mass gainers",
"modest runway speeds",
"early O-type stars",
".",
"red supergiants",
... | [
"binaries: general",
"stars: evolution",
"stars: winds",
"outflows",
"Astrophysics - Solar and Stellar Astrophysics"
] | 7 | [
"10.1093/mnras/stw1533",
"10.48550/arXiv.1607.01054"
] | [
"Smith, Nathan"
] | [
"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA"
] | [
"2016ApJ...833..128M",
"2016MNRAS.463.2904S",
"2017A&A...603A..75L",
"2017ASPC..510..457K",
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12473085 | 1607.04995 | Searching for the optical counterparts of two young γ-ray pulsars | We report on the first deep optical observations of two γ-ray pulsars, both among the very first discovered by the Fermi Gamma-ray Space Telescope. The two pulsars are the radio-loud PSR J1907+0602 in the TeV pulsar wind nebula (PWN) MGRO J1908+06 and the radio-quiet PSR J1809-2332 in the `Taz' radio/X-ray PWN. These p... | [
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-... | 5.421006 | 4.733049 | 2016-07-01 | 3 | 2016MNRAS.463.2932M | [
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"-",
"+",
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"the Fermi Gamma-ray Space Telescope",
"VLT",
"their optical counterparts",
"TeV... | [
"stars: neutron",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 14 | [
"10.1093/mnras/stw2226",
"10.48550/arXiv.1607.04995"
] | [
"Mignani, R. P.",
"Testa, V.",
"Marelli, M.",
"De Luca, A.",
"Pierbattista, M.",
"Razzano, M.",
"Salvetti, D.",
"Belfiore, A.",
"Shearer, A.",
"Moran, P."
] | [
"INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica Milano, via E. Bassini 15, I-20133 Milano, Italy; Janusz Gil Institute of Astronomy, University of Zielona Góra, Lubuska 2, PL-65-265 Zielona Góra, Poland",
"INAF - Osservatorio Astronomico di Roma, via Frascati 33, I-00040 Monteporzio, Italy",
"INAF - I... | [
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14182734 | 1607.03051 | Design and expected performance of a novel hybrid detector for very-high-energy gamma-ray astrophysics | Current detectors for Very-High-Energy γ-ray astrophysics are either pointing instruments with a small field of view (Cherenkov telescopes), or large field-of-view instruments with relatively large energy thresholds (extensive air shower detectors). <P />In this article, we propose a new hybrid extensive air shower det... | [
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... | 6.99406 | 0.410704 | 2016-07-01 | 24 | 2018APh....99...34A | [
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"a new hybrid extensive air shower detector",
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"the accurate shower geome... | [
"Gamma-ray astronomy",
"Extensive air shower detectors",
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"Gamma-ray bursts",
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - High Energy Astrophysical Phenomena",
"High Energy Physics - Experiment"
] | 7 | [
"10.1016/j.astropartphys.2018.02.004",
"10.48550/arXiv.1607.03051"
] | [
"Assis, P.",
"Barres de Almeida, U.",
"Blanco, A.",
"Conceição, R.",
"D'Ettorre Piazzoli, B.",
"De Angelis, A.",
"Doro, M.",
"Fonte, P.",
"Lopes, L.",
"Matthiae, G.",
"Pimenta, M.",
"Shellard, R.",
"Tomé, B."
] | [
"LIP Lisboa, Portugal; IST Lisboa, Portugal",
"CBPF,Rio de Janeiro, Brazil",
"LIP Coimbra, University of Coimbra, Portugal",
"LIP Lisboa, Portugal; IST Lisboa, Portugal",
"Università di Napoli \"Federico II\" and INFN Roma Tor Vergata, Italy",
"INFN Padova, Italy; Università di Udine, Italy",
"Universit... | [
"2017AIPC.1792b0004D",
"2017EPJWC.13603013A",
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"2018EPJC...78..333A",
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"2019IEEEA...7k0531A",
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2933128 | 1607.03321 | Metal-rich or misclassified? The case of four RR Lyrae stars | We analysed the light curve of four, apparently extremely metal-rich fundamenta-mode RR Lyrae stars. We identified two stars, MT Tel and ASAS J091803-3022.6 as RRc (first-overtone) pulsators that were misclassified as RRab ones in the ASAS survey. In the case of the other two stars, V397 Gem and ASAS J075127-4136.3, we... | [
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"apparently extremely metal-rich fundamenta-mode RR Lyrae stars",
"the period-Fourier-... | [
"CCD photometry",
"Astrophysics - Solar and Stellar Astrophysics"
] | 6 | [
"10.48550/arXiv.1607.03321"
] | [
"Molnar, L.",
"Juhasz, A. L.",
"Plachy, E.",
"Szabo, R."
] | [
"-",
"-",
"-",
"-"
] | [
"2019ApJS..244...32P",
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3171598 | 1607.03117 | An unstable truth: how massive stars get their mass | The pressure exerted by massive stars' radiation fields is an important mechanism regulating their formation. Detailed simulation of massive star formation therefore requires an accurate treatment of radiation. However, all published simulations have either used a diffusion approximation of limited validity; have only ... | [
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... | 10.786679 | 10.291077 | 2016-07-01 | 108 | 2016MNRAS.463.2553R | [
"RT instabilities",
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"radiation",
"massive stars",
"stars",
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"massive stars radiation fields",
"the direct radiation field",
"interstellar dust",
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"hydrodynamics",
"instabilities",
"stars: formation",
"stars: massive",
"ISM: bubbles",
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 20 | [
"10.1093/mnras/stw2153",
"10.48550/arXiv.1607.03117"
] | [
"Rosen, Anna L.",
"Krumholz, Mark R.",
"McKee, Christopher F.",
"Klein, Richard I."
] | [
"Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 USA",
"Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia",
"Department of Astronomy, University of California, Berkeley, CA 94720, USA; Physics Department, Univers... | [
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2854570 | 1607.05526 | Using the local gas-phase oxygen abundances to explore a metallicity dependence in SNe Ia luminosities | We present an analysis of the gas-phase oxygen abundances of a sample of 28 galaxies in the local Universe (z < 0.02) hosting Type Ia supernovae (SNe Ia). The data were obtained with the 4.2 m William Herschel Telescope. We derive local oxygen abundances for the regions where the SNe Ia exploded by calculating oxyge... | [
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"SNe Ia",
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"local oxygen abundances",
"oxygen gradients",
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"non-reddened SNe",
"the SN Ia",
"the SNe Ia",
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"the oxygen abundance",
... | [
"methods: data analysis",
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"H II regions",
"galaxies: abundances",
"Astrophysics - Astrophysics of Galaxies",
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] | 4 | [
"10.1093/mnras/stw1706",
"10.48550/arXiv.1607.05526"
] | [
"Moreno-Raya, M. E.",
"López-Sánchez, Á. R.",
"Mollá, M.",
"Galbany, L.",
"Vílchez, J. M.",
"Carnero, A."
] | [
"Departamento de Investigación Básica, CIEMAT, Avda. Complutense 40, E-28040 Madrid, Spain",
"Australian Astronomical Observatory, PO Box 915, North Ryde, NSW 1670, Australia; Department of Physics and Astronomy, Macquarie University, NSW 2109, Australia",
"Departamento de Investigación Básica, CIEMAT, Avda. Co... | [
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12516680 | 1607.03874 | Evolution of Magnetic Helicity During Eruptive Flares and Coronal Mass Ejections | During eruptive solar flares and coronal mass ejections, a non-potential magnetic arcade with much excess magnetic energy goes unstable and reconnects. It produces a twisted erupting flux rope and leaves behind a sheared arcade of hot coronal loops. We suggest that the twist of the erupting flux rope can be determined ... | [
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0.... | 12.902495 | 16.174398 | 2016-07-01 | 20 | 2016SoPh..291.2017P | [
"magnetic helicity",
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"much excess magnetic energy",
"a non-potential magnetic arcade",
"hot coronal loops",
"coronal mass ejections",
"arcade",
"eruptive solar flares",
"reconnection",
"the initial pre-eruptive structure",
"the pre-eruptive state",
"a twisted erupting flux rop... | [
"Sun: flares",
"Sun: magnetic topology",
"Magnetic reconnection",
"Helicity",
"Astrophysics - Solar and Stellar Astrophysics"
] | 3 | [
"10.1007/s11207-016-0962-6",
"10.48550/arXiv.1607.03874"
] | [
"Priest, E. R.",
"Longcope, D. W.",
"Janvier, M."
] | [
"School of Mathematics and Statistics, University of St. Andrews, KY16 9SS, Scotland, Fife, UK",
"Dept. of Physics, Montana State University, Bozeman, MT, USA",
"School of Science and Engineering, University of Dundee, DD1 4HN, Dundee, UK; Institut d'Astrophysique Spatiale, UMR8617, Univ. Paris-Sud-CNRS, Univer... | [
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12473288 | 1607.01795 | Variable stars in the Quintuplet stellar cluster with the VVV survey<SUP>★</SUP> | The Quintuplet cluster is one of the most massive star clusters in the Milky Way, situated very close to the Galactic Centre. We present a new search for variable stars in the vicinity of the cluster, using the five-year data base of the Vista Variables in the Via Lactea (VVV) ESO Public Survey in the near-infrared. A ... | [
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... | 8.126454 | 9.767975 | 2016-07-01 | 9 | 2016MNRAS.462.1180N | [
"variable stars",
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"VVV",
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"long-period variables",
"the variable stars",
"slow/semiregular variables",
"the most massive star clusters",
"the cluster centre",
"K<SUB>S</SUB>-band variability",
"the Galactic Centre",
"variations",
... | [
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.1093/mnras/stw1613",
"10.48550/arXiv.1607.01795"
] | [
"Navarro Molina, Claudio",
"Borissova, J.",
"Catelan, M.",
"Alonso-García, J.",
"Kerins, E.",
"Kurtev, R.",
"Lucas, P. W.",
"Medina, N.",
"Minniti, D.",
"Dékány, I."
] | [
"Instituto de Física y Astronomía, Universidad de Valparaíso, Av. Gran Bretaña 1111, Playa Ancha, Casilla 5030, Valparaíso, Chile; Millennium Institute of Astrophysics, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile",
"Instituto de Física y Astronomía, Universidad de Valparaíso, Av. Gran Bretaña 1111, ... | [
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12464575 | 1607.05663 | Converting entropy to curvature perturbations after a cosmic bounce | We study two-field bouncing cosmologies in which primordial perturbations are created in either an ekpyrotic or a matter-dominated contraction phase. We use a non-singular ghost condensate bounce model to follow the perturbations through the bounce into the expanding phase of the universe. In contrast to the adiabatic ... | [
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"several beneficial implications",
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"matter bounce models",
"entropy perturbations",
"ekpyrotic models",
"a non-singular ghost condensate bounce model",
"the bounce phase",
"the associated primordial gravitational waves",
"large scales",
"Gaussianity",
"adiabatic/curva... | [
"High Energy Physics - Theory",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 7 | [
"10.1088/1475-7516/2016/10/005",
"10.48550/arXiv.1607.05663"
] | [
"Fertig, Angelika",
"Lehners, Jean-Luc",
"Mallwitz, Enno",
"Wilson-Ewing, Edward"
] | [
"Max Planck Institute for Gravitational Physics, Albert Einstein Institute, 14476 Potsdam-Golm, Germany",
"Max Planck Institute for Gravitational Physics, Albert Einstein Institute, 14476 Potsdam-Golm, Germany",
"Max Planck Institute for Gravitational Physics, Albert Einstein Institute, 14476 Potsdam-Golm, Germ... | [
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"2020PhRvD.101f3522B",
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12593770 | 1607.00270 | Constraining the dark energy equation of state using Bayes theorem and the Kullback-Leibler divergence | Data-driven model-independent reconstructions of the dark energy equation of state w(z) are presented using Planck 2015 era cosmic microwave background, baryonic acoustic oscillations (BAO), Type Ia supernova (SNIa) and Lyman α (Lyα) data. These reconstructions identify the w(z) behaviour supported by the data and show... | [
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"10.1093/mnras/stw3102",
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"Hee, S.",
"Vázquez, J. A.",
"Handley, W. J.",
"Hobson, M. P.",
"Lasenby, A. N."
] | [
"Astrophysics Group, Battcock Centre, Cavendish Laboratory, JJ Thomson Avenue, Cambridge CB3 0HE, UK; Kavli Institute for Cosmology Cambridge, Madingley Road, Cambridge CB3 0HA, UK",
"Brookhaven National Laboratory, 2 Center Road, Upton, NY 11973, USA",
"Astrophysics Group, Battcock Centre, Cavendish Laboratory... | [
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12517945 | 1607.02043 | Jets of SS 433 on scales of dozens of parsecs | Context. The radio nebula W 50 harbours the relativistic binary system <ASTROBJ>SS 433</ASTROBJ>, which is a source of powerful wind and jets. The origin of <ASTROBJ>W 50</ASTROBJ> is wrapped in the interplay of the wind, supernova remnant, and jets. The evolution of the jets of SS 433 on the scale of the nebula W 50 i... | [
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] | 6 | [
"10.1051/0004-6361/201629256",
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] | [
"Panferov, Alexander A."
] | [
"Institute of Mathematics, Physics and Information Technologies (IMFIT), Togliatti State University, Belorusskaya 14, 445667, Togliatti, Russia"
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12510923 | 1607.07450 | Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations | Binary neutron star mergers are promising sources of gravitational waves for ground-based detectors such as Advanced LIGO. Neutron-rich material ejected by these mergers may also be the main source of r-process elements in the Universe, while radioactive decays in the ejecta can power bright electromagnetic postmerger ... | [
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"10.1103/PhysRevD.94.123016",
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"Foucart, Francois",
"O'Connor, Evan",
"Roberts, Luke",
"Kidder, Lawrence E.",
"Pfeiffer, Harald P.",
"Scheel, Mark A."
] | [
"Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, California 94720, USA",
"Department of Physics, North Carolina State University, Raleigh, North Carolina 27695, USA",
"TAPIR, Walter Burke Institute for Theoretical Physics, MC 350-17, California Institute of Technology, Pasadena, California 91... | [
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12612018 | 1607.06937 | Optical spectroscopy of four young radio sources | We report the optical spectroscopy of four young radio sources which are observed with the Lijiang 2.4 m telescope. The Eddington ratios of these sources are similar with those of narrow-line Seyfert 1 galaxies (NLS1s). Their Fe II emission is strong while [O III] strength is weak. These results confirm the NLS1 featur... | [
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"10.1016/j.newast.2016.07.009",
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] | [
"Fan, Xu-Liang",
"Bai, Jin-Ming",
"Hu, Chen",
"Wang, Jian-Guo"
] | [
"Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China; Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China",
"Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China; Key Laboratory for the Structure and Evolu... | [
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12461495 | 1607.04874 | Cosmological implications of modified gravity induced by quantum metric fluctuations | We investigate the cosmological implications of modified gravities induced by the quantum fluctuations of the gravitational metric. If the metric can be decomposed as the sum of the classical and of a fluctuating part, of quantum origin, then the corresponding Einstein quantum gravity generates at the classical level m... | [
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0... | 10.355738 | 0.537676 | 2016-07-01 | 31 | 2016EPJC...76..420L | [
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"10.1140/epjc/s10052-016-4275-6",
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"Liu, Xing",
"Harko, Tiberiu",
"Liang, Shi-Dong"
] | [
"School of Physics, Sun Yat-Sen University, Guangzhou, People's Republic of China; Yat Sen School, Sun Yat-Sen University, Guangzhou, People's Republic of China",
"Department of Physics, Babes-Bolyai University, Cluj-Napoca, Romania; Department of Mathematics, University College London, London, UK",
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3556381 | 1607.06089 | Morphology Dependence of Stellar Age in Quenched Galaxies at Redshift ∼1.2: Massive Compact Galaxies Are Older than More Extended Ones | We report the detection of morphology-dependent stellar age in massive quenched galaxies (QGs) at z ∼ 1.2. The sense of the dependence is that compact QGs are 0.5-2 Gyr older than normal-sized ones. The evidence comes from three different age indicators—{D}<SUB>n</SUB>4000, {{{H}}}<SUB>δ </SUB>, and fits to spectral sy... | [
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0.006451... | 12.282971 | 6.562494 | 2016-07-01 | 43 | 2017ApJ...838...94W | [
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"10.3847/1538-4357/aa662f",
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"Williams, Christina C.",
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"Cappelluti, Nico",
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"Liu, Teng",
"Lee, Bomee",
"Tundo, Elena",
"Vanzella, Eros"
] | [
"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA",
"Department of Astronomy, University of Massachusetts, 710 North Pleasant Street, Amherst, MA 01003, USA",
"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA;",
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12586013 | 1607.03453 | Renormalization-group flow of the effective action of cosmological large-scale structures | Following an approach of Matarrese and Pietroni, we derive the functional renormalization group (RG) flow of the effective action of cosmological large-scale structures. Perturbative solutions of this RG flow equation are shown to be consistent with standard cosmological perturbation theory. Non-perturbative approximat... | [
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] | 5 | [
"10.1088/1475-7516/2017/01/048",
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] | [
"Floerchinger, Stefan",
"Garny, Mathias",
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] | [
"Institut für Theoretische Physik, Universität Heidelberg, Philosophenweg 16, 69120 Heidelberg, Germany",
"Theoretical Physics Department, CERN, CH-1211 Genève 23, Switzerland ; Centre de Physique Théorique, Ecole Polytechnique, CNRS, 91128 Palaiseau Cedex, France;",
"Theoretical Physics Department, CERN, CH-12... | [
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1635230 | 1607.08788 | Cluster abundance in chameleon f(R) gravity I: toward an accurate halo mass function prediction | We refine the mass and environment dependent spherical collapse model of chameleon f(R) gravity by calibrating a phenomenological correction inspired by the parameterized post-Friedmann framework against high-resolution N-body simulations. We employ our method to predict the corresponding modified halo mass function, a... | [
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"the parameterized post-Friedmann framework",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 24 | [
"10.1088/1475-7516/2016/12/024",
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] | [
"Cataneo, Matteo",
"Rapetti, David",
"Lombriser, Lucas",
"Li, Baojiu"
] | [
"Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark",
"Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark; Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, 816... | [
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4353175 | 1607.03386 | Probing the intra-group medium of a z = 0.28 galaxy group | We present new MUSE observations of a galaxy group probed by a background quasar. The quasar sightline passes between multiple z = 0.28 galaxies, whilst showing at the same redshift low-ionized metal line species, including Ca II, Mg I, Mg II and Fe II. Based on the galaxy redshifts measured from the MUSE data, we esti... | [
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"Mg II",
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"the intra-group medium",
"a galaxy group",
"the group galaxies",
"a single group member",
"stars",
"a single galaxy",... | [
"galaxies: groups: general",
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] | 11 | [
"10.1093/mnras/stx528",
"10.48550/arXiv.1607.03386"
] | [
"Bielby, R.",
"Crighton, N. H. M.",
"Fumagalli, M.",
"Morris, S. L.",
"Stott, J. P.",
"Tejos, N.",
"Cantalupo, S."
] | [
"Centre for Extragalactic Astronomy, Durham University, South Road, Durham DH1 3LE, UK",
"Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia",
"Centre for Extragalactic Astronomy, Durham University, South Road, Durham DH1 3LE, UK; Institute for Com... | [
"2017ASSL..430..145K",
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2418689 | 1607.00385 | A Model for (Quasi-)Periodic Multiwavelength Photometric Variability in Young Stellar Objects | We present radiation transfer models of rotating young stellar objects (YSOs) with hot spots in their atmospheres, inner disk warps, and other three-dimensional effects in the nearby circumstellar environment. Our models are based on the geometry expected from magneto-accretion theory, where material moving inward in t... | [
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-0... | 9.402853 | 11.598577 | 2016-07-01 | 21 | 2016ApJ...828...42K | [
"stellar hot spots",
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"stars: pre-main sequence",
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] | 3 | [
"10.3847/0004-637X/828/1/42",
"10.48550/arXiv.1607.00385"
] | [
"Kesseli, Aurora Y.",
"Petkova, Maya A.",
"Wood, Kenneth",
"Whitney, Barbara A.",
"Hillenbrand, L. A.",
"Gregory, Scott G.",
"Stauffer, J. R.",
"Morales-Calderon, M.",
"Rebull, L.",
"Alencar, S. H. P."
] | [
"Boston University, 725 Commonwealth Ave, Boston, MA 02215, USA",
"SUPA, School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews, Fife, KY16 9AD, UK",
"SUPA, School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews, Fife, KY16 9AD, UK",
"Department of A... | [
"2017MNRAS.465.3889R",
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2775839 | 1607.02663 | Similarity of jet radiation between flat spectrum radio quasars and GeV narrow-line Seyfert 1 galaxies: a universal δ-L <SUB>c</SUB> correlation | By modeling the broadband spectral energy distributions (SEDs) of a typical flat spectrum radio quasar (FSRQ, 3C 279) and two GeV narrow-line Seyfert 1 galaxies (NLS1s, PMN J0948+0022 and 1H 0323+342) in different flux stages with one-zone leptonic models, we find a universal correlation between their Doppler factors (... | [
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... | [
"Astrophysics - High Energy Astrophysical Phenomena"
] | 3 | [
"10.1088/1674-4527/16/11/170",
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] | [
"Zhu, Yong-Kai",
"Zhang, Jin",
"Zhang, Hai-Ming",
"Liang, En-Wei",
"Yan, Da-Hai",
"Cui, Wei",
"Zhang, Shuang-Nan"
] | [
"Guangxi Key Laboratory for Relativistic Astrophysics, Department of Physics, Guangxi University, Nanning 530004, China",
"Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China ; Department of Physics and Astronomy, Purdue Univer... | [
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12472956 | 1607.00499 | ExoMol molecular line lists - XVI. The rotation-vibration spectrum of hot H<SUB>2</SUB>S | This work presents the AYT2 line list: a comprehensive list of 115 million <SUP>1</SUP>H<SUB>2</SUB><SUP>32</SUP>S vibration-rotation transitions computed using an empirically adjusted potential energy surface and an ab initio dipole moment surface. The line list gives complete coverage up to 11 000 cm<SUP>-1</SUP> (wa... | [
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"an ab initio dipole moment surface",
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"(wavelengt... | [
"Astrophysics - Earth and Planetary Astrophysics"
] | 6 | [
"10.1093/mnras/stw1133",
"10.48550/arXiv.1607.00499"
] | [
"Azzam, Ala'a. A. A.",
"Tennyson, Jonathan",
"Yurchenko, Sergei N.",
"Naumenko, Olga V."
] | [
"Department of Physics and Astronomy, University College London, London WC1E 6BT, UK; Department of Physics, The University of Jordan, Queen Rania Street, Amman 11942, Jordan",
"Department of Physics and Astronomy, University College London, London WC1E 6BT, UK",
"Department of Physics and Astronomy, University... | [
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12409118 | 1607.07046 | Effect of Spectral Index Distribution on Estimating the AGN Radio Luminosity Function | In this paper, we scrutinize the effect of spectral index distribution on estimating the active galactic nucleus radio luminosity function (RLF) by a Monte Carlo method. We find that the traditional bivariate RLF estimators can cause bias in varying degrees. The bias is especially pronounced for the flat-spectrum radio... | [
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0.0228... | 14.968842 | 6.313339 | 2016-07-01 | 5 | 2016ApJ...829...95Y | [
"RLF",
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"galaxies: active",
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"radio continuum: galaxies",
"Astrophysics - High Energy Astrophysical Phenomena",
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] | 6 | [
"10.3847/0004-637X/829/2/95",
"10.48550/arXiv.1607.07046"
] | [
"Yuan, Zunli",
"Wang, Jiancheng",
"Zhou, Ming",
"Mao, Jirong"
] | [
"Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China ; Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China;",
"Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China ; Key Laboratory for the Structure and E... | [
"2017ApJ...840...46I",
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12510302 | 1607.07877 | Quartic chameleons: Safely scale-free in the early Universe | In chameleon gravity, there exists a light scalar field that couples to the trace of the stress-energy tensor in such a way that its mass depends on the ambient matter density, and the field is screened in local, high-density environments. Recently it was shown that, for the runaway potentials commonly considered in ch... | [
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0... | 9.699926 | 0.915294 | 2016-07-01 | 2 | 2016PhRvD..94j4049M | [
"runaway potentials",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 4 | [
"10.1103/PhysRevD.94.104049",
"10.48550/arXiv.1607.07877"
] | [
"Miller, Carisa",
"Erickcek, Adrienne L."
] | [
"Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Phillips Hall CB3255, Chapel Hill, North Carolina 27599, USA",
"Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Phillips Hall CB3255, Chapel Hill, North Carolina 27599, USA"
] | [
"2018LRR....21....1B",
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4474935 | 1607.02513 | ALMA Observations of the Debris Disk of Solar Analog τ Ceti | We present 1.3 mm observations of the Sun-like star τ Ceti with the Atacama Large Millimeter/submillimeter Array that probe angular scales of ∼ 1<SUP>\prime\prime</SUP> (4 au). This first interferometric image of the τ Ceti system, which hosts both a debris disk and a possible multiplanet system, shows emission from a ... | [
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0.0015687099657952785... | 9.260272 | 12.993963 | 2016-07-01 | 35 | 2016ApJ...828..113M | [
"narrow belts",
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"an unresolved central source",
"parametric models",
"a... | [
"circumstellar matter",
"stars: individual: τ Ceti",
"submillimeter: planetary systems",
"Astrophysics - Solar and Stellar Astrophysics",
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] | 7 | [
"10.3847/0004-637X/828/2/113",
"10.48550/arXiv.1607.02513"
] | [
"MacGregor, Meredith A.",
"Lawler, Samantha M.",
"Wilner, David J.",
"Matthews, Brenda C.",
"Kennedy, Grant M.",
"Booth, Mark",
"Di Francesco, James"
] | [
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"National Research Council of Canada, Herzberg Astronomy & Astrophysics Program, Victoria, BC V9E 2E7, Canada",
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"National Re... | [
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12470281 | 1607.05934 | Landau quantization and neutron emissions by nuclei in the crust of a magnetar | Magnetars are neutron stars endowed with surface magnetic fields of the order of 10<SUP>14</SUP> - 10<SUP>15</SUP> G, and with presumably much stronger fields in their interior. As a result of Landau quantization of electron motion, the neutron-drip transition in the crust of a magnetar is shifted to either higher or l... | [
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0... | 4.987517 | 2.905418 | 2016-07-01 | 5 | 2016JPhCS.724a2034C | [
"surface magnetic fields",
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"Brussels",
"the threshold density",
"neu... | [
"Astrophysics - High Energy Astrophysical Phenomena",
"Nuclear Theory"
] | 2 | [
"10.1088/1742-6596/724/1/012034",
"10.48550/arXiv.1607.05934"
] | [
"Chamel, N.",
"Mutafchieva, Y. D.",
"Stoyanov, Zh K.",
"Mihailov, L. M.",
"Pavlov, R. L."
] | [
"Institute of Astronomy and Astrophysics, Université Libre de Bruxelles, CP 226, Boulevard du Triomphe, B-1050 Brussels, Belgium",
"Institute for Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences, 72 Tsarigradsko Chaussee, 1784 Sofia, Bulgaria",
"Institute for Nuclear Research and Nuclear Energ... | [
"2018ASSL..457..337B",
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5398079 | 1607.08006 | Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere Using Six Years of IceCube Data | The IceCube Collaboration has previously discovered a high-energy astrophysical neutrino flux using neutrino events with interaction vertices contained within the instrumented volume of the IceCube detector. We present a complementary measurement using charged current muon neutrino events where the interaction vertex c... | [
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0... | 5.85455 | -0.543142 | 2016-07-01 | 413 | 2016ApJ...833....3A | [
"reconstructed muon energies",
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"neutrino flux",
"charged current muon",
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"previous IceCube analyses",
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"astroparticle physics",
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] | 23 | [
"10.3847/0004-637X/833/1/3",
"10.48550/arXiv.1607.08006"
] | [
"Aartsen, M. G.",
"Abraham, K.",
"Ackermann, M.",
"Adams, J.",
"Aguilar, J. A.",
"Ahlers, M.",
"Ahrens, M.",
"Altmann, D.",
"Andeen, K.",
"Anderson, T.",
"Ansseau, I.",
"Anton, G.",
"Archinger, M.",
"Argüelles, C.",
"Auffenberg, J.",
"Axani, S.",
"Bai, X.",
"Barwick, S. W.",
"Bau... | [
"Department of Physics, University of Adelaide, Adelaide, 5005, Australia",
"Physik-department, Technische Universität München, D-85748 Garching, Germany",
"DESY, D-15735 Zeuthen, Germany",
"Dept. of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand",
"Université L... | [
"2016ApJ...832...20X",
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2500994 | 1607.03778 | Gamma-ray Upper Limits on Magnetars with Six Years of Fermi-LAT Observations | We report on the search for gamma-ray emission from 20 magnetars using six years of Fermi Large Area Telescope observations. No significant evidence for gamma-ray emission from any of the currently known magnetars is found. We derived the most stringent upper limits to date on the 0.1-10 GeV emission of Galactic magnet... | [
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-0.... | 5.433737 | 3.976502 | 2016-07-01 | 28 | 2017ApJ...835...30L | [
"Fermi Large Area Telescope observations",
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"10.3847/1538-4357/835/1/30",
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] | [
"Li, Jian",
"Rea, Nanda",
"Torres, Diego F.",
"de Oña-Wilhelmi, Emma"
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"Institute of Space Sciences (IEEC–CSIC), Campus UAB, Carrer de Magrans s/n, E-08193 Barcelona, Spain",
"Institute of Space Sciences (IEEC–CSIC), Campus UAB, Carrer de Magrans s/n, E-08193 Barcelona, Spain; Anton Pannekoek Institute for Astronomy, University of Amsterdam, Postbus 94249, NL-1090 GE Amsterdam, The ... | [
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12517460 | 1607.04644 | A neural network gravitational arc finder based on the Mediatrix filamentation method | Context. Automated arc detection methods are needed to scan the ongoing and next-generation wide-field imaging surveys, which are expected to contain thousands of strong lensing systems. Arc finders are also required for a quantitative comparison between predictions and observations of arc abundance. Several algorithms... | [
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12472930 | 1607.06194 | An information theory based search for homogeneity on the largest accessible scale | We analyse the Sloan Digital Sky Survey Data Release 12 quasar catalogue to test the large-scale smoothness in the quasar distribution. We quantify the degree of inhomogeneity in the quasar distribution using information theory based measures and find that the degree of inhomogeneity diminishes with increasing length s... | [
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"Sarkar, Suman",
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1821095 | 1607.05532 | Magnetic field evolution and reversals in spiral galaxies | We study the evolution of galactic magnetic fields using 3D smoothed particle magnetohydrodynamics (SPMHD) simulations of galaxies with an imposed spiral potential. We consider the appearance of reversals of the field, and amplification of the field. We find that magnetic field reversals occur when the velocity jump ac... | [
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12520275 | 1607.02915 | Interpretation of the historic Yemeni reports of supernova SN 1006: Early discovery in mid-April 1006? | The recently published Yemeni observation report about SN 1006 from al-Yamānī clearly gives AD 1006 April 17 ± 2 (mid-Rajab 396h) as the first observation date. Since this is ∼1.5 weeks earlier than the otherwise earliest reports (April 28 or 30) as discussed so far, we were motivated to investigate an early sighting i... | [
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12436480 | 1607.06916 | General features of single-scalar field dark energy models | We present a systematic study of modified gravity (MG) models containing a single scalar field non-minimally coupled to the metric. Despite a large parameter space, exploiting the effective field theory of dark energy (EFT of DE) formulation and imposing simple physical constraints such as stability conditions and (sub... | [
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0... | 10.881541 | 0.568483 | 2016-07-01 | 2 | 2016arXiv160706916P | [
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] | 3 | [
"10.48550/arXiv.1607.06916"
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"Perenon, Louis"
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"-"
] | [
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12593550 | 1607.07910 | Simultaneous constraints on cosmology and photometric redshift bias from weak lensing and galaxy clustering | We investigate the expected cosmological constraints from a combination of cosmic shear and large-scale galaxy clustering using realistic photometric redshift distributions. Introducing a systematic bias in the lensing distributions (of 0.05 in redshift) produces a >2σ bias in the recovered matter power spectrum amp... | [
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0.... | 12.25819 | 3.528267 | 2016-07-01 | 17 | 2017MNRAS.465L..20S | [
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] | 5 | [
"10.1093/mnrasl/slw201",
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"Samuroff, S.",
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"Jodrell Bank Centre for Astrophysics, University of Manchester, Oxford Road, Manchester M13 9PL, UK",
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12406458 | 1607.07317 | Stellar mass distribution of S<SUP>4</SUP>G disk galaxies and signatures of bar-induced secular evolution | Context. Models of galaxy formation in a cosmological framework need to be tested against observational constraints, such as the average stellar density profiles (and their dispersion) as a function of fundamental galaxy properties (e.g. the total stellar mass). Simulation models predict that the torques produced by st... | [
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] | 10 | [
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"Díaz-García, S.",
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"Astronomy Research Group, University of Oulu, 90014, Oulu, Finland",
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2775130 | 1607.05312 | A MegaCam Survey of Outer Halo Satellites. VI. The Spatially Resolved Star-formation History of the Carina Dwarf Spheroidal Galaxy | We present the spatially resolved star-formation history (SFH) of the Carina dwarf spheroidal galaxy, obtained from deep, wide-field g and r imaging and a metallicity distribution from the literature. Our photometry covers ∼2 deg<SUP>2</SUP>, reaching up to ∼10 times the half-light radius of Carina with a completeness ... | [
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"Departamento de Astronomía, Universidad de Chile, Camino El Observatorio 1515, Las Condes, Santiago, Chile",
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1296310 | 1607.07245 | A GMRT survey of regions towards the Taurus molecular cloud at 323 and 608 MHz | We present observations of three active sites of star formation in the Taurus molecular cloud complex taken at 323 and 608 MHz (90 and 50 cm, respectively) with the Giant Metrewave Radio Telescope (GMRT). Three pointings were observed as part of a pathfinder project, targeted at the young stellar objects (YSOs) L1551 I... | [
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"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - Solar and Stellar Astrophysics"
] | 3 | [
"10.1093/mnras/stw1847",
"10.48550/arXiv.1607.07245"
] | [
"Ainsworth, Rachael E.",
"Coughlan, Colm P.",
"Green, David A.",
"Scaife, Anna M. M.",
"Ray, Tom P."
] | [
"Dublin Institute for Advanced Studies, School of Cosmic Physics, 31 Fitzwilliam Place, Dublin D02 XF86, Ireland",
"Dublin Institute for Advanced Studies, School of Cosmic Physics, 31 Fitzwilliam Place, Dublin D02 XF86, Ireland",
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5087092 | 1607.05289 | Molecular and atomic gas along and across the main sequence of star-forming galaxies | We use spectra from the ALFALFA, GASS and COLD GASS surveys to quantify variations in the mean atomic and molecular gas mass fractions throughout the SFR-M<SUB>*</SUB> plane and along the main sequence (MS) of star-forming galaxies. Although galaxies well below the MS tend to be undetected in the Arecibo and IRAM obser... | [
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"sta... | [
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] | 20 | [
"10.1093/mnras/stw1715",
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"Saintonge, Amelie",
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"Lutz, Katharina A.",
"Schiminovich, David",
"Tacconi, Linda J.",
"Wuyts, Stijn",
"Accurso, Gioacchino"
] | [
"Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK",
"International Centre for Radio Astronomy Research (ICRAR), The University of Western Australia, Perth, WA 6009, Australia",
"International Centre for Radio Astronomy Research (ICRAR), The University of Western ... | [
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12516984 | 1607.05847 | Early-time signatures of γ-ray emission from supernovae in dense circumstellar media | We present our results on the γ-ray emission from interaction-powered supernovae (SNe), a recently discovered SN type that is suggested to be surrounded by a circumstellar medium (CSM) with densities 10^7-10^12~ cm^-3. Such high densities favor inelastic collisions between relativistic protons accelerated in the SN bla... | [
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... | 3.930745 | 4.423158 | 2016-07-01 | 0 | 2016sros.confE.139K | [
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] | 3 | [
"10.48550/arXiv.1607.05847"
] | [
"Kantzas, Dimitrios",
"Petropoulou, Maria",
"Mastichiadis, Apostolos"
] | [
"University of Athens, Greece",
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12434965 | 1607.02460 | Through the Big Bang | All measurements are comparisons. The only physically accessible degrees of freedom (DOFs) are dimensionless ratios. The objective description of the universe as a whole thus predicts only how these ratios change collectively as one of them is changed. Here we develop a description for classical Bianchi IX cosmology im... | [
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"General Relativity and Quantum Cosmology",
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] | 8 | [
"10.48550/arXiv.1607.02460"
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"Koslowski, Tim A",
"Mercati, Flavio",
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"-",
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4925402 | 1607.06075 | The relationship between star formation activity and galaxy structural properties in CANDELS and a semi-analytic model | We study the correlation of galaxy structural properties with their location relative to the SFR-M<SUB>*</SUB> correlation, also known as the star formation `star-forming main sequence' (SFMS), in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey and Galaxy and Mass Assembly Survey and in a semi-analyt... | [
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0.0076... | 12.037335 | 6.900483 | 2016-07-01 | 47 | 2017MNRAS.465..619B | [
"lower SFR density",
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"galaxies: bulges",
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"Astrophysics - Astrophysics of Galaxies"
] | 7 | [
"10.1093/mnras/stw2690",
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] | [
"Brennan, Ryan",
"Pandya, Viraj",
"Somerville, Rachel S.",
"Barro, Guillermo",
"Bluck, Asa F. L.",
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"Wuyts, Stijn",
"Bell, Eric F.",
"Dekel, Avishai",
"Faber, Sandra",
"Ferguson, Henry C.",
"Koekemoer, Anton M.",
"Kurczynski, Peter",
"McIntosh, Daniel H.",
"Newman, Je... | [
"Department of Physics and Astronomy, Rutgers, The State University of New Jersey, 136 Frelinghuysen Rd, Piscataway, NJ 08854, USA",
"Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USA",
"Department of Physics and Astronomy, Rutgers, The State University of New Jer... | [
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2307884 | 1607.06769 | The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Continuum Number Counts, Resolved 1.2 mm Extragalactic Background, and Properties of the Faintest Dusty Star-forming Galaxies | We present an analysis of a deep (1σ = 13 μJy) cosmological 1.2 mm continuum map based on ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field. In the 1 arcmin<SUP>2</SUP> covered by ASPECS we detect nine sources at \gt 3.5σ significance at 1.2 mm. Our ALMA-selected sample has a median redshift of z=1.6... | [
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] | 25 | [
"10.3847/1538-4357/833/1/68",
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"Aravena, M.",
"Decarli, R.",
"Walter, F.",
"Da Cunha, E.",
"Bauer, F. E.",
"Carilli, C. L.",
"Daddi, E.",
"Elbaz, D.",
"Ivison, R. J.",
"Riechers, D. A.",
"Smail, I.",
"Swinbank, A. M.",
"Weiss, A.",
"Anguita, T.",
"Assef, R. J.",
"Bell, E.",
"Bertoldi, F.",
"Bacon, R.",
"Bouwen... | [
"Núcleo de Astronomía, Facultad de Ingeniería, Universidad Diego Portales, Av. Ejército 441, Santiago, Chile",
"Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany",
"Max-Planck Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany; Astronomy Department, California Ins... | [
"2016A&A...596A..75S",
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12406226 | 1607.03699 | Glancing through the accretion column of EXO 2030+375 | Context. The current generation of X-ray instruments progressively reveals more and more details about the complex magnetic field topology and the geometry of the accretion flows in highly magnetized accretion-powered pulsars. <BR /> Aims: We took advantage of the large collecting area and good timing capabilities of t... | [
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"X-ray instruments",
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"possible spectral variations",
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"the neutron star spin period",
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"X-rays: binaries",
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"pulsars: individual: EXO 2030+375",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 9 | [
"10.1051/0004-6361/201527837",
"10.48550/arXiv.1607.03699"
] | [
"Ferrigno, Carlo",
"Pjanka, Patryk",
"Bozzo, Enrico",
"Klochkov, Dmitry",
"Ducci, Lorenzo",
"Zdziarski, Andrzej A."
] | [
"ISDC, Department of astronomy, University of Geneva, chemin d'Écogia 16, 1290, Versoix, Switzerland",
"Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, NJ, 08544, Princeton, USA; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00-716, Warszawa, Poland",
... | [
"2017A&A...606A..89F",
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12408839 | 1607.03520 | Panchromatic Imaging of a Transitional Disk: The Disk of GM Aur in Optical and FUV Scattered Light | We have imaged GM Aurigae with the Hubble Space Telescope, detected its disk in scattered light at 1400 and 1650 Å, and compared these with observations at 3300 Å, 5550 Å, 1.1 μm, and 1.6 μm. The scattered light increases at shorter wavelengths. The radial surface brightness profile at 3300 Å shows no evidence of the 2... | [
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... | 9.662555 | 12.508538 | 2016-07-01 | 11 | 2016ApJ...829...65H | [
"dust grain opacity models",
"submillimeter observations",
"submicron grains",
"Barbara Whitney",
"the submillimeter cavity wall",
"observations",
"the submillimeter cavity",
"scattered light",
"the Monte Carlo radiative transfer code",
"an observed cavity",
"Surveys/Solar Blind Channel",
"sho... | [
"circumstellar matter",
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"stars: protostars",
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"Herbig Ae/Be",
"ultraviolet: planetary systems",
"Astrophysics - Solar and Stellar Astrophysics"
] | 7 | [
"10.3847/0004-637X/829/2/65",
"10.48550/arXiv.1607.03520"
] | [
"Hornbeck, J. B.",
"Swearingen, J. R.",
"Grady, C. A.",
"Williger, G. M.",
"Brown, A.",
"Sitko, M. L.",
"Wisniewski, J. P.",
"Perrin, M. D.",
"Lauroesch, J. T.",
"Schneider, G.",
"Apai, D.",
"Brittain, S.",
"Brown, J. M.",
"Champney, E. H.",
"Hamaguchi, K.",
"Henning, Th.",
"Lynch, D... | [
"Department of Physics & Astronomy, University of Louisville, Louisville, KY 40292, USA",
"Department of Physics, University of Cincinnati, 400 Geology/Physics Building, P.O. Box 210011, Cincinnati, OH 45221-0377, USA",
"Eureka Scientific, 2452 Delmer Street, Suite 100, Oakland, CA 96402, USA ; Exoplanets a... | [
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12409560 | 1607.07465 | The Dynamical Generation of Current Sheets in Astrophysical Plasma Turbulence | Turbulence profoundly affects particle transport and plasma heating in many astrophysical plasma environments, from galaxy clusters to the solar corona and solar wind to Earth's magnetosphere. Both fluid and kinetic simulations of plasma turbulence ubiquitously generate coherent structures, in the form of current sheet... | [
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0.0... | 12.78839 | 14.530781 | 2016-07-01 | 34 | 2016ApJ...827L..28H | [
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"plasmas",
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] | 6 | [
"10.3847/2041-8205/827/2/L28",
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] | [
"Howes, Gregory G."
] | [
"Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA"
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12406907 | 1607.01844 | A Monte Carlo Method for Making the SDSS u-Band Magnitude More Accurate | We develop a new Monte Carlo-based method to convert the Sloan Digital Sky Survey (SDSS) u-band magnitude to the south Galactic Cap of the u-band Sky Survey (SCUSS) u-band magnitude. Due to the increased accuracy of SCUSS u-band measurements, the converted u-band magnitude becomes more accurate compared with the origin... | [
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0.0... | 8.46212 | 9.52484 | 2016-07-01 | 1 | 2016AJ....152..106G | [
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] | 6 | [
"10.3847/0004-6256/152/4/106",
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"Gu, Jiayin",
"Du, Cuihua",
"Zuo, Wenbo",
"Jing, Yingjie",
"Wu, Zhenyu",
"Ma, Jun",
"Zhou, Xu"
] | [
"Department of Physics, Wuhan University of Technology, Wuhan 430000, People's Republic of China",
"School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China",
"School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, People... | [
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3237743 | 1607.03593 | Tidal deformability and I-Love-Q relations for gravastars with polytropic thin shells | The moment of inertia, the spin-induced quadrupole moment, and the tidal Love number of neutron-star and quark-star models are related through some relations which depend only mildly on the stellar equation of state. These "I-Love-Q" relations have important implications for astrophysics and gravitational-wave astronom... | [
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] | 5 | [
"10.1103/PhysRevD.94.064015",
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] | [
"Uchikata, Nami",
"Yoshida, Shijun",
"Pani, Paolo"
] | [
"Department of Physics, Rikkyo University, Nishi-ikebukuro, Toshima-ku, Tokyo 171-8501, Japan; Department of Mathematics and Physics, Graduate School of Science, Osaka City University, Sumiyoshi-ku, Osaka 558-8585, Japan",
"Astronomical Institute, Tohoku University, Aramaki-Aoba, Aoba-ku, Sendai 980-8578, Japan",... | [
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12434876 | 1607.01769 | Detecting patchy reionization in the CMB | Upcoming cosmic microwave background (CMB) experiments will measure temperature fluctuations on small angular scales with unprecedented precision. Small-scale CMB fluctuations are a mixture of late-time effects: gravitational lensing, Doppler shifting of CMB photons by moving electrons (the kSZ effect), and residual fo... | [
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15138610 | 1607.03907 | Erratum: “External Compton Scattering in Blazar Jets and the Location of the Gamma-Ray Emitting Region” (<A href="http://doi.org/10.3847/0004-637x/830/2/94">2016, ApJ, 830, 94</A>) | I study the location of the $\gamma$-ray emission in blazar jets by creating a Compton-scattering approximation valid for all anisotropic radiation fields in the Thomson through Klein-Nishina regimes, which is highly accurate and can speed up numerical calculations by up to a factor $\sim10$. I apply this approximation... | [
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"10.3847/1538-4357/aac9c6",
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] | [
"Finke, Justin D."
] | [
"U.S. Naval Research Laboratory, Code 7653, 4555 Overlook Ave. SW, Washington, DC 20375-5352, USA"
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4718718 | 1607.08538 | Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions | I start by providing an updated summary of the penalized pixel-fitting (PPXF) method that is used to extract the stellar and gas kinematics, as well as the stellar population of galaxies, via full spectrum fitting. I then focus on the problem of extracting the kinematics when the velocity dispersion σ is smaller than t... | [
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... | 10.915155 | 6.437457 | 2016-07-01 | 940 | 2017MNRAS.466..798C | [
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"10.1093/mnras/stw3020",
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"Cappellari, Michele"
] | [
"Sub-department of Astrophysics, Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK"
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12594048 | 1607.03136 | Variations of cosmic large-scale structure covariance matrices across parameter space | The likelihood function for cosmological parameters, given by e.g. weak lensing shear measurements, depends on contributions to the covariance induced by the non-linear evolution of the cosmic web. As highly non-linear clustering to date has only been described by numerical N-body simulations in a reliable and sufficie... | [
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... | 12.127925 | 2.969891 | 2016-07-01 | 15 | 2017MNRAS.465.4016R | [
"parameter space",
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"10.1093/mnras/stw2976",
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] | [
"Reischke, Robert",
"Kiessling, Alina",
"Schäfer, Björn Malte"
] | [
"Zentrum für Astronomie der Universität Heidelberg, Astronomisches Recheninstitut, Philosophenweg 12, D-69120 Heidelberg, Germany",
"Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California, USA",
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1340278 | 1607.06239 | High-energy gamma-ray observations of the accreting black hole V404 Cygni during its 2015 June outburst | We report on Fermi/Large Area Telescope observations of the accreting black hole low-mass X-ray binary V404 Cygni during its outburst in 2015 June-July. Detailed analyses reveal a possible excess of γ-ray emission on 2015 26 June, with a very soft spectrum above 100 MeV, at a position consistent with the direction of V... | [
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] | 7 | [
"10.1093/mnrasl/slw142",
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"Loh, A.",
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"Laboratoire AIM (CEA/IRFU-CNRS/INSU-Univ. Paris Diderot), CEA DSM/IRFU/SAp, F-91191 Gif-sur-Yvette, France",
"Laboratoire AIM (CEA/IRFU-CNRS/INSU-Univ. Paris Diderot), CEA DSM/IRFU/SAp, F-91191 Gif-sur-Yvette, France; Station de Radioastronomie de Nançay, Observatoire de Paris, PSL Research University, CNRS, Uni... | [
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1104522 | 1607.01023 | Numerical Simulations Challenged on the Prediction of Massive Subhalo Abundance in Galaxy Clusters: The Case of Abell 2142 | In this Letter we compare the abundance of the member galaxies of a rich, nearby (z = 0.09) galaxy cluster, Abell 2142, with that of halos of comparable virial mass extracted from sets of state-of-the-art numerical simulations, both collisionless at different resolutions and with the inclusion of baryonic physics in th... | [
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] | 3 | [
"10.3847/2041-8205/827/1/L5",
"10.48550/arXiv.1607.01023"
] | [
"Munari, E.",
"Grillo, C.",
"De Lucia, G.",
"Biviano, A.",
"Annunziatella, M.",
"Borgani, S.",
"Lombardi, M.",
"Mercurio, A.",
"Rosati, P."
] | [
"Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark ; INAF—Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143, Trieste, Italy ; Dipartimento di Fisica, Università degli Studi di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Ita... | [
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12406366 | 1607.08334 | Suzaku and XMM-Newton observations of the North Polar Spur: Charge exchange or ISM absorption? | By revisiting the Suzaku and XMM-Newton data of the North Polar Spur, we discovered that the spectra are inconsistent with the traditional model consisting of pure thermal emission and neutral absorption. The most prominent discrepancies are the enhanced O vii and Ne ix forbidden-to-resonance ratios, and a high O viii ... | [
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] | 5 | [
"10.1051/0004-6361/201628609",
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] | [
"Gu, Liyi",
"Mao, Junjie",
"Costantini, Elisa",
"Kaastra, Jelle"
] | [
"SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands",
"SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands",
"SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, The Netherlands",
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12614223 | 1607.06329 | Universal features of quantum bounce in loop quantum cosmology | In this Letter, we study analytically the evolutions of the flat Friedmann-Lemaitre-Robertson-Walker (FLRW) universe and its linear perturbations in the framework of the dressed metric approach in loop quantum cosmology (LQC). Assuming that the evolution of the background is dominated by the kinetic energy of the infla... | [
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] | 6 | [
"10.1016/j.physletb.2017.08.025",
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] | [
"Zhu, Tao",
"Wang, Anzhong",
"Kirsten, Klaus",
"Cleaver, Gerald",
"Sheng, Qin"
] | [
"Institute for Advanced Physics & Mathematics, Zhejiang University of Technology, Hangzhou, 310032, China",
"Institute for Advanced Physics & Mathematics, Zhejiang University of Technology, Hangzhou, 310032, China",
"GCAP-CASPER, Mathematics Department, Baylor University, Waco, TX 76798-7328, USA",
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12436224 | 1607.06059 | Modelling multimodal photometric redshift regression with noisy observations | In this work, we are trying to extent the existing photometric redshift regression models from modeling pure photometric data back to the spectra themselves. To that end, we developed a PCA that is capable of describing the input uncertainty (including missing values) in a dimensionality reduction framework. With this ... | [
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... | 11.903533 | 4.517343 | 2016-07-01 | 4 | 2016arXiv160706059K | [
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] | 3 | [
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"Kügler, S. D.",
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1963660 | 1607.01954 | MICADO: first light imager for the E-ELT | MICADO will equip the E-ELT with a first light capability for diffraction limited imaging at near-infrared wavelengths. The instrument's observing modes focus on various flavours of imaging, including astrometric, high contrast, and time resolved. There is also a single object spectroscopic mode optimised for wavelengt... | [
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] | 9 | [
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... | [
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"Max Planck Institute for Extraterrestrial Physics (Germany)",
"Univ. of Vienna (Austria)",
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12472758 | 1607.06868 | Formation and evolution of blue compact dwarfs: the origin of their steep rotation curves | The origin of the observed steep rotation curves of blue compact dwarf galaxies (BCDs) remains largely unexplained by theoretical models of BCD formation. We therefore investigate the rotation curves in BCDs formed from mergers between gas-rich dwarf irregular galaxies based on the results of numerical simulations for ... | [
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] | 5 | [
"10.1093/mnras/stw1812",
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] | [
"Watts, Adam",
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">ICRAR M468, The University of Western Australia, 35 Stirling Hwy, Crawley, WA 6009, Australia</aff>",
">ICRAR M468, The University of Western Australia, 35 Stirling Hwy, Crawley, WA 6009, Australia</aff>"
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12408587 | 1607.02350 | Reconciling the Orbital and Physical Properties of the Martian Moons | The origin of Phobos and Deimos is still an open question. Currently, none of the three proposed scenarios for their origin (intact capture of two distinct outer solar system small bodies, co-accretion with Mars, and accretion within an impact-generated disk) are able to reconcile their orbital and physical properties.... | [
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"two distinct outer solar system small bodies",
"an unlikely capture scenario",
"an impact-genera... | [
"planets and satellites: composition",
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] | 6 | [
"10.3847/0004-637X/828/2/109",
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"Ronnet, T.",
"Vernazza, P.",
"Mousis, O.",
"Brugger, B.",
"Beck, P.",
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"Witasse, O.",
"Cipriani, F."
] | [
"Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, F-13388, Marseille, France",
"Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, F-13388, Marseille, France",
"Aix Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marse... | [
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12586057 | 1607.05600 | Gravitomagnetic effect in magnetized neutron stars | Rotating bodies in General Relativity produce frame dragging, also known as the gravitomagnetic effect in analogy with classical electromagnetism. In this work, we study the effect of magnetic field on the gravitomagnetic effect in neutron stars with poloidal geometry, which is produced as a result of its rotation. We ... | [
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"10.1088/1475-7516/2017/01/062",
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"Chatterjee, Debarati",
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"LPC/ENSICAEN, 6 Boulevard Maréchal Juin, Caen, 14050 France",
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1361182 | 1607.02216 | Search for continuous gravitational waves from neutron stars in globular cluster NGC 6544 | We describe a directed search for continuous gravitational waves in data from the sixth initial LIGO science run. The target was the nearby globular cluster NGC 6544 at a distance of ≈2.7 kpc . The search covered a broad band of frequencies along with first and second frequency derivatives for a fixed sky position. The... | [
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"10.1103/PhysRevD.95.082005",
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"Abbott, B. P.",
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"Ain, A.",
"Al... | [
"California Institute of Technology, Pasadena, California 91125, USA",
"California Institute of Technology, Pasadena, California 91125, USA",
"Louisiana State University, Baton Rouge, Louisiana 70803, USA",
"American University, Washington, D.C. 20016, USA",
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12515523 | 1607.07928 | Shape parameters of the solar corona from 1991 to 2016 | The global structure of the solar corona observed in the optical window is governed by the global magnetic field with different characteristics over a solar activity cycle. The Ludendorff flattening index has become a popular measure of global structure of the solar corona as observed during an eclipse. In this study, ... | [
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] | 3 | [
"10.1088/1674-4527/16/12/181",
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] | [
"Priyatikanto, Rhorom"
] | [
"Astronomy Program, Faculty of Mathematics and Natural Sciences, Institut Teknologi Bandung, Bandung 40132, Indonesia; Space Science Center, National Institute of Aeronautics and Space, Bandung 40173, Indonesia"
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12408803 | 1607.01329 | Plasma Sloshing in Pulse-heated Solar and Stellar Coronal Loops | There is evidence that coronal heating is highly intermittent, and flares are the high energy extreme. The properties of the heat pulses are difficult to constrain. Here, hydrodynamic loop modeling shows that several large amplitude oscillations (∼20% in density) are triggered in flare light curves if the duration of t... | [
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... | [
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] | 2 | [
"10.3847/2041-8205/826/2/L20",
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] | [
"Reale, F."
] | [
"Dipartimento di Fisica & Chimica, Università di Palermo, Piazza del Parlamento 1, I-90134 Palermo, Italy"
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12620764 | 1607.08208 | Future CMB tests of dark matter: Ultralight axions and massive neutrinos | Measurements of cosmic microwave background (CMB) anisotropies provide strong evidence for the existence of dark matter and dark energy. They can also test its composition, probing the energy density and particle mass of different dark-matter and dark-energy components. CMB data have already shown that ultralight axion... | [
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12594612 | 1607.03095 | Bayesian evidence for the prevalence of waterworlds | Should we expect most habitable planets to share the Earth's marbled appearance? For a planetary surface to boast extensive areas of both land and water, a delicate balance must be struck between the volume of water it retains and the capacity of its perturbations. These two quantities may show substantial variability ... | [
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12500418 | 1607.01090 | Parallax of a Mira variable R Ursae Majoris studied with astrometric VLBI | We have measured an annual parallax of the Mira variable R Ursae Majoris (R UMa) with the VLBI Exploration for Radio Astronomy (VERA). From the monitoring VLBI observations over a span of about two years, we detected H<SUB>2</SUB>O maser spots in the LSR velocity range from 37 to 42 km s<SUP>-1</SUP>. We derived an ann... | [
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12473101 | 1607.08178 | Modelling the cross-spectral variability of the black hole binary MAXI J1659-152 with propagating accretion rate fluctuations | The power spectrum of the X-ray fluctuations of accreting black holes often consists of two broad humps. We quantitatively investigate the hypothesis that the lower frequency hump originates from variability in a truncated thin accretion disc, propagating into a large scaleheight inner hot flow which, in turn, itself i... | [
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"Rapisarda, S.",
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"Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, NL-1098XH Amsterdam, the Netherlands",
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