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12585936 | 1607.01803 | Multi-phase induced inflation in theories with non-minimal coupling to gravity | In this paper we investigate the induced inflation with two flat regions: one Starobinsky-like plateau in strong coupling regime and one shorter plateau around the saddle point of the Einstein frame potential. This multi-phase inflationary scenario can be used to solve problems of classical cosmology as well as the pro... | [
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-0.06322604417800903,... | 10.998425 | -0.770152 | 2016-07-01 | 12 | 2017JCAP...01..011A | [
"strong coupling regime",
"inflation",
"initial conditions",
"classical cosmology",
"problems",
"the α-attractors",
"Starobinsky",
"the Einstein frame potential",
"one shorter plateau",
"Einstein",
"the saddle-point plateau",
"arbitrarily low scale",
"the saddle point",
"one Starobinsky-li... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Theory"
] | 5 | [
"10.1088/1475-7516/2017/01/011",
"10.48550/arXiv.1607.01803"
] | [
"Artymowski, Michał",
"Lalak, Zygmunt",
"Lewicki, Marek"
] | [
"Institute of Physics, Jagiellonian University, Łojasiewicza 11, 30-348 Kraków, Poland",
"Institute of Theoretical Physics, Faculty of Physics, University of Warsaw ul. Hoża 69, 00-681 Warszawa, Poland",
"Institute of Theoretical Physics, Faculty of Physics, University of Warsaw ul. Hoża 69, 00-681 Warszawa, Po... | [
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12406950 | 1607.00943 | WISEP J060738.65+242953.4: A Nearby Pole-on L8 Brown Dwarf with Radio Emission | We present a simultaneous, multi-wavelength campaign targeting the nearby (7.2 pc) L8/L9 (optical/near-infrared) dwarf WISEP J060738.65+242953.4 in the mid-infrared, radio, and optical. Spitzer Space Telescope observations show no variability at the 0.2% level over 10 hr each in the 3.6 and 4.5 μm bands. Kepler K2 moni... | [
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... | 7.71574 | 12.716134 | 2016-07-01 | 12 | 2016AJ....152..123G | [
"various proposed radio emission scenarios",
"Non-simultaneous Gemini optical spectroscopy detects lithium",
"other brown dwarfs",
"stable periodic signals",
"radio",
"sin",
"variability",
"Campaign",
"I.",
"lack",
"amplitudes",
"periods",
"Balmer",
"The low measured projected rotation vel... | [
"brown dwarfs",
"solar neighborhood",
"stars: activity",
"stars: individual: WISEP J060738.65+242953.4",
"starspots",
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Earth and Planetary Astrophysics"
] | 3 | [
"10.3847/0004-6256/152/5/123",
"10.48550/arXiv.1607.00943"
] | [
"Gizis, John E.",
"Williams, Peter K. G.",
"Burgasser, Adam J.",
"Libralato, Mattia",
"Nardiello, Domenico",
"Piotto, Giampaolo",
"Bedin, Luigi R.",
"Berger, Edo",
"Paudel, Rishi"
] | [
"Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA",
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Center for Astrophysics and Space Science, University of California San Diego, La Jolla, CA 92093, USA",
"Dipartimento di Fisica e A... | [
"2016arXiv160903587C",
"2017ApJ...843..115R",
"2017ApJ...846...75P",
"2017MNRAS.469.1949L",
"2018haex.bookE.171W",
"2020ApJ...903...74R",
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5472549 | 1607.02494 | Optimal non-circular fiber geometries for image scrambling in high-resolution spectrographs | Optical fibers are a key component for high-resolution spectrographs to attain high precision in radial velocity measurements. We present a custom fiber with a novel core geometry - a 'D'-shape. From a theoretical standpoint, such a fiber should provide superior scrambling and modal noise mitigation, since unlike the c... | [
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"common polygonal fibers",
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"modal noise behaviour",
"chaotic scrambling",
"radial velocity measurements",
"superior scrambling and modal noise mitigation",
"high precision",
"the commonly used circular and polygonal fiber cross sections",
"a test fiber",
"a custom fibe... | [
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Astrophysics - Earth and Planetary Astrophysics"
] | 5 | [
"10.1117/12.2234552",
"10.48550/arXiv.1607.02494"
] | [
"Stürmer, Julian",
"Schwab, Christian",
"Grimm, Stephan",
"Kalide, André",
"Sutherland, Adam P.",
"Seifahrt, Andreas",
"Schuster, Kay",
"Bean, Jacob L.",
"Quirrenbach, Andreas"
] | [
"The Univ. of Chicago (United States)",
"Macquarie Univ. (Australia)",
"Leibniz-Institut für Photonische Technologien e.V. (Germany)",
"Leibniz-Institut für Photonische Technologien e.V. (Germany)",
"The Univ. of Chicago (United States)",
"The Univ. of Chicago (United States)",
"Leibniz-Institut für Pho... | [
"2017OExpr..2515549B",
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12408747 | 1607.00491 | First Observational Signature of Rotational Deceleration in a Massive, Intermediate-age Star Cluster in the Magellanic Clouds | While the extended main-sequence turnoffs (eMSTOs) found in almost all 1-2 Gyr old star clusters in the Magellanic Clouds are often explained by postulating extended star formation histories (SFHs), the tight subgiant branches (SGBs) seen in some clusters challenge this popular scenario. Puzzlingly, the SGB of the eMST... | [
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-0.0... | 9.28109 | 9.426627 | 2016-07-01 | 14 | 2016ApJ...826L..14W | [
"SGB",
"redder colors",
"extended star formation histories",
"stars",
"red giants",
"stellar ages",
"the blue SGB region",
"main-sequence turnoff stars",
"angular momentum",
"the eMSTO stars",
"rapidly rotating stars",
"the SGB",
"the eMSTO cluster",
"NGC",
"the red part",
"bluer",
"... | [
"galaxies: star clusters: individual: NGC 419",
"Hertzsprung–Russell and C–M diagrams",
"Magellanic Clouds",
"stars: rotation",
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 5 | [
"10.3847/2041-8205/826/1/L14",
"10.48550/arXiv.1607.00491"
] | [
"Wu, Xiaohan",
"Li, Chengyuan",
"de Grijs, Richard",
"Deng, Licai"
] | [
"School of Physics, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, China ; Kavli Institute for Astronomy & Astrophysics and Department of Astronomy, Peking University, Yi He Yuan Lu 5, Hai Dian District, Beijing 100871, China;",
"Kavli Institute for Astronomy & Astrophysics and Dep... | [
"2016RAA....16..179L",
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2745658 | 1607.02341 | WASP-113b and WASP-114b, two inflated hot Jupiters with contrasting densities | <BR /> Aims: We present the discovery and characterisation of the exoplanets WASP-113b and WASP-114b by the WASP surveys, SOPHIE and CORALIE. <BR /> Methods: The planetary nature of the systems was established by performing follow-up photometric and spectroscopic observations. The follow-up data were combined with the ... | [
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-0... | 6.336308 | 14.620687 | 2016-07-01 | 20 | 2016A&A...593A.113B | [
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"planets and satellites: detection",
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"Astrophysics - Earth and Planetary Astrophysics"
] | 12 | [
"10.1051/0004-6361/201526517",
"10.48550/arXiv.1607.02341"
] | [
"Barros, S. C. C.",
"Brown, D. J. A.",
"Hébrard, G.",
"Gómez Maqueo Chew, Y.",
"Anderson, D. R.",
"Boumis, P.",
"Delrez, L.",
"Hay, K. L.",
"Lam, K. W. F.",
"Llama, J.",
"Lendl, M.",
"McCormac, J.",
"Skiff, B.",
"Smalley, B.",
"Turner, O.",
"Vanhuysse, M.",
"Armstrong, D. J.",
"Boi... | [
"Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762, Porto, Portugal ; Aix-Marseille Université, CNRS, LAM (Laboratoire d'Astrophysique de Marseille) UMR 7326, 13388, Marseille, France",
"Department of Physics, University of Warwick, Gibbet Hill Road, Coventry, ... | [
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12470831 | 1607.02388 | Moving inhomogeneous envelopes of stars | Massive stars are extremely luminous and drive strong winds, blowing a large part of their matter into the galactic environment before they finally explode as a supernova. Quantitative knowledge of massive star feedback is required to understand our Universe as we see it. Traditionally, massive stars have been studied ... | [
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-0.... | 9.040446 | 10.903369 | 2016-07-01 | 4 | 2016JQSRT.183..100O | [
"stellar winds",
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"... | [
"Stars: mass-loss",
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"Astrophysics - Solar and Stellar Astrophysics"
] | 11 | [
"10.1016/j.jqsrt.2016.06.017",
"10.48550/arXiv.1607.02388"
] | [
"Oskinova, Lidia M.",
"Kubátová, Brankica",
"Hamann, Wolf-Rainer"
] | [
"Institute for Physics and Astronomy, University of Potsdam, 14476 Potsdam, Germany",
"Astronomický ústav AV ČR, Fričova 298, 251 65 Ondřejov, Czech Republic",
"Institute for Physics and Astronomy, University of Potsdam, 14476 Potsdam, Germany"
] | [
"2018A&A...620A..89N",
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12408800 | 1607.00344 | Today a Duo, but Once a Trio? The Double White Dwarf HS 2220+2146 May Be a Post-blue Straggler Binary | For sufficiently wide orbital separations a, the two members of a stellar binary evolve independently. This implies that in a wide double white dwarf (DWD), the more massive WD should always be produced first, when its more massive progenitor ends its main sequence (MS) life, and should therefore be older and cooler th... | [
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... | 6.007193 | 11.23483 | 2016-07-01 | 9 | 2016ApJ...828...38A | [
"other WD systems",
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"HS",
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"the WD p... | [
"binaries: visual",
"blue stragglers",
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"Astrophysics - Solar and Stellar Astrophysics"
] | 5 | [
"10.3847/0004-637X/828/1/38",
"10.48550/arXiv.1607.00344"
] | [
"Andrews, Jeff J.",
"Agüeros, Marcel",
"Brown, Warren R.",
"Gosnell, Natalie M.",
"Gianninas, A.",
"Kilic, Mukremin",
"Koester, Detlev"
] | [
"Foundation for Research and Technology-Hellas, 71110 Heraklion, Crete, Greece ; Columbia University, Department of Astronomy, 550 West 120th Street, New York, NY 10027, USA",
"Columbia University, Department of Astronomy, 550 West 120th Street, New York, NY 10027, USA",
"Smithsonian Astrophysical Observatory, ... | [
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12593841 | 1607.01562 | Modelling the thermal X-ray emission around the Galactic Centre from colliding Wolf-Rayet winds | The Galactic Centre is a hotbed of astrophysical activity, with the injection of wind material from ∼30 massive Wolf-Rayet (WR) stars orbiting within 12 arcsec of the supermassive black hole (SMBH) playing an important role. Hydrodynamic simulations of such colliding and accreting winds produce a complex density and te... | [
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-0.... | 8.188542 | 6.22221 | 2016-07-01 | 30 | 2017MNRAS.464.4958R | [
"WR winds",
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"SMBH feedback mechanisms",
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"Chandra X-ray",
"the thermal X-ray emission",
"the X-ray emission",
"stronger feedback",
"the X-ray flux",
"hot, X-ray-emitting gas",
"WR",
"the ... | [
"Galaxy: centre",
"stars: Wolf-Rayet",
"stars: winds",
"outflows",
"hydrodynamics",
"radiative transfer",
"X-rays: stars",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 8 | [
"10.1093/mnras/stw2584",
"10.48550/arXiv.1607.01562"
] | [
"Russell, Christopher M. P.",
"Wang, Q. Daniel",
"Cuadra, Jorge"
] | [
"X-ray Astrophysics Laboratory, Code 662, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA",
"Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA",
"Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, 782-0436 Santiago, Chile"
] | [
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3150910 | 1607.08733 | The ALMA Protostellar Interferometric Line Survey (PILS). First results from an unbiased submillimeter wavelength line survey of the Class 0 protostellar binary IRAS 16293-2422 with ALMA | Context. The inner regions of the envelopes surrounding young protostars are characterized by a complex chemistry, with prebiotic molecules present on the scales where protoplanetary disks eventually may form. The Atacama Large Millimeter/submillimeter Array (ALMA) provides an unprecedented view of these regions zoomin... | [
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... | 11.429715 | 11.907032 | 2016-07-01 | 315 | 2016A&A...595A.117J | [
"prebiotic molecules",
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"CO",
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"10.1051/0004-6361/201628648",
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"Jørgensen, J. K.",
"van der Wiel, M. H. D.",
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"Müller, H. S. P.",
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"Calcutt, H.",
"Bjerkeli, P.",
"Bourke, T. L.",
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"Favre, C.",
"Fayolle, E. C.",
"Garrod, R. T.",
"Jacobsen, S. K.",
"Öberg, K. I.",
"Persson, M.... | [
"Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen, Øster Voldgade 5-7, 1350, Copenhagen K., Denmark",
"Centre for Star and Planet Formation, Niels Bohr Institute & Natural History Museum of Denmark, University of Copenhagen, Øster Vol... | [
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12409034 | 1607.06518 | Star Formation Relations in the Milky Way | The relations between star formation and properties of molecular clouds (MCs) are studied based on a sample of star-forming regions in the Galactic Plane. Sources were selected by having radio recombination lines to provide identification of associated MCs and dense clumps. Radio continuum emission and mid-infrared emi... | [
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0.... | 11.59344 | 8.846237 | 2016-07-01 | 90 | 2016ApJ...831...73V | [
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"Vutisalchavakul, Nalin",
"Evans, Neal J., II",
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] | [
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12406381 | 1607.07458 | Brown dwarf disks with Herschel: Linking far-infrared and (sub)-mm fluxes | Brown dwarf disks are excellent laboratories to test our understanding of disk physics in an extreme parameter regime. In this paper we investigate a sample of 29 well-characterized brown dwarfs and very low-mass stars, for which Herschel far-infrared fluxes and (sub)-mm fluxes are available. We measured new Herschel/P... | [
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0.0... | 9.106122 | 12.516197 | 2016-07-01 | 22 | 2016A&A...594A..83D | [
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"10.1051/0004-6361/201628431",
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"Daemgen, Sebastian",
"Natta, Antonella",
"Scholz, Alexander",
"Testi, Leonardo",
"Jayawardhana, Ray",
"Greaves, Jane",
"Eastwood, Daniel"
] | [
"ETH Zürich, Institut für Astronomie, Wolfgang-Pauli-Strasse 27, 8093, Zürich, Switzerland ; Department of Astronomy & Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON, M5H 3H4, Canada",
"INAF/Osservatorio Astrofisico of Arcetri, Largo E. Fermi, 5, 50125, Firenze, Italy; School of Cosmic... | [
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12516962 | 1607.07399 | Design and development of an ambient-temperature continuously-rotating achromatic half-wave plate for CMB polarization modulation on the POLARBEAR-2 experiment | We describe the development of an ambient-temperature continuously-rotating half-wave plate (HWP) for study of the Cosmic Microwave Background (CMB) polarization by the POLARBEAR-2 (PB2) experiment. Rapid polarization modulation suppresses 1/f noise due to unpolarized atmospheric turbulence and improves sensitivity to ... | [
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... | [
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"10.1117/12.2232280",
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"Matsuda, Frederick",
"Plambeck, Richard",
"Suzuki, Aritoki",
"Takakura, Satoru"
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"Univ. of California, Berkeley (United States)",
"Univ. of California, Berkeley (United States)",
"Univ. of California, Berkeley (United States)",
"Univ. of California, Berkeley (United States)",
"Kavli Institute for The Physics and Mathematics of The Universe, The Univ. of Tokyo (Japan)",
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12473518 | 1607.05449 | The circumstellar disc of FS Tau B - a self-consistent model based on observations in the mid-infrared with NACO | Protoplanetary discs are a byproduct of the star formation process. In the dense mid-plane of these discs, planetesimals and planets are expected to form. The first step in planet formation is the growth of dust particles from submicrometre-sized grains to macroscopic mm-sized aggregates. The grain growth is accompanie... | [
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] | 8 | [
"10.1093/mnras/stw1692",
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] | [
"Kirchschlager, Florian",
"Wolf, Sebastian",
"Madlener, David"
] | [
"Institute of Theoretical Physics and Astrophysics, Kiel University, Leibnizstraße 15, D-24118 Kiel, Germany",
"Institute of Theoretical Physics and Astrophysics, Kiel University, Leibnizstraße 15, D-24118 Kiel, Germany",
"Max Planck Institute for Radio Astronomy, Auf dem Hügel 69, D-53121 Bonn, Germany"
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12593541 | 1607.07166 | Lyman α radiation hydrodynamics of galactic winds before cosmic reionization | The dynamical impact of Lyman α (Lyα) radiation pressure on galaxy formation depends on the rate and duration of momentum transfer between Lyα photons and neutral hydrogen gas. Although photon trapping has the potential to multiply the effective force, ionizing radiation from stellar sources may relieve the Lyα pressur... | [
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... | 13.618917 | 6.39726 | 2016-07-01 | 37 | 2017MNRAS.464.2963S | [
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] | 4 | [
"10.1093/mnras/stw2591",
"10.48550/arXiv.1607.07166"
] | [
"Smith, Aaron",
"Bromm, Volker",
"Loeb, Abraham"
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"Department of Astronomy, The University of Texas at Austin, Austin, TX 78712, USA",
"Department of Astronomy, The University of Texas at Austin, Austin, TX 78712, USA",
"Department of Astronomy, Harvard University, 60 Garden Street, Cambridge, MA 02138, USA"
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12409336 | 1607.02119 | Strong-lensing Analysis of the Powerful Lensing Cluster MACS J2135.2-0102 (z = 0.33) | We present a light-traces-mass (LTM) strong-lensing model of the massive lensing cluster MACS J2135.2-0102 (z = 0.33 hereafter MACS2135), known in part for hosting the cosmic eye galaxy lens. MACS2135 is also known to multiply lens a z = 2.3 sub-millimeter galaxy near the brightest cluster galaxy (BCG), as well as a pr... | [
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"dark matter",
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] | 4 | [
"10.3847/0004-637X/833/1/25",
"10.48550/arXiv.1607.02119"
] | [
"Zitrin, Adi",
"Broadhurst, Tom"
] | [
"Cahill Center for Astronomy and Astrophysics, California Institute of Technology, MC 249-17, Pasadena, CA 91125, USA ; Physics Department, Ben-Gurion University of the Negev, P.O. Box 653, Be'er-Sheva 84105, Israel ;;",
"Department of Theoretical Physics, University of Basque Country UPV/EHU, Bilbao, Spain ; IKE... | [
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12458756 | 1607.04185 | X-ray variability of SS 433: Evidence for supercritical accretion | We study the X-ray variability of SS 433 based on data from the ASCA observatory and the MAXI and RXTE/ASM monitoring missions. Based on the ASCA data, we have constructed the power spectrum of SS 433 in the frequency range from 10<SUP>-6</SUP> to 0.1 Hz, which confirms the presence of a flat portion in the spectrum at... | [
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0... | 6.718875 | 7.459055 | 2016-07-01 | 8 | 2016AstL...42..517A | [
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"SS 433",
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] | 4 | [
"10.1134/S106377371607001X",
"10.48550/arXiv.1607.04185"
] | [
"Atapin, K. E.",
"Fabrika, S. N."
] | [
"Sternberg Astronomical Institute, Moscow State University, Moscow, Russia; Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Karachai-Cherkessian Republic, Russia",
"Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, Karachai-Cherkessian Republic, Russia... | [
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3831799 | 1607.03059 | Saturation of the f -mode instability in neutron stars. II. Applications and results | We present the first results on the saturation of the f -mode instability in neutron stars due to nonlinear mode coupling. Emission of gravitational waves drives the f -mode (fundamental mode) unstable in fast-rotating, newborn neutron stars. The initial growth phase of the mode is followed by its saturation, because o... | [
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0.... | 5.47471 | 2.489076 | 2016-07-01 | 8 | 2016PhRvD..94b4053P | [
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"(un... | [
"Astrophysics - High Energy Astrophysical Phenomena",
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] | 7 | [
"10.1103/PhysRevD.94.024053",
"10.48550/arXiv.1607.03059"
] | [
"Pnigouras, Pantelis",
"Kokkotas, Kostas D."
] | [
"Theoretical Astrophysics, IAAT, Eberhard-Karls University of Tübingen, 72076 Tübingen, Germany",
"Theoretical Astrophysics, IAAT, Eberhard-Karls University of Tübingen, 72076 Tübingen, Germany"
] | [
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12619061 | 1607.06998 | Spectrum of shear modes in the neutron-star crust: Estimating the nuclear-physics uncertainties | I construct a model of the inner crust of neutron stars using interactions from chiral effective field theory (EFT) in order to calculate its equation of state (EOS), shear properties, and the spectrum of crustal shear modes. I systematically study uncertainties associated with the nuclear physics input, the crust comp... | [
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... | 4.820969 | 2.523389 | 2016-07-01 | 39 | 2017PhRvC..95a5803T | [
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] | 4 | [
"10.1103/PhysRevC.95.015803",
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] | [
"Tews, I."
] | [
"Institute for Nuclear Theory, University of Washington, Seattle, Washington 98195-1550, USA"
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12408861 | 1607.03090 | Effects of Proxima Centauri on Planet Formation in Alpha Centauri | Proxima Centauri is an M dwarf approximately 15,000 au from the Alpha Centauri binary, comoving and likely in a loosely bound orbit. Dynamic simulations show that this configuration can form from a more tightly bound triple system. As our nearest neighbors, these stars command great interest as potential planet hosts, ... | [
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] | 6 | [
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"Worth, R.",
"Sigurdsson, S."
] | [
"Center for Exoplanets and Habitable Worlds, The Astronomy & Astrophysics Department, Pennsylvania State University, University Park, PA 16802, USA",
"Center for Exoplanets and Habitable Worlds, The Astronomy & Astrophysics Department, Pennsylvania State University, University Park, PA 16802, USA"
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16261671 | 1607.07881 | Galaxy Quenching from Cosmic Web Detachment | We propose the Cosmic Web Detachment (CWD) model, a framework to interpret the star-formation history of galaxies in a cosmological context. The CWD model unifies several starvation mechanisms known to disrupt or stop star formation into one single physical framework. Galaxies begin accreting star-forming gas at early ... | [
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"Aragon Calvo, Miguel A.",
"Neyrinck, Mark C.",
"Silk, Joseph"
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"-",
"-",
"-"
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12407490 | 1607.02213 | Downward Catastrophe of Solar Magnetic Flux Ropes | 2.5-dimensional time-dependent ideal magnetohydrodynamic (MHD) models in Cartesian coordinates were used in previous studies to seek MHD equilibria involving a magnetic flux rope embedded in a bipolar, partially open background field. As demonstrated by these studies, the equilibrium solutions of the system are separat... | [
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... | 12.881807 | 16.182045 | 2016-07-01 | 9 | 2016ApJ...825..109Z | [
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"10.3847/0004-637X/825/2/109",
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] | [
"Zhang, Quanhao",
"Wang, Yuming",
"Hu, Youqiu",
"Liu, Rui"
] | [
"CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026, China ; Mengcheng National Geophysical Observatory, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China;",
"... | [
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1297853 | 1607.01026 | Beyond Kaiser bias: mildly non-linear two-point statistics of densities in distant spheres | We present simple parameter-free analytic bias functions for the two-point correlation of densities in spheres at large separation. These bias functions generalize the so-called Kaiser bias to the mildly non-linear regime for arbitrary density contrasts and grow as b(ρ) - b(1) ∝ (1 - ρ<SUP>-13/21</SUP>)ρ<SUP>1 + n/3</S... | [
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0.... | 11.907189 | 2.985671 | 2016-07-01 | 15 | 2017MNRAS.466.2067U | [
"correlations",
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"methods: analytical",
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] | 2 | [
"10.1093/mnras/stw3221",
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"Uhlemann, C.",
"Codis, S.",
"Kim, J.",
"Pichon, C.",
"Bernardeau, F.",
"Pogosyan, D.",
"Park, C.",
"L'Huillier, B."
] | [
"Institute for Theoretical Physics, Utrecht University, Princetonplein 5, NL-3584 CC Utrecht, the Netherlands",
"Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8, Canada",
"Korea Institute for Advanced Study (KIAS), 85 Hoegiro, Dongdaemun-gu, Seou... | [
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12436674 | 1607.08088 | Correspondence of Many-flavor Limit and Kaluza-Klein Degrees of Freedom in the Description of Compact Stars | We present the correspondence between non-interacting multi-hadron fermion star equation of state in the many-flavor limit and the degrees of freedom of a Kaluza\,--\,Klein compact star. Many flavors can be interpreted in this framework as one extra compacti\-fied spatial dimension with various, more-and-more massive h... | [
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... | 4.989673 | 1.852158 | 2016-07-01 | 0 | 2016arXiv160708088K | [
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"High Energy Physics - Phenomenology",
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] | 4 | [
"10.48550/arXiv.1607.08088"
] | [
"Karsai, Szilvia",
"Gábor Barnaföldi, Gergely",
"Forgács-Dajka, Emese",
"Pósfay, Péter"
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"-",
"-",
"-"
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12473512 | 1607.01483 | Galaxy growth from redshift 5 to 0 at fixed comoving number density | Studying the average properties of galaxies at a fixed comoving number density over a wide redshift range has become a popular observational method, because it may trace the evolution of galaxies statistically. We test this method by comparing the evolution of galaxies at fixed number density and by following individua... | [
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"low redshift galaxies",
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] | 7 | [
"10.1093/mnras/stw1690",
"10.48550/arXiv.1607.01483"
] | [
"van de Voort, Freeke"
] | [
"Department of Astronomy and Theoretical Astrophysics Center, University of California, Berkeley, CA 94720-3411, USA; Academia Sinica Institute of Astronomy and Astrophysics, PO Box 23-141, Taipei 10617, Taiwan"
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4175893 | 1607.01998 | On the ages of resonant, eroded and fossil asteroid families | In this work we have estimated 10 collisional ages of 9 families for which for different reasons our previous attempts failed. In general, these are difficult cases that required dedicated effort, such as a new family classifications for asteroids in mean motion resonances, in particular the 1/1 and 2/1 with Jupiter, a... | [
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"family membership",
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"a ... | [
"Asteroids",
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] | 12 | [
"10.1016/j.icarus.2016.12.030",
"10.48550/arXiv.1607.01998"
] | [
"Milani, Andrea",
"Knežević, Zoran",
"Spoto, Federica",
"Cellino, Alberto",
"Novaković, Bojan",
"Tsirvoulis, Georgios"
] | [
"Dipartimento di Matematica, Università di Pisa, Largo Pontecorvo 5, Pisa 56127, Italy",
"Serbian Academy of Sciences and Arts, Knez Mihailova 35, Belgrade 11000, Serbia",
"Laboratoire Lagrange, Universitè Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, France",
"INAF-Osservatorio Astrofisico di Torino, 10... | [
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3778370 | 1607.03486 | Simulating galaxy formation with black hole driven thermal and kinetic feedback | The inefficiency of star formation in massive elliptical galaxies is widely believed to be caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas. Achieving a sufficiently rapid reddening of moderately massive galaxies without expelling too many baryons has however proven difficult for ... | [
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"massive elliptical galaxies",
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"black hole growth histories",
"supermassive black holes",
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"black hole physics",
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"Astrophysics - Astrophysics of Galaxies"
] | 108 | [
"10.1093/mnras/stw2944",
"10.48550/arXiv.1607.03486"
] | [
"Weinberger, Rainer",
"Springel, Volker",
"Hernquist, Lars",
"Pillepich, Annalisa",
"Marinacci, Federico",
"Pakmor, Rüdiger",
"Nelson, Dylan",
"Genel, Shy",
"Vogelsberger, Mark",
"Naiman, Jill",
"Torrey, Paul"
] | [
"Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany",
"Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany; Zentrum für Astronomie der Universität Heidelberg, ARI, Mönchhofstr. 12-14, D-69120 Heidelberg, Germany",... | [
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1497674 | 1607.03679 | The role of gas infall in the evolution of disc galaxies | Spiral galaxies are thought to acquire their gas through a protracted infall phase resulting in the inside-out growth of their associated discs. For field spirals, this infall occurs in the lower density environments of the cosmic web. The overall infall rate, as well as the galactocentric radius at which this infall i... | [
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"Mollá, Mercedes",
"Díaz, Ángeles I.",
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"Departamento de Investigación Básica, CIEMAT, Avda. Complutense 40, E-28040 Madrid, Spain",
"Universidad Autónoma de Madrid, E-28049 Madrid, Spain; Astro-UAM, Unidad Asociada CSIC, Universidad Autónoma de Madrid, E-28049 Madrid, Spain",
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12584581 | 1607.00883 | Gravitational waves from the phase transition of a nonlinearly realized electroweak gauge symmetry | Within the Standard Model with nonlinearly realized electroweak symmetry, the LHC Higgs boson may reside in a singlet representation of the gauge group. Several new interactions are then allowed, including anomalous Higgs self-couplings, which may drive the electroweak phase transition to be strongly first-order. In th... | [
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12409228 | 1607.07692 | On Understanding the Nature of Collisions of Coronal Mass Ejections Observed by STEREO | We attempt to understand the collision characteristics of two coronal mass ejections (CMEs) launched successively from the Sun on 2013 October 25. The estimated kinematics, from three-dimensional (3D) reconstruction techniques applied to observations of CMEs by the SECCHI/Coronagraphic (COR) and Heliospheric Imagers, r... | [
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"Srivastava, Nandita"
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12516673 | 1607.07001 | First Simultaneous Views of the Axial and Lateral Perspectives of a Coronal Mass Ejection | The different appearances exhibited by coronal mass ejections (CMEs) are believed to be in part the result of different orientations of their main axis of symmetry, consistent with a flux-rope configuration. There are observational reports of CMEs seen along their main axis (axial perspective) and perpendicular to it (... | [
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"Cabello, I.",
"Cremades, H.",
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"Facultad Regional Mendoza, Universidad Tecnológica Nacional, Mendoza, Argentina; Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Buenos Aires, Argentina; Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Buenos Aires, Argentina",
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12511041 | 1607.05232 | Multitracing anisotropic non-Gaussianity with galaxy shapes | Correlations between intrinsic galaxy shapes on large scales arise due to the effect of the tidal field of the large-scale structure. Anisotropic primordial non-Gaussianity induces a distinct scale-dependent imprint in these tidal alignments on large scales. Motivated by the observational finding that the alignment str... | [
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] | 10 | [
"10.1103/PhysRevD.94.123507",
"10.48550/arXiv.1607.05232"
] | [
"Chisari, Nora Elisa",
"Dvorkin, Cora",
"Schmidt, Fabian",
"Spergel, David N."
] | [
"Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, United Kingdom",
"Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA",
"Max-Planck-Institute for Astrophysics, D-85748 Garching, Germany",
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12409123 | 1607.00692 | Three-Dimensional Simulations of Tearing and Intermittency in Coronal Jets | Observations of coronal jets increasingly suggest that local fragmentation and intermittency play an important role in the dynamics of these events. In this work, we investigate this fragmentation in high-resolution simulations of jets in the closed-field corona. We study two realizations of the embedded-bipole model, ... | [
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] | 9 | [
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"Wyper, P. F.",
"DeVore, C. R.",
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"Lynch, B. J."
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"Universities Space Research Association, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA",
"Heliophysics Science Division, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA",
"Heliophysics Science Division, NASA Goddard Space Flight Center, 8800 Gre... | [
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1171111 | 1607.03622 | Spatial Variations of PAH Properties in M17SW Revealed by Spitzer/IRS Spectral Mapping | We present Spitzer/IRS mid-infrared spectral maps of the Galactic star-forming region M17 as well as IRSF/SIRIUS Brγ and Nobeyama 45 m/FOREST <SUP>13</SUP>CO (J = 1-0) maps. The spectra show prominent features due to polycyclic aromatic hydrocarbons (PAHs) at wavelengths of 6.2, 7.7, 8.6, 11.3, 12.0, 12.7, 13.5, and 14... | [
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... | 12.394043 | 10.286899 | 2016-07-01 | 7 | 2016ApJ...833..163Y | [
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] | 5 | [
"10.3847/1538-4357/833/2/163",
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] | [
"Yamagishi, M.",
"Kaneda, H.",
"Ishihara, D.",
"Oyabu, S.",
"Suzuki, T.",
"Onaka, T.",
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"Umemoto, T.",
"Minamidani, T.",
"Nishimura, A.",
"Matsuo, M.",
"Fujita, S.",
"Tsuda, Y.",
"Kohno, M.",
"Ohashi, S."
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"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Chuo-ku, Sagamihara 252-5210, Japan",
"Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602, Japan",
"Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602, Japan",
... | [
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12408683 | 1607.06007 | Thermal Infrared Imaging and Atmospheric Modeling of VHS J125601.92-125723.9 b: Evidence for Moderately Thick Clouds and Equilibrium Carbon Chemistry in a Hierarchical Triple System | We present and analyze Subaru/IRCS L‧ and M‧ images of the nearby M dwarf VHS J125601.92-125723.9 (VHS 1256), which was recently claimed to have an ∼11 M <SUB> J </SUB> companion (VHS 1256 b) at ∼102 au separation. Our adaptive optics images partially resolve the central star into a binary, whose components are nearly ... | [
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... | [
"binaries: general",
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] | 7 | [
"10.3847/0004-637X/830/2/114",
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] | [
"Rich, Evan A.",
"Currie, Thayne",
"Wisniewski, John P.",
"Hashimoto, Jun",
"Brandt, Timothy D.",
"Carson, Joseph C.",
"Kuzuhara, Masayuki",
"Uyama, Taichi"
] | [
"Homer L. Dodge Department of Physics, University of Oklahoma, 440 W. Brooks St., Norman, OK 73071, USA",
"National Astronomical Observatory of Japan, Subaru Telescope, Hilo, HI, USA",
"Homer L. Dodge Department of Physics, University of Oklahoma, 440 W. Brooks St., Norman, OK 73071, USA",
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12620768 | 1607.01761 | Looking through the same lens: Shear calibration for LSST, Euclid, and WFIRST with stage 4 CMB lensing | The next-generation weak lensing surveys (i.e., LSST, Euclid, and WFIRST) will require exquisite control over systematic effects. In this paper, we address shear calibration and present the most realistic forecast to date for LSST/Euclid/WFIRST and CMB lensing from a stage 4 CMB experiment ("CMB S4"). We use the cosmol... | [
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... | 12.285607 | 3.416112 | 2016-07-01 | 75 | 2017PhRvD..95l3512S | [
"most tomographic bins",
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... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 17 | [
"10.1103/PhysRevD.95.123512",
"10.48550/arXiv.1607.01761"
] | [
"Schaan, Emmanuel",
"Krause, Elisabeth",
"Eifler, Tim",
"Doré, Olivier",
"Miyatake, Hironao",
"Rhodes, Jason",
"Spergel, David N."
] | [
"Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA",
"Stanford University, Stanford, California 94305, USA",
"California Institute of Technology, Pasadena, California 91109, USA; California Institute of Technology, Pasadena, California 91125, USA",
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1376451 | 1607.06970 | OSSOS. IV. Discovery of a Dwarf Planet Candidate in the 9:2 Resonance with Neptune | We report the discovery and orbit of a new dwarf planet candidate, 2015 RR<SUB>245</SUB>, by the Outer Solar System Origins Survey (OSSOS). The orbit of 2015 RR<SUB>245</SUB> is eccentric (e = 0.586), with a semimajor axis near 82 au, yielding a perihelion distance of 34 au. 2015 RR<SUB>245</SUB> has g-r=0.59+/- 0.11 a... | [
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"Kuiper belt objects: individual: 2015 RR245",
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] | 19 | [
"10.3847/0004-6256/152/6/212",
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"Bannister, Michele T.",
"Alexandersen, Mike",
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"Delsanti, Audrey",
"Fraser, Wesley C.",
"Gladman, Brett J.",
"Granvik, Mikael",
"Grundy, Will M.",
"Guilbert-Lepoutre, Aurélie",
"Gwyn, Stephen D. J.",
"Ip, Wing-Huen",
"Jakubik, Marian",
"Jones, R. Ly... | [
"Department of Physics and Astronomy, University of Victoria, Elliott Building, 3800 Finnerty Road, Victoria, BC V8P 5C2, Canada ; Astrophysics Research Centre, Queen's University Belfast, Belfast BT7 1NN, UK ; NRC-Herzberg Astronomy and Astrophysics, National Research Council of Canada, 5071 West Saanich Road, Vic... | [
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12434019 | 1607.00147 | HERA Mock Observations: Looking for Closure HERA Memorandum Number 13 | We investigate the use of closure phase as a method to detect the HI 21cm signal from the neutral IGM during cosmic reionzation. Closure quantities have the unique advantage of being independent of antenna-based calibration terms. We employ realistic, large area sky models from Sims et al. (2016). These include an esti... | [
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0.00... | 12.649944 | 3.303118 | 2016-07-01 | 1 | 2016arXiv160700147C | [
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"Astrophysics - Instrumentation and Methods for Astrophysics",
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"10.48550/arXiv.1607.00147"
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"Carilli, C. L.",
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"-",
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5393954 | 1607.05886 | Constraints on Ultrahigh-Energy Cosmic-Ray Sources from a Search for Neutrinos above 10 PeV with IceCube | We report constraints on the sources of ultrahigh-energy cosmic rays (UHECRs) above 1 0<SUP>9</SUP> GeV , based on an analysis of seven years of IceCube data. This analysis efficiently selects very high- energy neutrino-induced events which have deposited energies from 5 ×1 0<SUP>5</SUP> GeV to above 1 0<SUP>11</SUP> G... | [
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-0... | 5.826675 | -0.294728 | 2016-07-01 | 147 | 2016PhRvL.117x1101A | [
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"Astrophysics - High Energy Astrophysical Phenomena",
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] | 17 | [
"10.1103/PhysRevLett.117.241101",
"10.48550/arXiv.1607.05886"
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"Aartsen, M. G.",
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"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",
"Department of Physics and Astronomy, University of Canterbury, Private Bag 4800 Christchurch, New Zealand",
"Universit... | [
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4158672 | 1607.05248 | Two Small Planets Transiting HD 3167 | We report the discovery of two super-Earth-sized planets transiting the bright (V = 8.94, K = 7.07) nearby late G-dwarf HD 3167, using data collected by the K2 mission. The inner planet, HD 3167 b, has a radius of 1.6 R <SUB>⊕</SUB> and an ultra-short orbital period of only 0.96 days. The outer planet, HD 3167 c, has a... | [
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"multiple transiting planets",
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"planetary systems",
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"Astrophysics - Earth and Planetary Astrophysics",
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] | 13 | [
"10.3847/2041-8205/829/1/L9",
"10.48550/arXiv.1607.05248"
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"Vanderburg, Andrew",
"Bieryla, Allyson",
"Duev, Dmitry A.",
"Jensen-Clem, Rebecca",
"Latham, David W.",
"Mayo, Andrew W.",
"Baranec, Christoph",
"Berlind, Perry",
"Kulkarni, Shrinivas",
"Law, Nicholas M.",
"Nieberding, Megan N.",
"Riddle, Reed",
"Salama, Maïssa"
] | [
"Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA ;;",
"Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"California Institute of Technology, Pasadena, CA 91125, USA",
"California Institute of Technology, Pasadena, CA 91125, USA",... | [
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12409019 | 1607.05281 | Sizing Up the Milky Way: A Bayesian Mixture Model Meta-analysis of Photometric Scale Length Measurements | The exponential scale length (L <SUB> d </SUB>) of the Milky Way’s (MW’s) disk is a critical parameter for describing the global physical size of our Galaxy, important both for interpreting other Galactic measurements and helping us to understand how our Galaxy fits into extragalactic contexts. Unfortunately, current e... | [
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0.00219... | 9.981111 | 6.754095 | 2016-07-01 | 21 | 2016ApJ...831...71L | [
"other Galactic measurements",
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"Galaxy: disk",
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] | 9 | [
"10.3847/0004-637X/831/1/71",
"10.48550/arXiv.1607.05281"
] | [
"Licquia, Timothy C.",
"Newman, Jeffrey A."
] | [
"Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260, USA ; Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT PACC), Pittsburgh, PA 15260, USA;",
"Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, ... | [
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12435945 | 1607.05762 | The Effect of Nearby Voids on Galaxy Number Counts | The size, shape and degree of emptiness of void interiors sheds light on the details of galaxy formation. A particularly interesting question is whether void interiors are completely empty or contain a dwarf population. However the nearby voids that are most conducive for dwarf searches have large angular diameters, on... | [
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"Astrophysics - Instrumentation and Methods for Astrophysics",
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] | 5 | [
"10.48550/arXiv.1607.05762"
] | [
"Bucklein, Brian K.",
"Moody, J. Ward",
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12581754 | 1607.00237 | Bell violation in the sky | In this work, we have studied the possibility of setting up Bell's inequality violating experiment in the context of cosmology, based on the basic principles of quantum mechanics. First we start with the physical motivation of implementing the Bell inequality violation in the context of cosmology. Then to set up the co... | [
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"string theory motivated axion monodromy model",
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"High Energy Physics - Theory",
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"10.1140/epjc/s10052-016-4553-3",
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] | [
"Choudhury, Sayantan",
"Panda, Sudhakar",
"Singh, Rajeev"
] | [
"Department of Theoretical Physics, Tata Institute of Fundamental Research, Mumbai, India; DTP, TIFR, Mumbai, India",
"Institute of Physics, Bhubaneswar, Odisha, India; Homi Bhabha National Institute, Mumbai, India",
"Department of Physics, Savitribai Phule Pune University, Pune, India"
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12466240 | 1607.03002 | Rates, flux densities, and spectral indices of meteor radio afterglows | Using the narrowband all-sky imager mode of the Long Wavelength Array (LWA1), we have now detected 30 transients at 25.6 MHz, 1 at 34 MHz, and 93 at 38.0 MHz. While we have only optically confirmed that 37 of these events are radio afterglows from meteors, evidence suggests that most, if not all, are. Using the beam-fo... | [
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"radio afterglows",
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"meteors",
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] | 0 | [
"10.1002/2016JA022606",
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"Obenberger, K. S.",
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"Hancock, P. J.",
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"Pedersen, T. R.",
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] | [
"Space Vehicles Directorate, Air Force Research Laboratory, Kirtland AFB, New Mexico USA",
"University of New Mexico, Albuquerque, New Mexico USA",
"International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia Australia",
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12435475 | 1607.03658 | X-ray emission from single Wolf-Rayet stars | This review briefly summarizes our knowledge of the X-ray emission from single WN, WC, and WO stars. These stars have relatively modest X-ray luminosities, typically not exceeding L_sun. The analysis of X-ray spectra usually reveals thermal plasma with temperatures reaching a few 10 MK. X-ray variability is detected in... | [
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941376 | 1607.06282 | Simulating the impact of X-ray heating during the cosmic dawn | Upcoming observations of the 21-cm signal from the epoch of reionization will soon provide the first direct detection of this era. This signal is influenced by many astrophysical effects, including long-range X-ray heating of the intergalactic gas. During the preceding cosmic dawn era, the impact of this heating on the... | [
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"Ross, Hannah E.",
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"Iliev, Ilian T.",
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"Astronomy Centre, Department of Physics and Astronomy, Pevensey III Building, University of Sussex, Falmer, Brighton BN1 9QH, UK; Department of Astronomy and Oskar Klein Centre, AlbaNova, Stockholm University, SE-106 91 Stockholm, Sweden",
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2774738 | 1607.03144 | The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: angular clustering tomography and its cosmological implications | We investigate the cosmological implications of studying galaxy clustering using a tomographic approach applied to the final Baryon Oscillation Spectroscopic Survey (BOSS) DR12 galaxy sample, including both auto- and cross-correlation functions between redshift shells. We model the signal of the full shape of the angul... | [
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"Chuang, Chia-Hsun",
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"Olmstead, Matthew D.",
"Percival, Will J.",
"Prada, Francisco",
"Rodríg... | [
"Universitäts-Sternwarte München, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, D-81679 Munich, Germany; Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, Giessenbachstr, D-85741 Garching, Germany",
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12435249 | 1607.04552 | Optimal Orderings of k-subsets for Star Identification | Finding the optimal ordering of k-subsets with respect to an objective function is known to be an extremely challenging problem. In this paper we introduce a new objective for this task, rooted in the problem of star identification on spacecrafts: subsets of detected spikes are to be generated in an ordering that minim... | [
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"Mueller, Joerg H.",
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12408486 | 1607.08060 | Reverberation Mapping of the Broad-line Region in NGC 5548: Evidence for Radiation Pressure? | NGC 5548 is the best-observed reverberation-mapped active galactic nucleus with long-term, intensive monitoring. Here we report results from a new observational campaign between 2015 January and July. We measure the centroid time lag of the broad Hβ emission line with respect to the 5100 Å continuum and obtain {τ }<SUB... | [
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"Department of Astronomy, Beijing Normal University, Beijing 100875, China ; Key Laboratory for Particle Astrophysics, Institute of High Energy Physics,Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China;",
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3811176 | 1607.01188 | Machine-learning identification of galaxies in the WISE × SuperCOSMOS all-sky catalogue | Context. The two currently largest all-sky photometric datasets, WISE and SuperCOSMOS, have been recently cross-matched to construct a novel photometric redshift catalogue on 70% of the sky. Galaxies were separated from stars and quasars through colour cuts, which may leave imperfections because different source types ... | [
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"Krakowski, T.",
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"National Centre for Nuclear Research, ul. Andrzeja Sołtana 7, 05-400, Otwock, Poland",
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12620975 | 1607.06858 | New observational limits on dark radiation in braneworld cosmology | A dark radiation term arises as a correction to the energy-momentum tensor in the simplest five-dimensional RS-II brane-world cosmology. In this paper we revisit the constraints on dark radiation based upon the newest results for light element nuclear reaction rates, observed light element abundances, and the power spe... | [
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"10.1103/PhysRevD.95.083516",
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"Sasankan, Nishanth",
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12593704 | 1607.01964 | Evolution of an accretion disc in binary black hole systems | We investigate evolution of an accretion disc in binary black hole (BBH) systems and possible electromagnetic counterparts of the gravitational waves from mergers of BBHs. Perna et al. proposed a novel evolutionary scenario of an accretion disc in BBHs in which a disc eventually becomes 'dead', I.e. the magnetorotation... | [
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"Kimura, Shigeo S.",
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"Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Sendai 980-8578, Japan; Astronomical Institute, Tohoku University, Sendai 980-8578, Japan; Center for Particle and Gravitational Astrophysics, Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA ... | [
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12464606 | 1607.01363 | Angular dependence of primordial trispectra and CMB spectral distortions | Under the presence of anisotropic sources in the inflationary era, the trispectrum of the primordial curvature perturbation has a very specific angular dependence between each wavevector that is distinguishable from the one encountered when only scalar fields are present, characterized by an angular dependence describe... | [
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"10.1088/1475-7516/2016/10/015",
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"Shiraishi, Maresuke",
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"Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), UTIAS, The University of Tokyo, Chiba, 277-8583, Japan",
"Dipartimento di Fisica e Astronomia ``G. Galilei'', Università degli Studi di Padova, via Marzolo 8, I-35131, Padova, Italy ; INFN, Sezione di Padova, via Marzolo 8, I-3513... | [
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12472669 | 1607.06296 | Cosmological tests with the FSRQ gamma-ray luminosity function | The extensive catalogue of gamma-ray selected flat-spectrum radio quasars (FSRQs) produced by Fermi during a four-year survey has generated considerable interest in determining their gamma-ray luminosity function (GLF) and its evolution with cosmic time. In this paper, we introduce the novel idea of using this extensiv... | [
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... | 15.1858 | 6.17011 | 2016-07-01 | 11 | 2016MNRAS.462.3094Z | [
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"10.1093/mnras/stw1817",
"10.48550/arXiv.1607.06296"
] | [
"Zeng, Houdun",
"Melia, Fulvio",
"Zhang, Li"
] | [
"Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China; Key Laboratory of Astroparticle Physics of Yunnan Province, Kunming 650091, China",
"Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China; Department of Physics, The Applied Math Program, and Department of... | [
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12409286 | 1607.04293 | Examining the Accuracy of Astrophysical Disk Simulations with a Generalized Hydrodynamical Test Problem | We discuss a generalization of the classic Keplerian disk test problem allowing for both pressure and rotational support, as a method of testing astrophysical codes incorporating both gravitation and hydrodynamics. We argue for the inclusion of pressure in rotating disk simulations on the grounds that realistic, astrop... | [
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0.03... | 9.122813 | 4.741177 | 2016-07-01 | 9 | 2016ApJ...831...26R | [
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"... | [
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] | 0 | [
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] | [
"Raskin, Cody",
"Owen, J. Michael"
] | [
"Lawrence Livermore National Laboratory, P.O. Box 808, L-038, Livermore, CA 94550, USA",
"Lawrence Livermore National Laboratory, P.O. Box 808, L-038, Livermore, CA 94550, USA"
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3386625 | 1607.01013 | Knot a Bad Idea: Testing BLISS Mapping for Spitzer Space Telescope Photometry | Much of transiting exoplanet science relies on high-precision photometry. The current generation of instruments can exhibit sensitivity variations greater than the astrophysical signals. For the InfraRed Array Camera (IRAC) on the Spitzer Space Telescope, a popular way to handle this is BiLinearly-Interpolated Subpixel... | [
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0.... | 6.952408 | 14.459582 | 2016-07-01 | 7 | 2017PASP..129a4001S | [
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] | 5 | [
"10.1088/1538-3873/129/971/014001",
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] | [
"Schwartz, J. C.",
"Cowan, N. B."
] | [
"Department of Physics & Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL, 60208, USA ; Department of Earth & Planetary Sciences, McGill University, 3450 rue University, Montreal, QC, H3A 0E8, Canada ; Department of Physics, McGill University, 3600 rue University, Montreal, QC, H3A 2T8, ... | [
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12521020 | 1607.05406 | Galaxy-Galaxy Weak-lensing Measurements from SDSS. I. Image Processing and Lensing Signals | We present our image processing pipeline that corrects the systematics introduced by the point-spread function (PSF). Using this pipeline, we processed Sloan Digital Sky Survey (SDSS) DR7 imaging data in r band and generated a galaxy catalog containing the shape information. Based on our shape measurements of the galax... | [
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... | 12.335458 | 3.716866 | 2016-07-01 | 20 | 2017ApJ...836...38L | [
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"... | [
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"10.3847/1538-4357/836/1/38",
"10.48550/arXiv.1607.05406"
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"Luo, Wentao",
"Yang, Xiaohu",
"Zhang, Jun",
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"Fu, Liping",
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"van den Bosch, Frank C.",
"Shu, Chenggang",
"Li, Ran",
"Li, Nan",
"Liu, Xiangkun",
"Pan, Chuzhong",
"Wang, Yiran",
"Radovich, Mario"
] | [
"Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Nandan Road 80, Shanghai 200030, China ; Center for Astronomy and Astrophysics, Shanghai Jiaotong University, Shanghai, 200240, China ; Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213, USA;",
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12587367 | 1607.00824 | Large-scale-vortex dynamos in planar rotating convection | Several recent studies have demonstrated how large-scale vortices may arise spontaneously in rotating planar convection. Here we examine the dynamo properties of such flows in rotating Boussinesq convection. For moderate values of the magnetic Reynolds number ($100 \lesssim Rm \lesssim 550$, with $Rm$ based on the box ... | [
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0.033... | 11.445432 | 14.326591 | 2016-07-01 | 13 | 2017JFM...815..333G | [
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"10.1017/jfm.2017.56",
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"Guervilly, Céline",
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1836135 | 1607.00015 | Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia | Recent improvements in the age dating of stellar populations and single stars allow us to study the ages and abundance of stars and galaxies with unprecedented accuracy. We here compare the relation between age and α-element abundances for stars in the solar neighborhood to that of local, early-type galaxies. We find t... | [
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"galaxies",
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"unprecedented accuracy",
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... | [
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"cD",
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] | 6 | [
"10.1051/0004-6361/201528019",
"10.48550/arXiv.1607.00015"
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"Walcher, C. J.",
"Yates, R. M.",
"Minchev, I.",
"Chiappini, C.",
"Bergemann, M.",
"Bruzual, G.",
"Charlot, S.",
"Coelho, P. R. T.",
"Gallazzi, A.",
"Martig, M."
] | [
"Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482, Potsdam, Germany",
"Max-Planck Institut für Extraterrestrische Physik, Giessenbachstraße 1, 85748, Garching, Germany; Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85748, Garching, Germany",
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12586099 | 1607.08609 | Cumulative effects in inflation with ultra-light entropy modes | In multi-field inflation one or more non-adiabatic modes may become light, potentially inducing large levels of isocurvature perturbations in the cosmic microwave background. If in addition these light modes are coupled to the adiabatic mode, they influence its evolution on super horizon scales. Here we consider the ca... | [
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0.... | 11.024451 | -0.681149 | 2016-07-01 | 57 | 2017JCAP...02..013A | [
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"the cosmic microwave background",
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] | 12 | [
"10.1088/1475-7516/2017/02/013",
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] | [
"Achúcarro, Ana",
"Atal, Vicente",
"Germani, Cristiano",
"Palma, Gonzalo A."
] | [
"Instituut-Lorentz for Theoretical Physics, Universiteit Leiden, 2333 CA Leiden, The Netherlands ; Department of Theoretical Physics, University of the Basque Country, 48080 Bilbao, Spain;",
"Instituut-Lorentz for Theoretical Physics, Universiteit Leiden, 2333 CA Leiden, The Netherlands",
"Institut de Ciéncies ... | [
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12408700 | 1607.07545 | Cosmic Shear Measurement Using Auto-convolved Images | We study the possibility of using quadrupole moments of auto-convolved galaxy images to measure cosmic shear. The autoconvolution of an image corresponds to the inverse Fourier transformation of its power spectrum. The new method has the following advantages: the smearing effect due to the point-spread function (PSF) c... | [
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... | 12.249169 | 3.43641 | 2016-07-01 | 4 | 2016ApJ...830..116L | [
"simulated galaxy images",
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"the auto-convol... | [
"large-scale structure of universe",
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] | 4 | [
"10.3847/0004-637X/830/2/116",
"10.48550/arXiv.1607.07545"
] | [
"Li, Xiangchong",
"Zhang, Jun"
] | [
"Center for Astronomy and Astrophysics, Department of Physics and Astronomy, Shanghai Jiao Tong University, 955 Jianchuan road, Shanghai, 200240, China",
"Center for Astronomy and Astrophysics, Department of Physics and Astronomy, Shanghai Jiao Tong University, 955 Jianchuan road, Shanghai, 200240, China"
] | [
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12470600 | 1607.01543 | A corrugated termination shock in pulsar wind nebulae? | Successful phenomenological models of pulsar wind nebulae assume efficient dissipation of the Poynting flux of the magnetized electron-positron wind as well as efficient acceleration of the pairs in the vicinity of the termination shock, but how this is realized is not yet well understood. This paper suggests that the ... | [
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0.011... | 5.481113 | 4.067772 | 2016-07-01 | 11 | 2016JPlPh..82d6301L | [
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] | 0 | [
"10.1017/S0022377816000659",
"10.48550/arXiv.1607.01543"
] | [
"Lemoine, Martin"
] | [
"Institut d'Astrophysique de Paris, CNRS - UPMC, 98 bis boulevard Arago, F-75014 Paris, France"
] | [
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2838379 | 1607.03293 | Two giant outbursts of V0332+53 observed with INTEGRAL | Context. In July 2015, the high-mass X-ray binary V0332+53 underwent a giant outburst, a decade after the previous one. V0332+53 hosts a strongly magnetized neutron star. During the 2004-2005 outburst, an anti-correlation between the centroid energy of its fundamental cyclotron resonance scattering features (CRSFs) and... | [
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"-",
"the X-ray luminosity",
"the Joint European X-ray Monitors",
"~330 ks",
"the high-mass X-ray binary V0332",
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"ks",
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"~330",
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"the fundame... | [
"stars: neutron",
"X-rays: binaries",
"pulsars: individual: V0332+53",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 4 | [
"10.1051/0004-6361/201628865",
"10.48550/arXiv.1607.03293"
] | [
"Ferrigno, Carlo",
"Ducci, Lorenzo",
"Bozzo, Enrico",
"Kretschmar, Peter",
"Kühnel, Matthias",
"Malacaria, Christian",
"Pottschmidt, Katja",
"Santangelo, Andrea",
"Savchenko, Volodymyr",
"Wilms, Jörn"
] | [
"ISDC, University of Geneva, chemin d'Écogia, 16 1290, Versoix, Switzerland",
"ISDC, University of Geneva, chemin d'Écogia, 16 1290, Versoix, Switzerland; Institut für Astronomie und Astrophysik, Kepler Center for Astro and Particle Physics, Eberhard Karls Universität, Sand 1, 72076, Tübingen, Germany",
"ISDC, ... | [
"2017A&A...606L..13S",
"2017MNRAS.466.2143D",
"2017MNRAS.470.2457D",
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2614419 | 1607.03636 | Sardinia Radio Telescope wide-band spectral-polarimetric observations of the galaxy cluster 3C 129 | We present new observations of the galaxy cluster 3C 129 obtained with the Sardinia Radio Telescope in the frequency range 6000-7200 MHz, with the aim to image the large-angular-scale emission at high-frequency of the radio sources located in this cluster of galaxies. The data were acquired using the recently commissio... | [
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"polarization",
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"radio continuum: galaxies",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 9 | [
"10.1093/mnras/stw1552",
"10.48550/arXiv.1607.03636"
] | [
"Murgia, M.",
"Govoni, F.",
"Carretti, E.",
"Melis, A.",
"Concu, R.",
"Trois, A.",
"Loi, F.",
"Vacca, V.",
"Tarchi, A.",
"Castangia, P.",
"Possenti, A.",
"Bocchinu, A.",
"Burgay, M.",
"Casu, S.",
"Pellizzoni, A.",
"Pisanu, T.",
"Poddighe, A.",
"Poppi, S.",
"D'Amico, N.",
"Bache... | [
"INAF-Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius (CA), Italy",
"INAF-Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius (CA), Italy",
"INAF-Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius (CA), Italy",
"INAF-Osservatorio ... | [
"2017A&A...600A..18K",
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12408712 | 1607.05683 | Magnetic Diagnostics of the Solar Chromosphere with the Mg II h-k Lines | We investigated the formation of the Mg II h-k doublet in a weakly magnetized atmosphere (20-100 G) using a newly developed numerical code for polarized radiative transfer in a plane-parallel geometry, which implements a recent formulation of partially coherent scattering by polarized multi-term atoms in arbitrary magn... | [
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"∼10 G",
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"the non-magnetic case",
"relatively small field strengths",
"a magnetic field",
"previous work",
"the classical magnetograph formula",
"the broadband linear pol... | [
"atomic processes",
"line: formation",
"polarization",
"Sun: magnetic fields",
"Astrophysics - Solar and Stellar Astrophysics"
] | 10 | [
"10.3847/2041-8205/830/2/L24",
"10.48550/arXiv.1607.05683"
] | [
"del Pino Alemán, T.",
"Casini, R.",
"Manso Sainz, R."
] | [
"High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000, USA ;",
"High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000, USA",
"Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, D-37077... | [
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12509751 | 1607.00290 | Implications of gamma-ray observations on proton models of ultrahigh energy cosmic rays | The origin of ultrahigh energy cosmic rays (UHECR) is still unknown. However, great progress has been achieved in past years due to the good quality and large statistics in experimental data collected by the current observatories. The data of the Pierre Auger Observatory show that the composition of UHECRs becomes prog... | [
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... | 5.942949 | 0.051518 | 2016-07-01 | 29 | 2016PhRvD..94f3002S | [
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"large statistics",
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"Astrophysics - High Energy Astrophysical Phenomena"
] | 3 | [
"10.1103/PhysRevD.94.063002",
"10.48550/arXiv.1607.00290"
] | [
"Supanitsky, A. D."
] | [
"Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), CC 67, Sucursal 28, C1428ZAA Buenos Aires, Argentina"
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12515367 | 1607.00897 | Pre-DECIGO can get the smoking gun to decide the astrophysical or cosmological origin of GW150914-like binary black holes | Pre-DECIGO (DECihertz laser Interferometer Gravitational wave Observatory) consists of three spacecraft arranged in an equilateral triangle with 100 km arm lengths orbiting 2000 km above the surface of the earth. It is hoped that the launch date will be in the late 2020s. <P />Pre-DECIGO has one clear target: binary bl... | [
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"earth",
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"the cu... | [
"E01",
"E02",
"E31",
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"Astrophysics - High Energy Astrophysical Phenomena",
"General Relativity and Quantum Cosmology"
] | 4 | [
"10.1093/ptep/ptw127",
"10.48550/arXiv.1607.00897"
] | [
"Nakamura, Takashi",
"Ando, Masaki",
"Kinugawa, Tomoya",
"Nakano, Hiroyuki",
"Eda, Kazunari",
"Sato, Shuichi",
"Musha, Mitsuru",
"Akutsu, Tomotada",
"Tanaka, Takahiro",
"Seto, Naoki",
"Kanda, Nobuyuki",
"Itoh, Yousuke"
] | [
"1Department of Physics, Kyoto University, Kyoto 606-8502, Japan",
"2Department of Physics, The University of Tokyo, Tokyo 113-0033, Japan; 3National Astronomical Observatory of Japan, Tokyo 181-8588, Japan; 4Institute for Cosmic Ray Research, The University of Tokyo, Chiba 277-8582, Japan",
"5Research Center f... | [
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1576892 | 1607.07190 | Oxygen abundance maps of CALIFA galaxies | We construct maps of the oxygen abundance distribution across the discs of 88 galaxies using Calar Alto Legacy Integral Field Area survey (CALIFA) Data Release 2 (DR2) spectra. The position of the centre of a galaxy (coordinates on the plate) was also taken from the CALIFA DR2. The galaxy inclination, the position angl... | [
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0.00458... | 11.194604 | 7.892041 | 2016-07-01 | 47 | 2016MNRAS.462.2715Z | [
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"ISM: abundances",
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"Astrophysics - Astrophysics of Galaxies"
] | 10 | [
"10.1093/mnras/stw1857",
"10.48550/arXiv.1607.07190"
] | [
"Zinchenko, I. A.",
"Pilyugin, L. S.",
"Grebel, E. K.",
"Sánchez, S. F.",
"Vílchez, J. M."
] | [
"Main Astronomical Observatory of National Academy of Sciences of Ukraine, 27 Zabolotnogo Str., 03680 Kiev, Ukraine; Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12-14, D-69120 Heidelberg, Germany",
"Main Astronomical Observatory of National Academy of Sciences o... | [
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12522503 | 1607.00409 | VULCAN: An Open-source, Validated Chemical Kinetics Python Code for Exoplanetary Atmospheres | We present an open-source and validated chemical kinetics code for studying hot exoplanetary atmospheres, which we name VULCAN. It is constructed for gaseous chemistry from 500 to 2500 K, using a reduced C-H-O chemical network with about 300 reactions. It uses eddy diffusion to mimic atmospheric dynamics and excludes p... | [
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... | 7.476991 | 14.593283 | 2016-07-01 | 122 | 2017ApJS..228...20T | [
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"methods: numerical",
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] | 31 | [
"10.3847/1538-4365/228/2/20",
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] | [
"Tsai, Shang-Min",
"Lyons, James R.",
"Grosheintz, Luc",
"Rimmer, Paul B.",
"Kitzmann, Daniel",
"Heng, Kevin"
] | [
"University of Bern, Center for Space and Habitability, Sidlerstrasse 5, CH-3012, Bern, Switzerland",
"Arizona State University, School of Earth and Space Exploration, Bateman Physical Sciences, Tempe, AZ 85287-1404, USA",
"University of Bern, Center for Space and Habitability, Sidlerstrasse 5, CH-3012, Bern, S... | [
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2826878 | 1607.00912 | High-resolution HI and CO observations of high-latitude intermediate-velocity clouds | Context. Intermediate-velocity clouds (IVCs) are HI halo clouds that are likely related to a Galactic fountain process. In-falling IVCs are candidates for the re-accretion of matter onto the Milky Way. <BR /> Aims: We study the evolution of IVCs at the disk-halo interface, focussing on the transition from atomic to mol... | [
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"instrumentation: high angular resolution",
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] | 6 | [
"10.1051/0004-6361/201526801",
"10.48550/arXiv.1607.00912"
] | [
"Röhser, T.",
"Kerp, J.",
"Ben Bekhti, N.",
"Winkel, B."
] | [
"Argelander-Institut für Astronomie (AIfA), Universität Bonn, Auf dem Hügel 71, 53121, Bonn, Germany",
"Argelander-Institut für Astronomie (AIfA), Universität Bonn, Auf dem Hügel 71, 53121, Bonn, Germany",
"Argelander-Institut für Astronomie (AIfA), Universität Bonn, Auf dem Hügel 71, 53121, Bonn, Germany",
"... | [
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15679025 | 1607.08232 | Radio Detection of High Energy Neutrinos | The following sections are included: <P />* Introduction * Motivation for the radio technique * Experimental strategies * Balloon experiments * Ground-based experiments * Goals of future experimental efforts * Acknowledgements * References | [
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0.02... | 6.306139 | -0.323166 | 2016-07-01 | 14 | 2017nacs.book..217C | [
"future experimental efforts",
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"Acknowledgements * References",
"the radio technique",
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] | [
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 3 | [
"10.1142/9789814759410_0015",
"10.48550/arXiv.1607.08232"
] | [
"Connolly, Amy",
"Vieregg, Abigail G."
] | [
"Ohio State University, Department of Physics and CCAPP, Columbus, OH 43210, USA",
"-"
] | [
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12500415 | 1607.06533 | VLBI observations of flared optical quasar CGRaBS J0809+5341 | A bright optical flare was detected in the high-redshift (z = 2.133) quasar CGRaBS J0809+5341 on 2014 April 13. The absolute magnitude of the object reached -30.0 during the flare, making it the brightest one (in flaring stage) among all known quasars so far. The 15-GHz flux density of CGRaBS J0809+5341 monitored in th... | [
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0... | 16.745623 | 5.43484 | 2016-07-01 | 4 | 2016PASJ...68...77A | [
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"the major optical and radio flare",
"the European VLBI Network",
"the innermost radio structure",
"a possibly emerging new... | [
"galaxies: active",
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"Astrophysics - High Energy Astrophysical Phenomena"
] | 22 | [
"10.1093/pasj/psw067",
"10.48550/arXiv.1607.06533"
] | [
"An, Tao",
"Cui, Yu-Zhu",
"Paragi, Zsolt",
"Frey, Sándor",
"Gurvits, Leonid I.",
"Gabányi, Krisztina É."
] | [
"Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Rd., 200030 Shanghai, China; School of Electrical and Electronic Engineering, Shanghai Institute of Technology, 100 Hai Quan Rd., 201418 Shanghai, China; Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, 2 West Beijing Rd., 210... | [
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12406376 | 1607.04193 | Spectral clustering for optical confirmation and redshift estimation of X-ray selected galaxy cluster candidates in the SDSS Stripe 82 | We develop a galaxy cluster finding algorithm based on spectral clustering technique to identify optical counterparts and estimate optical redshifts for X-ray selected cluster candidates. As an application, we run our algorithm on a sample of X-ray cluster candidates selected from the third XMM-Newton serendipitous sou... | [
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... | 12.940869 | 5.074866 | 2016-07-01 | 3 | 2016A&C....16..174M | [
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] | 6 | [
"10.1016/j.ascom.2016.07.001",
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] | [
"Mahmoud, E.",
"Takey, A.",
"Shoukry, A."
] | [
"Egypt-Japan University of Science and Technology (E-JUST), 21934 New Borg El-Arab, Alexandria, Egypt; National Research Institute of Astronomy and Geophysics (NRIAG), 11421 Helwan, Cairo, Egypt",
"National Research Institute of Astronomy and Geophysics (NRIAG), 11421 Helwan, Cairo, Egypt; Sorbonne Universités, U... | [
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12625680 | 1607.00535 | Energy exchanges in reconnection outflows | Reconnection outflows are highly energetic directed flows that interact with the ambient plasma or with flows from other reconnection regions. Under these conditions the flow becomes highly unstable and chaotic, as any flow jets interacting with a medium. We report here massively parallel simulations of the two cases o... | [
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... | 13.330449 | 14.60148 | 2016-07-01 | 16 | 2017PPCF...59a4019L | [
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] | 6 | [
"10.1088/0741-3335/59/1/014019",
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] | [
"Lapenta, Giovanni",
"Goldman, Martin V.",
"Newman, David L.",
"Markidis, Stefano"
] | [
"Department of Mathematics, Center for Mathematical Plasma Astrophysics, University of Leuven (KU Leuven), Celestijnenlaan 200B, 3001 Leuven, Belgium",
"University of Colorado, Boulder, CO 80309, USA",
"University of Colorado, Boulder, CO 80309, USA",
"High Performance Computing and Visualization (HPCViz), KT... | [
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12522361 | 1607.03700 | UV/Optical Emission from the Expanding Envelopes of Type II Supernovae | The early part of a supernova (SN) light curve is dominated by radiation escaping from the expanding shock-heated progenitor envelope. For polytropic hydrogen envelopes, the properties of the emitted radiation are described by simple analytic expressions and are nearly independent of the polytropic index, n. This analy... | [
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"Sapir, Nir",
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] | [
"Deptartment of Particle Physics & Astrophysics, Weizmann Institute of Science, Rehovot 76100, Israel ; Plasma Physics Department, Soreq Nuclear Research Center, Yavne 81800, Israel",
"Deptartment of Particle Physics & Astrophysics, Weizmann Institute of Science, Rehovot 76100, Israel"
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12593896 | 1607.04316 | Study of velocity centroids based on the theory of fluctuations in position-position-velocity space | We study the possibility of obtaining power spectrum of gas velocity in the turbulent interstellar medium from spatial correlation of velocity centroids (VCs) of optically thick emission lines. Combining this study with the earlier studies of centroids in Esquivel & Lazarian, we conclude that centroids are applicab... | [
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0.... | 12.172832 | 10.112529 | 2016-07-01 | 46 | 2017MNRAS.464.3617K | [
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"10.1093/mnras/stw2512",
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] | [
"Kandel, D.",
"Lazarian, A.",
"Pogosyan, D."
] | [
"Physics Department, University of Alberta, Edmonton, AB T6G 2E1, Canada; CNRS and UPMC, UMR 7095, Institut d'Astrophysique de Paris, F-75014 Paris, France",
"Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706, USA",
"Physics Department, University of Alberta, Edmonton... | [
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1950511 | 1607.01019 | Galaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift bias | The majority of galaxies in the local Universe exhibit spiral structure with a variety of forms. Many galaxies possess two prominent spiral arms, some have more, while others display a many-armed flocculent appearance. Spiral arms are associated with enhanced gas content and star formation in the discs of low-redshift ... | [
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"methods: data analysis",
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] | 21 | [
"10.1093/mnras/stw1588",
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] | [
"Hart, Ross E.",
"Bamford, Steven P.",
"Willett, Kyle W.",
"Masters, Karen L.",
"Cardamone, Carolin",
"Lintott, Chris J.",
"Mackay, Robert J.",
"Nichol, Robert C.",
"Rosslowe, Christopher K.",
"Simmons, Brooke D.",
"Smethurst, Rebecca J."
] | [
"School of Physics and Astronomy, The University of Nottingham, University Park, Nottingham NG7 2RD, UK",
"School of Physics and Astronomy, The University of Nottingham, University Park, Nottingham NG7 2RD, UK",
"School of Physics and Astronomy, University of Minnesota, 116 Church St SE, Minneapolis, MN 55455, ... | [
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12520661 | 1607.08412 | KIC011764567: An evolved Kepler -star showing substantial flare activity | We intensively studied the flare activity on the stellar object KIC011764567. The star was thought to be a solar type, with a temperature of T<SUB>eff</SUB>≈(5640±200) K, log(g) = (4.3 ± 0.3) dex, and a rotational period of P<SUB>rot</SUB>≈22 days. High-resolution spectra turn the target to an evolved object with T<SUB... | [
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-... | 8.50382 | 13.178401 | 2016-07-01 | 2 | 2017AN....338...49K | [
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] | 4 | [
"10.1002/asna.201613053",
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] | [
"Kitze, M.",
"Akopian, A. A.",
"Hambaryan, V.",
"Torres, G.",
"Neuhäuser, R."
] | [
"Astrophysikalisches Institut und Universitäts-Sternwarte, Universität Jena, Jena, Germany; Institut für Physik, Universität Rostock, Rostock, Germany",
"Byurakan Astrophysical Observatory, National Academy of Sciences of Armenia, Byurakan, Armenia",
"Astrophysikalisches Institut und Universitäts-Sternwarte, Un... | [
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2984929 | 1607.08248 | Common Envelope Ejection for a Luminous Red Nova in M101 | We present the results of optical, near-infrared, and mid-infrared observations of M101 OT2015-1 (PSN J14021678+5426205), a luminous red transient in the Pinwheel galaxy (M101), spanning a total of 16 years. The light curve showed two distinct peaks with absolute magnitudes {M}<SUB>r</SUB>≤slant -12.4 and {M}<SUB>r</SU... | [
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"binaries: close",
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] | 19 | [
"10.3847/1538-4357/834/2/107",
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] | [
"Blagorodnova, N.",
"Kotak, R.",
"Polshaw, J.",
"Kasliwal, M. M.",
"Cao, Y.",
"Cody, A. M.",
"Doran, G. B.",
"Elias-Rosa, N.",
"Fraser, M.",
"Fremling, C.",
"Gonzalez-Fernandez, C.",
"Harmanen, J.",
"Jencson, J.",
"Kankare, E.",
"Kudritzki, R. -P.",
"Kulkarni, S. R.",
"Magnier, E.",
... | [
"Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA; Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK",
"Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK",
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12594756 | 1607.04299 | Extracting information from AGN variability | Active galactic nuclei (AGNs) exhibit rapid, high-amplitude stochastic flux variations across the entire electromagnetic spectrum on time-scales ranging from hours to years. The cause of this variability is poorly understood. We present a Green's function-based method for using variability to (1) measure the time-scale... | [
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3478318 | 1607.01182 | WISE × SuperCOSMOS Photometric Redshift Catalog: 20 Million Galaxies over 3/pi Steradians | We cross-match the two currently largest all-sky photometric catalogs—mid-infrared Wide-field Infrared Survey Explorer and SuperCOSMOS scans of UKST/POSS-II photographic plates—to obtain a new galaxy sample that covers 3π steradians. In order to characterize and purify the extragalactic data set, we use external GAMA a... | [
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2892735 | 1607.08776 | XQ-100: A legacy survey of one hundred 3.5 ≲ z ≲ 4.5 quasars observed with VLT/X-shooter | We describe the execution and data reduction of the European Southern Observatory Large Programme "Quasars and their absorption lines: a legacy survey of the high-redshift Universe with VLT/X-shooter" (hereafter "XQ-100"). XQ-100 has produced and made publicly available a homogeneous and high-quality sample of echelle ... | [
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12593465 | 1607.08630 | Outer-planet scattering can gently tilt an inner planetary system | Chaotic dynamics are expected during and after planet formation, and a leading mechanism to explain large eccentricities of gas giant exoplanets is planet-planet gravitational scattering. The same scattering has been invoked to explain misalignments of planetary orbital planes with respect to their host star's spin. Ho... | [
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2417702 | 1607.04302 | Maximizing Science in the Era of LSST, Stars Study Group Report: Rotation and Magnetic Activity in the Galactic Field Population and in Open Star Clusters | This is the stars chapter of the Kavli workshop report, which resulted from the community-based study of needed US OIR capabilities in the LSST era. The full report, which will include this chapter, is anticipated to be available in Fall 2016. See NOAO website (http://www.noao.edu/meetings/lsst-oir-study/) for more det... | [
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1917404 | 1607.05903 | Improving lensing cluster mass estimate with flexion | Gravitational lensing has long been considered as a valuable tool to determine the total mass of galaxy clusters. The shear profile, as inferred from the statistics of ellipticity of background galaxies, allows us to probe the cluster intermediate and outer regions, thus determining the virial mass estimate. However, t... | [
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12436827 | 1607.07137 | Some cosmological solutions in Einstein-Chern-Simons gravity | In this paper we find new solutions for the so called Einstein-Chern-Simons Friedmann-Robertson-Walker field equations studied in refs. (Phys. Rev. D 84 (2011) 063506, Eur. Phys. J. C 74 (2014) 3087). We consider three cases:(i) in the first case we find some solutions of the five-dimensional ChS-FRW field equations wh... | [
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12472533 | 1607.06086 | Modelling the nebular emission from primeval to present-day star-forming galaxies | We present a new model of the nebular emission from star-forming galaxies in a wide range of chemical compositions, appropriate to interpret observations of galaxies at all cosmic epochs. The model relies on the combination of state-of-the-art stellar population synthesis and photoionization codes to describe the ensem... | [
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"Gutkin, Julia",
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"Instituto de Radioastronomía y Astrofísica, UNAM, Campus Morelia, Michoacan, Mexico, C.P. 58089, Mexico"
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12409191 | 1607.02148 | Natal Kicks and Time Delays in Merging Neutron Star Binaries: Implications for r-process Nucleosynthesis in Ultra-faint Dwarfs and in the Milky Way | Merging neutron star binaries are prime candidate sources for heavy r-process nucleosynthesis. The amount of heavy r-process material is consistent with the mass ejection and rates of mergers, and abundances of relic radioactive materials suggest that heavy r-process material is produced in rare events. Observations of... | [
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19742116 | 1607.02979 | Unveiling the Dynamics of the Universe | We explore the dynamics and evolution of the Universe at early and late times, focusing on both dark energy and extended gravity models and their astrophysical and cosmological consequences. Modified theories of gravity not only provide an alternative explanation for the recent expansion history of the universe, but th... | [
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"Mimoso, José Pedro",
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"Rubiera-García, Diego",
"Sáez-Gómez, Diego",
"Sousa, Lara",
"Tereno, Ismael",
"Trindade, Arlindo"
] | [
"Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal; Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Rua do Campo Alegre 687, PT4169-007 Porto, Portugal",
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12521004 | 1607.03843 | Reconnection-driven Magnetohydrodynamic Turbulence in a Simulated Coronal-hole Jet | Extreme-ultraviolet and X-ray jets occur frequently in magnetically open coronal holes on the Sun, especially at high solar latitudes. Some of these jets are observed by white-light coronagraphs as they propagate through the outer corona toward the inner heliosphere, and it has been proposed that they give rise to micr... | [
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0.... | 12.847398 | 15.719255 | 2016-07-01 | 20 | 2017ApJ...837..123U | [
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"Uritsky, Vadim M.",
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"DeVore, C. Richard",
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"Catholic University of America, 620 Michigan Avenue NE, Washington, DC 20064, USA ; Heliophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA;",
"Catholic University of America, 620 Michigan Avenue NE, Washington, DC 20064, USA ; Heliophysics Science Division, NASA Goddard Space ... | [
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12464675 | 1607.03303 | Baryogenesis in the two doublet and inert singlet extension of the Standard Model | We investigate an extension of the Standard Model containing two Higgs doublets and a singlet scalar field (2HDSM). We show that the model can have a strongly first-order phase transition and give rise to the observed baryon asymmetry of the Universe, consistent with all experimental constraints. In particular, the con... | [
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"Alanne, Tommi",
"Kainulainen, Kimmo",
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"CP^3-Origins, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark",
"Department of Physics, University of Jyväskylä, P.O. Box 35 (YFL), FI-40014 Jyväskylä, Finland ; Helsinki Institute of Physics, University of Helsinki, P.O. Box 64, FI-00014 Helsinki, Finland;",
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12407529 | 1607.03244 | Simulation study of the correlation (X<SUB>max</SUB><SUP>μ</SUP>, N<SUP>μ</SUP>) in view of obtaining information on primary mass of the UHECRs | In this paper we study, using Monte Carlo simulations, the possibility to discriminate the mass of the Ultra High Energy Cosmic Rays (UHECRs) by combining information obtained from the maximum X<SUB>max</SUB><SUP>μ</SUP> of the muon production rate longitudinal profile of Extensive Air Showers (EAS) and the number of m... | [
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] | 2 | [
"10.1016/j.astropartphys.2016.06.008",
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] | [
"Arsene, Nicusor",
"Sima, Octavian",
"Haungs, Andreas",
"Rebel, Heinigerd"
] | [
"Physics Department, University of Bucharest, Bucharest Magurele, Romania",
"Physics Department, University of Bucharest, Bucharest Magurele, Romania",
"Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany",
"Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germ... | null | [
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4017729 | 1607.03134 | Can stellar activity make a planet seem misaligned? | Several studies have shown that the occultation of stellar active regions by the transiting planet can generate anomalies in the high-precision transit light curves, and these anomalies may lead to an inaccurate estimate of the planetary parameters (e.g., the planet radius). Since the physics and geometry behind the tr... | [
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0.0001624462311156094... | 6.919075 | 14.086004 | 2016-07-01 | 20 | 2016A&A...593A..25O | [
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"stars: activity",
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"Astrophysics - Earth and Planetary Astrophysics",
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] | 6 | [
"10.1051/0004-6361/201628728",
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"Oshagh, M.",
"Dreizler, S.",
"Santos, N. C.",
"Figueira, P.",
"Reiners, A."
] | [
"Institut für Astrophysik, Georg-August-Universität, Friedrich-Hund-Platz 1, 37077, Göttingen, Germany ; Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762, Porto, Portugal",
"Institut für Astrophysik, Georg-August-Universität, Friedrich-Hund-Platz 1, 37077, Göt... | [
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12473471 | 1607.02304 | Free-free and H42α emission from the dusty starburst within NGC 4945 as observed by ALMA | We present observations of the 85.69 GHz continuum emission and H42α line emission from the central 30 arcsec within NGC 4945. Both sources of emission originate from nearly identical structures that can be modelled as exponential discs with scalelengths of ∼2.1 arcsec (or ∼40 pc). An analysis of the spectral energy di... | [
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"galaxies: individual: NGC 4945",
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"radio continuum: galaxies",
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"Astrophysics - Astrophysics of Galaxies"
] | 7 | [
"10.1093/mnras/stw1659",
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] | [
"Bendo, G. J.",
"Henkel, C.",
"D'Cruze, M. J.",
"Dickinson, C.",
"Fuller, G. A.",
"Karim, A."
] | [
"Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester M13 9PL, UK; UK ALMA Regional Centre Node",
"Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany; Faculty of Science, Astronomy Department, King Abdulaziz Univ... | [
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2763278 | 1607.02132 | A Hot Big Bang Theory: Magnetic Fields and the Early Evolution of the Protolunar Disk | The leading theory for the formation of Earth’s Moon invokes a collision between a Mars-sized body and the proto-Earth to produce a disk of orbiting material that later condenses to form the Moon. We show that the disk opacity is large, and cooling is therefore inefficient ({t}<SUB>{cool</SUB>}{{Ω }}\gg 1). In this reg... | [
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... | 8.728964 | 15.257274 | 2016-07-01 | 16 | 2016ApJ...828...58G | [
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"... | [
"planets and satellites: formation",
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] | 5 | [
"10.3847/0004-637X/828/1/58",
"10.48550/arXiv.1607.02132"
] | [
"Gammie, C. F.",
"Liao, Wei-Ting",
"Ricker, P. M."
] | [
"Department of Astronomy, University of Illinois, 1002 West Green Street, Urbana, IL 61801, USA",
"Department of Astronomy, University of Illinois, 1002 West Green Street, Urbana, IL 61801, USA",
"Department of Astronomy, University of Illinois, 1002 West Green Street, Urbana, IL 61801, USA"
] | [
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12517401 | 1607.02903 | Magnetorotational dynamo chimeras. The missing link to turbulent accretion disk dynamo models? | In Keplerian accretion disks, turbulence and magnetic fields may be jointly excited through a subcritical dynamo mechanisminvolving magnetorotational instability (MRI). This dynamo may notably contribute to explaining the time-variability of various accreting systems, as high-resolution simulations of MRI dynamo turbul... | [
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-0.027070837095379... | 11.027196 | 13.625352 | 2016-07-01 | 20 | 2017A&A...598A..87R | [
"MRI dynamo turbulence",
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"magnetic fields",
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"low Pm",... | [
"accretion",
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"magnetohydrodynamics (MHD)",
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] | 5 | [
"10.1051/0004-6361/201629285",
"10.48550/arXiv.1607.02903"
] | [
"Riols, A.",
"Rincon, F.",
"Cossu, C.",
"Lesur, G.",
"Ogilvie, G. I.",
"Longaretti, P. -Y."
] | [
"Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 0WA, UK",
"Université de Toulouse, UPS-OMP, IRAP Toulouse, 31400, Toulouse, France ; CNRS, IRAP, 14 avenue Édouard Belin, 31400, Toulouse, France",
"Institut de... | [
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12473219 | 1607.02768 | Relating information entropy and mass variance to measure bias and non-Gaussianity | We relate the information entropy and the mass variance of any distribution in the regime of small fluctuations. We use a set of Monte Carlo simulations of different homogeneous and inhomogeneous distributions to verify the relation and also test it in a set of cosmological N-body simulations. We find that the relation... | [
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... | 11.940031 | 2.685576 | 2016-07-01 | 7 | 2016MNRAS.463.4239P | [
"galaxy distributions",
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"methods: data analysis",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 7 | [
"10.1093/mnras/stw2356",
"10.48550/arXiv.1607.02768"
] | [
"Pandey, Biswajit"
] | [
"Department of Physics, Visva-Bharati University, Santiniketan, Birbhum 731235, India"
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12467807 | 1607.01395 | α' Inflation: moduli stabilisation and observable tensors from higher derivatives | The leading order dynamics of the type IIB Large Volume Scenario is characterised by the interplay between α' and non-perturbative effects which fix the overall volume and all local blow-up modes leaving (in general) several flat directions. In this paper we show that, in an arbitrary Calabi-Yau with at least one blow-... | [
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"10.1007/JHEP09(2016)026",
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"Cicoli, Michele",
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"de Alwis, Senarath",
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"Dipartimento di Fisica ed Astronomia, Università di Bologna, Bologna, Italy; INFN, Sezione di Bologna, Bologna, Italy",
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"Physics Department, University of Colorado, Boulder, CO, U.S.A.",
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12409026 | 1607.03673 | The Fossil Nuclear Outflow in the Central 30 pc of the Galactic Center | We report a new 1 pc (30″) resolution CS(J=2-1) line map of the central 30 pc of the Galactic center (GC), made with the Nobeyama 45 m telescope. We revisit our previous study of an extraplanar feature called the polar arc (PA), which is a molecular cloud located above SgrA*, with a velocity gradient perpendicular to t... | [
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] | 7 | [
"10.3847/0004-637X/831/1/72",
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"Hsieh, Pei-Ying",
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"Hwang, Chorng-Yuan",
"Shimajiri, Yoshito",
"Matsushita, Satoki",
"Koch, Patrick M.",
"Iono, Daisuke"
] | [
"Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taipei 10617, Taiwan, R.O.C. ; Institute of Astronomy, National Central University, No. 300, Jhongda Rd., Jhongli City, Taoyuan County 32001, Taiwan, R.O.C.;",
"Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, Taip... | [
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1284652 | 1607.08082 | M31N 2008-12a - The Remarkable Recurrent Nova in M31: Panchromatic Observations of the 2015 Eruption. | The Andromeda Galaxy recurrent nova M31N 2008-12a had been observed in eruption 10 times, including yearly eruptions from 2008 to 2014. With a measured recurrence period of {P}<SUB>{rec</SUB>}=351+/- 13 days (we believe the true value to be half of this) and a white dwarf very close to the Chandrasekhar limit, M31N 200... | [
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] | 12 | [
"10.3847/1538-4357/833/2/149",
"10.48550/arXiv.1607.08082"
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"Darnley, M. J.",
"Henze, M.",
"Bode, M. F.",
"Hachisu, I.",
"Hernanz, M.",
"Hornoch, K.",
"Hounsell, R.",
"Kato, M.",
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"Osborne, J. P.",
"Page, K. L.",
"Ribeiro, V. A. R. M.",
"Rodríguez-Gil, P.",
"Shafter, A. W.",
"Shara, M. M.",
"Steele, I. A.",
"Williams, S. C.",
... | [
"Astrophysics Research Institute, Liverpool John Moores University, IC2 Liverpool Science Park, Liverpool, L3 5RF, UK",
"Institut de Ciències de l'Espai (CSIC-IEEC), Campus UAB, C/Can Magrans s/n, E-08193 Cerdanyola del Valles, Spain",
"Astrophysics Research Institute, Liverpool John Moores University, IC2 Live... | [
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12511309 | 1607.08561 | f (T ) gravitational baryogenesis | We investigate how baryogenesis can occur by the presence of an f (T )-related gravitational term. We study various cases of f (T ) gravity, and we discuss in detail the effect of the novel terms on the baryon-to-entropy ratio. Additionally, we study the constraints imposed by the observational values of the baryon-to-... | [
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... | 10.249527 | 0.935222 | 2016-07-01 | 75 | 2016PhRvD..94l4005O | [
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"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"High Energy Physics - Theory"
] | 6 | [
"10.1103/PhysRevD.94.124005",
"10.48550/arXiv.1607.08561"
] | [
"Oikonomou, V. K.",
"Saridakis, Emmanuel N."
] | [
"Tomsk State Pedagogical University, 634061 Tomsk, Russia; Laboratory for Theoretical Cosmology, Tomsk State University of Control Systems and Radioelectronics (TUSUR), 634050 Tomsk, Russia",
"Physics Division, National Technical University of Athens, 15780 Zografou Campus, Athens, Greece; Instituto de Física, Po... | [
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