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12473133 | 1607.01526 | Globular clusters as tracers of the host galaxy mass distribution: the Fornax dSph test case | The Fornax dwarf spheroidal galaxy is the most massive satellites of the Milky Way, claimed to be embedded in a huge dark matter halo, and the only among the Milky Way satellites hosting five globular clusters. Interestingly, their estimated masses, ages and positions seem hardly compatible with the presence of a signi... | [
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"cuspy density profiles",
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"five globular clusters",
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"the Fornax GC system",
"a huge dark matter halo",
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"methods: numerical",
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] | 1 | [
"10.1093/mnras/stw1647",
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] | [
"Arca-Sedda, M.",
"Capuzzo-Dolcetta, R."
] | [
"Department of Physics, Sapienza, University of Rome, Piazzale Aldo Moro 5, I-00185 Rome, Italy",
"Department of Physics, Sapienza, University of Rome, Piazzale Aldo Moro 5, I-00185 Rome, Italy"
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5209849 | 1607.03009 | Impacts of fragmented accretion streams onto classical T Tauri stars: UV and X-ray emission lines | Context. The accretion process in classical T Tauri stars (CTTSs) can be studied through the analysis of some UV and X-ray emission lines which trace hot gas flows and act as diagnostics of the post-shock downfalling plasma. In the UV-band, where higher spectral resolution is available, these lines are characterized by... | [
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"line profiles",
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] | [
"Colombo, S.",
"Orlando, S.",
"Peres, G.",
"Argiroffi, C.",
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"INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy",
"INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy",
"INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134, Palermo, Italy; Dipartimento di Fisica & Chimica,... | [
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12586989 | 1607.06240 | Hybrid entropy stable HLL-type Riemann solvers for hyperbolic conservation laws | It is known that HLL-type schemes are more dissipative than schemes based on characteristic decompositions. However, HLL-type methods offer greater flexibility to large systems of hyperbolic conservation laws because the eigenstructure of the flux Jacobian is not needed. We demonstrate in the present work that several ... | [
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"10.1016/j.jcp.2016.10.034",
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] | [
"Schmidtmann, Birte",
"Winters, Andrew R."
] | [
"MathCCES, RWTH Aachen University, Schinkelstr. 2, 52062 Aachen, Germany",
"Mathematisches Institut, Universität zu Köln, Weyertal 86-90, 50931 Köln, Germany"
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168897 | 1607.07246 | Dynamics of Saturn’s great storm of 2010-2011 from Cassini ISS and RPWS | Saturn’s quasi-periodic planet-encircling storms are the largest convecting cumulus outbursts in the Solar System. The last eruption was in 1990 (Sánchez-Lavega, A. [1994]. Chaos 4, 341-353). A new eruption started in December 2010 and presented the first-ever opportunity to observe such episodic storms from a spacecra... | [
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"Astrophysics - Earth and Planetary Astrophysics"
] | 18 | [
"10.1016/j.icarus.2012.12.013",
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"Sayanagi, Kunio M.",
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"Fischer, Georg",
"Ingersoll, Andrew P.",
"Kurth, William S.",
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"Porco, Carolyn C.",
"West, Robert A."
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"Department of Atmospheric and Planetary Sciences, Hampton University, Hampton, VA 23668, USA; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA",
"Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA",
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12408831 | 1607.07888 | Observed Variability at 1 and 4 μm in the Y0 Brown Dwarf WISEP J173835.52+273258.9 | We have monitored photometrically the Y0 brown dwarf WISEP J173835.52+273258.9 (W1738) at both near- and mid-infrared wavelengths. This ≲1 Gyr old 400 K dwarf is at a distance of 8 pc and has a mass around 5 M <SUB>Jupiter</SUB>. We observed W1738 using two near-infrared filters at λ ≈ 1 μm, Y and J, on Gemini Observat... | [
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... | 7.153717 | 12.541796 | 2016-07-01 | 31 | 2016ApJ...830..141L | [
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"10.3847/0004-637X/830/2/141",
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"Leggett, S. K.",
"Cushing, Michael C.",
"Hardegree-Ullman, Kevin K.",
"Trucks, Jesica L.",
"Marley, M. S.",
"Morley, Caroline V.",
"Saumon, D.",
"Carey, S. J.",
"Fortney, J. J.",
"Gelino, C. R.",
"Gizis, J. E.",
"Kirkpatrick, J. D.",
"Mace, G. N."
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"Gemini Observatory, Northern Operations Center, 670 N. A'ohoku Place, Hilo, HI 96720, USA",
"The University of Toledo, 2801 West Bancroft Street, Mailstop 111, Toledo, OH 43606, USA",
"The University of Toledo, 2801 West Bancroft Street, Mailstop 111, Toledo, OH 43606, USA",
"The University of Toledo, 2801 W... | [
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12518466 | 1607.08820 | Dispersion by pulsars, magnetars, fast radio bursts and massive electromagnetism at very low radio frequencies | Our understanding of the universe relies mostly on electromagnetism. As photons are the messengers, fundamental physics is concerned in testing their properties. Photon mass upper limits have been earlier set through pulsar observations, but new investigations are offered by the excess of dispersion measure (DM), somet... | [
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0.0... | 6.522832 | 3.614386 | 2016-07-01 | 28 | 2017AdSpR..59..736B | [
"unknown origin",
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... | [
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"General Relativity and Quantum Cosmology",
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"10.1016/j.asr.2016.10.018",
"10.48550/arXiv.1607.08820"
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"Bentum, Mark J.",
"Bonetti, Luca",
"Spallicci, Alessandro D. A. M."
] | [
"Universiteit van Twente, Faculteit van Elektrotechniek, Wiskunde en Informatica, Telecommunication Engineering Postbus 217, 7500 AE Enschede, The Netherlands; ASTRON, Postbus 2, 7900 AA Dwingeloo, The Netherlands",
"Université d'Orléans, Observatoire des Sciences de l'Univers en région Centre, 1A rue de la Férol... | [
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12406228 | 1607.06710 | Setting the volatile composition of (exo)planet-building material. Does chemical evolution in disk midplanes matter? | Context. The atmospheres of extrasolar planets are thought to be built largely through accretion of pebbles and planetesimals. Such pebbles are also the building blocks of comets. The chemical composition of their volatiles are usually taken to be inherited from the ices in the collapsing cloud. However, chemistry in t... | [
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"10.1051/0004-6361/201628509",
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"Eistrup, Christian",
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"Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands",
"Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands ; School of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT, UK",
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2774767 | 1607.08619 | The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey | Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical fiber-bundle integral-field unit (IFU) spectroscopic survey that is one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV). With a spectral coverage of 3622-10354 Å and an average footprint of ∼500 arcsec<SUP>2</SU... | [
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... | [
"methods: data analysis",
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] | 32 | [
"10.3847/0004-6256/152/4/83",
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"Law, David R.",
"Cherinka, Brian",
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"Bizyaev, Dmitry",
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"Blanton, Michael R.",
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"Brownstein, Joel R.",
"Bundy, Kevin",
"Chen, Yanmei",
"Drory, Niv",
"D'Souza, Richard",
"Fu, Hai",
"Jones... | [
"Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA",
"Center for Astrophysical Sciences, Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA",
"Department of Physics and Astronomy, University of Kentucky, 505 Rose Street, Lexington, KY 40506-0... | [
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12585901 | 1607.08157 | Dark matter directional detection: comparison of the track direction determination | Several directional techniques have been proposed for a directional detection of Dark matter, among others anisotropic crystal detectors, nuclear emulsion plates, and low-pressure gaseous TPCs. The key point is to get access to the initial direction of the nucleus recoiling due to the elastic scattering by a WIMP. In t... | [
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12509827 | 1607.01847 | Oscillating chiral tensor spectrum from axionic inflation | We study axionic inflation with a modulated potential and examine if the primordial tensor power spectrum exhibits oscillatory feature, which is testable with future space-based gravitational-wave experiments such as DECIGO and BBO. In the case of single-field axion monodromy inflation, it turns out that it is difficul... | [
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"10.1103/PhysRevD.94.044062",
"10.48550/arXiv.1607.01847"
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"Soda, Jiro"
] | [
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"Department of Physics, Kobe University, Kobe 657-8501, Japan"
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2775537 | 1607.07699 | A High-velocity Cloud Impact Forming a Supershell in the Milky Way | Neutral atomic hydrogen (H I) gas in interstellar space is largely organized into filaments, loops, and shells, the most prominent of which are “supershells.” These gigantic structures, which require ≳ 3× {10}<SUP>52</SUP> erg to form, are generally thought to be produced by either the explosion of multiple supernovae ... | [
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"Kang, Ji-hyun",
"Gibson, Steven J.",
"Peek, J. E. G.",
"Douglas, Kevin A.",
"Korpela, Eric J.",
"Heiles, Carl E."
] | [
"Department of Physics and Astronomy, Seoul National University Seoul 151-747, Korea",
"Department of Physics and Astronomy, Seoul National University Seoul 151-747, Korea",
"Korea Astronomy and Space Science Institute Daejeon 305-348, Korea",
"Department of Physics and Astronomy, Western Kentucky University ... | [
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4552757 | 1607.02243 | Diffuse gas in retired galaxies: nebular emission templates and constraints on the sources of ionization | We present emission-line templates for passively-evolving (`retired') galaxies, useful for investigation of the evolution of the interstellar medium in these galaxies, and characterization of their high-temperature source populations. The templates are based on high signal-to-noise (>800) co-added spectra (3700-6800... | [
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"Oh, Kyuseok"
] | [
"Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany; Department of Biological and Environmental Sciences, University of Gothenburg, Medicinaregatan 18, SE-40530 Gothenburg, Sweden",
"Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany; M... | [
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12410206 | 1607.02596 | Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields | New arguments supporting the reality of large-scale fluctuations in the density of the visible matter in deep galaxy surveys are presented. A statistical analysis of the radial distributions of galaxies in the COSMOS and HDF-N deep fields is presented. Independent spectral and photometric surveys exist for each field, ... | [
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"Shirokov, S. I.",
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"Baryshev, Yu. V.",
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"Saint-Petersburg State University, St. Petersburg, Russia",
"Saint-Petersburg State University, St. Petersburg, Russia",
"Saint-Petersburg State University of Architecture and Civil Engineering, St. Petersburg, Russia"
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12593510 | 1607.00841 | H I absorption towards low-luminosity radio-loud active galactic nuclei of different accretion modes and WISE colours | H I absorption studies of active galaxies enable us to probe their circumnuclear regions and the general interstellar medium and study the supply of gas that may trigger nuclear activity. In this article, we investigate the dependence of the detection rate of H I absorption on the nature of radio galaxies based on thei... | [
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] | 12 | [
"10.1093/mnras/stw2705",
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] | [
"Chandola, Yogesh",
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] | [
"National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China",
"Cotton College State University, Panbazar, Guwahati 781 001, India; NCRA, TIFR, Post Bag 3, Ganeshkhind, Pune 411 007, India"
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12409080 | 1607.05713 | Disk Detective: Discovery of New Circumstellar Disk Candidates through Citizen Science | The Disk Detective citizen science project aims to find new stars with 22 μm excess emission from circumstellar dust using data from NASA’s Wide-field Infrared Survey Explorer (WISE) mission. Initial cuts on the AllWISE catalog provide an input catalog of 277,686 sources. Volunteers then view images of each source onli... | [
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"10.3847/0004-637X/830/2/84",
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"McElwain, Michael",
"Padgett, Deborah L.",
"Rebull, Luisa M.",
"Wisniewski, John P.",
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"NASA Goddard Space Flight Center Exoplanets and Stellar Astrophysics Laboratory, Code 667 Greenbelt, MD 21230, USA",
"Homer L. Dodge Department of Physics and Astronomy The University of Oklahoma 440 W. Brooks St. Norman, OK 73019, USA",
"Valparaiso University, Department of Physics & Astronomy, Neils Scie... | [
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12406007 | 1607.07534 | K band SINFONI spectra of two z ~ 5 submillimeter galaxy systems: upper limits to the unobscured star formation from [O II] optical emission line searches | We present deep SINFONI K-band integral field spectra of two submillimeter galaxy systems (SMG): BR 1202-0725 and J1000+0234, at z = 4.69 and 4.55, respectively. Spectra extracted for each object in the two systems do not show any signature of the [O II]λλ3726, 29 Å emission-lines, placing upper flux limits of 3.9 and ... | [
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] | 3 | [
"10.1051/0004-6361/201628952",
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] | [
"Couto, Guilherme S.",
"Colina, Luis",
"López, Javier Piqueras",
"Storchi-Bergmann, Thaisa",
"Arribas, Santiago"
] | [
"Universidade Federal do Rio Grande do Sul, IF, CP 15051, 91501-970, Porto Alegre, RS, Brazil ; Centro de Astrobiología (INTA-CSIC), Ctra de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain",
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1093440 | 1607.07969 | The Automatic Calibration of Korean VLBI Network Data | The calibration of Very Long Baseline Interferometry (VLBI) data has long been a time consuming process. The Korean VLBI Network (KVN) is a simple array consisting of three identical antennas. Because four frequencies are observed simultaneously, phase solutions can be transferred from lower frequencies to higher frequ... | [
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"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 3 | [
"10.5303/JKAS.2016.49.4.137",
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] | [
"Hodgson, Jeffrey A.",
"Lee, Sang-Sung",
"Zhao, Guang-Yao",
"Algaba, Juan-Carlos",
"Yun, Youngjoo",
"Jung, Taehyun",
"Byun, Do-Young"
] | [
"Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Korea",
"University of Science and Technology, 217 Gajeong-ro, Yuseong-gu, Daejeon 34113, Korea",
"-",
"-",
"-",
"-",
"-"
] | [
"2016ApJS..227....8L",
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"2018arXiv180202766H",
"2019ApJ...877..106P",
"2019JKAS...52...31A",
"2020ApJ...902..104L",
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] |
11492261 | 1607.06368 | The Eruption of the Candidate Young Star ASASSN-15QI | Outbursts on young stars are usually interpreted as accretion bursts caused by instabilities in the disk or the star-disk connection. However, some protostellar outbursts may not fit into this framework. In this paper, we analyze optical and near-infrared spectra and photometry to characterize the 2015 outburst of the ... | [
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... | 9.681632 | 11.623852 | 2016-07-01 | 21 | 2016ApJ...831..133H | [
"young stars",
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"∼10,000 K gas",
"hot gas",
"the probable young star ASASSN-15qi",
"accretion bursts",
"v",
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"stars: formation",
"stars: pre-main sequence",
"stars: variables: general",
"stars: winds",
"outflows",
"Astrophysics - Solar and Stellar Astrophysics"
] | 14 | [
"10.3847/0004-637X/831/2/133",
"10.48550/arXiv.1607.06368"
] | [
"Herczeg, Gregory J.",
"Dong, Subo",
"Shappee, Benjamin J.",
"Chen, Ping",
"Hillenbrand, Lynne A.",
"Jose, Jessy",
"Kochanek, Christopher S.",
"Prieto, Jose L.",
"Stanek, K. Z.",
"Kaplan, Kyle",
"Holoien, Thomas W. -S.",
"Mairs, Steve",
"Johnstone, Doug",
"Gully-Santiago, Michael",
"Zhu,... | [
"Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Lu 5, Haidian Qu, 100871 Beijing, People's Republic of China",
"Kavli Institute for Astronomy and Astrophysics, Peking University, Yi He Yuan Lu 5, Haidian Qu, 100871 Beijing, People's Republic of China",
"Carnegie Observatories, 813... | [
"2017A&A...607A.127S",
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2246995 | 1607.01062 | A Deep X-Ray View of the Bare AGN Ark 120. I. Revealing the Soft X-Ray Line Emission | The Seyfert 1 galaxy Ark 120 is a prototype example of the so-called class of bare nucleus active galactic nuclei (AGNs), whereby there is no known evidence for the presence of ionized gas along the direct line of sight. Here deep (>400 ks exposure), high-resolution X-ray spectroscopy of Ark 120 is presented from XM... | [
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... | 15.980777 | 7.975695 | 2016-07-01 | 24 | 2016ApJ...828...98R | [
"several soft X-ray emission lines",
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"larger parsec scales",
"-",
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"galaxies: active",
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"galaxies: Seyfert",
"X-rays: galaxies",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Astrophysics of Galaxies"
] | 7 | [
"10.3847/0004-637X/828/2/98",
"10.48550/arXiv.1607.01062"
] | [
"Reeves, J. N.",
"Porquet, D.",
"Braito, V.",
"Nardini, E.",
"Lobban, A.",
"Turner, T. J."
] | [
"Center for Space Science and Technology, University of Maryland Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA ; Astrophysics Group, School of Physical and Geographical Sciences, Keele University, Keele, Staffordshire, ST5 5BG, UK;",
"Observatoire Astronomique de Strasbourg, Université de Strasb... | [
"2016ApJ...832...45N",
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12594280 | 1607.08005 | Similarities and uniqueness of Ly α emitters among star-forming galaxies at z = 2.5 | We conducted a deep narrow-band imaging survey with the Subaru Prime Focus Camera on the Subaru Telescope and constructed a sample of Lyα emitters (LAEs) at z = 2.53 in the UDS-CANDELS field, where a sample of Hα emitters (HAEs) at the same redshift is already obtained from our previous narrow-band observation at near-... | [
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-0... | 13.462973 | 6.428069 | 2016-07-01 | 17 | 2017MNRAS.468.1123S | [
"HAEs",
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"Lyα",
"stellar masses",
"LAAs",
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"a certain redshift slice",... | [
"galaxies: evolution",
"galaxies: formation",
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"Astrophysics - Astrophysics of Galaxies"
] | 12 | [
"10.1093/mnras/stx091",
"10.48550/arXiv.1607.08005"
] | [
"Shimakawa, Rhythm",
"Kodama, Tadayuki",
"Shibuya, Takatoshi",
"Kashikawa, Nobunari",
"Tanaka, Ichi",
"Matsuda, Yuichi",
"Tadaki, Ken-ichi",
"Koyama, Yusei",
"Hayashi, Masao",
"Suzuki, Tomoko L.",
"Yamamoto, Moegi"
] | [
"Department of Astronomical Science, SOKENDAI, Osawa, Mitaka, Tokyo 181-8588, Japan; National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588, Japan",
"Department of Astronomical Science, SOKENDAI, Osawa, Mitaka, Tokyo 181-8588, Japan; National Astronomical Observatory of Japan, Osawa, Mitaka, To... | [
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2219791 | 1607.06829 | A perturbation study of axisymmetric strongly magnetic degenerate stars: the case of super-Chandrasekhar white dwarfs | In the presence of a strong magnetic field, a stellar equilibrium configuration, aided by the Lorentz force, can support a larger mass than a non-magnetic one. This has been considered a possible explanation of the super-Chandrasekhar mass white dwarfs giving rise to overluminous Type-Ia supernovae. We present here lin... | [
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0... | 4.619769 | 3.167871 | 2016-07-01 | 6 | 2017MNRAS.465.4026B | [
"axisymmetric configurations",
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"the magnetically supported super-Chandrasekhar mass white dwarfs",
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"long-lived super-Chandr... | [
"instabilities",
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"Astrophysics - Solar and Stellar Astrophysics",
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] | 2 | [
"10.1093/mnras/stw2979",
"10.48550/arXiv.1607.06829"
] | [
"Bera, Prasanta",
"Bhattacharya, Dipankar"
] | [
"Inter University Centre for Astronomy and Astrophysics, Post Bag 4, Pune 411007, India",
"Inter University Centre for Astronomy and Astrophysics, Post Bag 4, Pune 411007, India"
] | [
"2017ASPC..509..395B",
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1243490 | 1607.02707 | The radio spectral energy distribution of infrared-faint radio sources | Context. Infrared-faint radio sources (IFRS) are a class of radio-loud (RL) active galactic nuclei (AGN) at high redshifts (z ≥ 1.7) that are characterised by their relative infrared faintness, resulting in enormous radio-to-infrared flux density ratios of up to several thousand. <BR /> Aims: Because of their optical a... | [
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-0.0463617593050003... | 3.292793 | 8.724657 | 2016-07-01 | 10 | 2016A&A...593A.130H | [
"radio spectral energy distributions",
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"higher frequencies",
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"young AGN",
"ordinary AGN",
"observed frequencies",
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"high redshifts",
"spectral index",
"CSS sources",
"different telescopes",
"SEDs",
"significantly steeper radio SEDs",
"turnove... | [
"galaxies: active",
"galaxies: high-redshift",
"radio continuum: galaxies",
"Astrophysics - Astrophysics of Galaxies"
] | 6 | [
"10.1051/0004-6361/201527000",
"10.48550/arXiv.1607.02707"
] | [
"Herzog, A.",
"Norris, R. P.",
"Middelberg, E.",
"Seymour, N.",
"Spitler, L. R.",
"Emonts, B. H. C.",
"Franzen, T. M. O.",
"Hunstead, R.",
"Intema, H. T.",
"Marvil, J.",
"Parker, Q. A.",
"Sirothia, S. K.",
"Hurley-Walker, N.",
"Bell, M.",
"Bernardi, G.",
"Bowman, J. D.",
"Briggs, F."... | [
"Astronomisches Institut, Ruhr-Universität Bochum, Universitätsstr. 150, 44801, Bochum, Germany ; Macquarie University, Sydney, NSW, 2109, Australia; CSIRO Astronomy and Space Science, Marsfield, PO Box 76, Epping, NSW, 1710, Australia",
"CSIRO Astronomy and Space Science, Marsfield, PO Box 76, Epping, NSW, 1710,... | [
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12518234 | 1607.00228 | The Appearance of Non-Spherical Systems. Application to LMXB | We study the appearance of the neutron star-accretion disk system as seen by a distant observer in the UV/X-ray domain. The observed intensity spectra are computed assuming non-spherical geometry of the whole system, in which outgoing spectrum is not represented by the flux spectrum, the latter being valid for spherica... | [
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"X-ray data",
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"soft X-ray domain",
"X-ray spectra",
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"hot inner compact corona",
"black hole systems",
"outgoing spectrum",
"UV/X-ray energy domains",
"existing data",
"accretion disk",
"non-spherical geometry",
"emitted area",
"the... | [
"Accretion",
"accretion disks",
"Stars: neutron",
"X-rays: binaries",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 4 | [
"10.32023/0001-5237/67.1.3",
"10.48550/arXiv.1607.00228"
] | [
"Różańska, A.",
"Bełdycki, B.",
"Madej, J.",
"Adhikari, T. P.",
"You, B."
] | [
"N. Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland",
"N. Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland",
"Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland",
"-",
"-"
] | [
"2018A&A...612L..12R",
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] | [
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12472610 | 1607.02477 | Is there substructure around M87? | We present a general method to identify infalling substructure in discrete data sets with position and line-of-sight velocity data. We exploit the fact that galaxies falling on to a brightest cluster galaxy (BCG) in a virialized cluster, or dwarf satellites falling on to a central galaxy like the Milky Way, follow near... | [
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-0.... | 10.674732 | 6.126083 | 2016-07-01 | 7 | 2016MNRAS.462..298O | [
"galaxy groups",
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"galaxies",
"the satellite galaxy population",
"mock data",
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"discrete data sets",
"groups",
"a brightest cluster galaxy",
"BCG",
"the satellite population",
"a central galaxy",
"objects",
"nearly radial orbits",
"an Abel integral equat... | [
"galaxies: individual: M87",
"galaxies: kinematics and dynamics",
"galaxies: structure",
"Astrophysics - Astrophysics of Galaxies"
] | 3 | [
"10.1093/mnras/stw1574",
"10.48550/arXiv.1607.02477"
] | [
"Oldham, L. J.",
"Evans, N. W."
] | [
"Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK",
"Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK"
] | [
"2018ApJ...864...36L",
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2241475 | 1607.03701 | Ionization and Dust Charging in Protoplanetary Disks | Ionization-recombination balance in dense interstellar and circumstellar environments is a key factor for a variety of important physical processes, such as chemical reactions, dust charging and coagulation, coupling of the gas with magnetic field, and development of instabilities in protoplanetary disks. We determine ... | [
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... | 10.12242 | 13.419773 | 2016-07-01 | 25 | 2016ApJ...833...92I | [
"protoplanetary disks",
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"low grain charges",
"dusty gas",
"coagulation",
"ions",
"dense molecular clouds",
"development",
"important physical processes",
"magnetic field",
"chemical reactions",
"the d... | [
"astrochemistry",
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"dust",
"extinction",
"ISM: clouds",
"protoplanetary disks",
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Earth and Planetary Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 9 | [
"10.3847/1538-4357/833/1/92",
"10.48550/arXiv.1607.03701"
] | [
"Ivlev, A. V.",
"Akimkin, V. V.",
"Caselli, P."
] | [
"Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstr. 1, D-85748 Garching, Germany",
"Institute of Astronomy of the Russian Academy of Sciences, Pyatnitskaya Street 48, 119017 Moscow, Russia",
"Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstr. 1, D-85748 Garching, Germany"
] | [
"2016ApJS..226...12T",
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"2019MNRAS.484..161G",
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12521732 | 1607.03537 | Hubble Parameter Measurement Constraints on the Redshift of the Deceleration-Acceleration Transition, Dynamical Dark Energy, and Space Curvature | We compile an updated list of 38 measurements of the Hubble parameter H(z) between redshifts 0.07 ≤ z ≤ 2.36 and use them to place constraints on model parameters of constant and time-varying dark energy cosmological models, both spatially flat and curved. We use five models to measure the redshift of the cosmological ... | [
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12408878 | 1607.01829 | The Hot Companion and Circumbinary Disk of the Be Star HR 2142 | We present a spectroscopic investigation of the Be+sdO binary system HR 2142 that is based upon large sets of ultraviolet observations from the International Ultraviolet Explorer (IUE) and ground-based Hα observations. We measured radial velocities for the Be star component from these spectra and computed a revised orb... | [
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2068556 | 1607.05726 | An Improved Distance and Mass Estimate for Sgr A* from a Multistar Orbit Analysis | We present new, more precise measurements of the mass and distance of our Galaxy’s central supermassive black hole, Sgr A*. These results stem from a new analysis that more than doubles the time baseline for astrometry of faint stars orbiting Sgr A*, combining 2 decades of speckle imaging and adaptive optics data. Spec... | [
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12434581 | 1607.02094 | Magneto-optic effects of the Cosmic Microwave Background | Generation of magneto-optic effects by the interaction of the CMB with cosmic magnetic fields is studied. Effects which generate polarization such as the Cotton-Mouton effect, vacuum polarization and photon-pseudoscalar mixing in external magnetic field are studied. Considering the CMB linearly polarized at decoupling ... | [
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1486962 | 1607.07723 | Probing the physics and history of cosmic reionization with the Sunyaev-Zel'dovich effect | Context. The evolution of the Universe during the dark ages (DA) and the epoch of reonization (EoR) marks an important transition in the history of the Universe but it is not yet fully understood. <BR /> Aims: We study here an alternative technique to probe the DA and EoR that makes use of the Comptonization of the CMB... | [
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0.... | 13.296888 | 3.253237 | 2016-07-01 | 5 | 2016A&A...595A..21C | [
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"10.1051/0004-6361/201424904",
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"Colafrancesco, S.",
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"Emritte, M. S."
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"INAF-Osservatorio Astronomico di Roma via Frascati 33, 00040, Monteporzio, Italy ; School of Physics, University of the Witwatersrand, Private Bag 3, 2050, Johannesburg, South Africa",
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11492527 | 1607.05383 | The Clustering of Luminous Red Galaxies at z ∼ 0.7 from EBOSS and BOSS Data | We present the first scientific results from the luminous red galaxy (LRG) sample of the extended Baryon Oscillation Spectroscopic Survey (eBOSS) combined with the high-redshift galaxies of the previous BOSS sample. We measure the small- and intermediate-scale clustering from a sample of more than 97,000 galaxies in th... | [
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"Zhai, Zhongxu",
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"Hahn, ChangHoon",
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"Daws... | [
"Center for Cosmology and Particle Physics, Department of Physics, New York University, 4 Washington Place, New York, NY 10003, USA",
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12408147 | 1607.00874 | Probabilistic Inference of Basic Stellar Parameters: Application to Flickering Stars | The relations between observable stellar parameters are usually assumed to be deterministic. That is, given an infinitely precise measurement of independent variable, “x”, and some model, the value of dependent variable, “y” can be known exactly. In practice this assumption is rarely valid and intrinsic stochasticity m... | [
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"Angus, Ruth",
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] | [
"Department of Physics, University of Oxford, UK",
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12408259 | 1607.08162 | Realistic Detectability of Close Interstellar Comets | During the planet formation process, billions of comets are created and ejected into interstellar space. The detection and characterization of such interstellar comets (ICs) (also known as extra-solar planetesimals or extra-solar comets) would give us in situ information about the efficiency and properties of planet fo... | [
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"10.3847/0004-637X/825/1/51",
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"Cook, Nathaniel V.",
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"Brigham Young University, BYU Department of Physics and Astronomy N283 ESC, Provo, UT 84602, USA",
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12500421 | 1607.04385 | Sulfur and zinc abundances of red giant stars† | Sulfur and zinc are chemically volatile elements, which play significant roles as depletion-free tracers in studying galactic chemical evolution. However, regarding red giants having evolved off the main sequence, reliable abundance determinations of S and Zn seem to be difficult, despite the several studies that have ... | [
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"Takeda, Yoichi",
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2526299 | 1607.03100 | Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE | The Tully-Fisher relation (TFR) links the stellar mass of a disc galaxy, M<SUB>str</SUB>, to its rotation speed: it is well approximated by a power law, shows little scatter, and evolves weakly with redshift. The relation has been interpreted as reflecting the mass-velocity scaling (M ∝ V<SUP>3</SUP>) of dark matter ha... | [
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"10.1093/mnras/stw2691",
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"Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P 5C2, Canada",
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12465617 | 1607.01105 | Using the PPML approach for constructing a low-dissipation, operator-splitting scheme for numerical simulations of hydrodynamic flows | An approach for constructing a low-dissipation numerical method is described. The method is based on a combination of the operator-splitting method, Godunov method, and piecewise-parabolic method on the local stencil. Numerical method was tested on a standard suite of hydrodynamic test problems. In addition, the perfor... | [
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"Kulikov, Igor",
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"Department of Astrophysics, University of Vienna, Turkenschanzstrasse, 17, Vienna, 1180, Austria"
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2944614 | 1607.08738 | Spectroscopic Characterisation of CARMENES Target Candidates from FEROS, CAFE and HRS High-Resolution Spectra | CARMENES (Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Échelle Spectrographs) started a new planet survey on M-dwarfs in January this year. The new high-resolution spectrographs are operating in the visible and near-infrared at Calar Alto Observatory. They will perform hi... | [
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12472778 | 1607.05795 | The anatomy of a star-forming galaxy: pressure-driven regulation of star formation in simulated galaxies | We explore the regulation of star formation in star-forming galaxies through a suite of high-resolution isolated galaxy simulations. We use the smoothed particle hydrodynamics code GASOLINE, including photoelectric heating and metal cooling, which produces a multi-phase interstellar medium (ISM). We show that represent... | [
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"10.1093/mnras/stw1741",
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"Benincasa, S. M.",
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"Couchman, H. M. P.",
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"Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1, Canada",
"Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1, Canada",
"Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1, Canada",
"Department of Physics and Astronomy, Mc... | [
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12593906 | 1607.00386 | The global 21-cm signal in the context of the high- z galaxy luminosity function | We build a new model for the global 21-cm signal that is calibrated to measurements of the high-z galaxy luminosity function (LF) and further tuned to match the Thomson scattering optical depth of the cosmic microwave background, τ<SUB>e</SUB>. Assuming that the z ≲ 8 galaxy population can be smoothly extrapolated to h... | [
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] | 12 | [
"10.1093/mnras/stw2412",
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] | [
"Mirocha, Jordan",
"Furlanetto, Steven R.",
"Sun, Guochao"
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"Department of Physics and Astronomy, University of California, Los Angeles, CA 90024, USA",
"Department of Physics and Astronomy, University of California, Los Angeles, CA 90024, USA",
"Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA"
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12473291 | 1607.07874 | Resistive tearing instability in electron MHD: application to neutron star crusts | We study a resistive tearing instability developing in a system evolving through the combined effect of Hall drift in the electron magnetohydrodynamic limit and Ohmic dissipation. We explore first the exponential growth of the instability in the linear case and we find the fastest growing mode, the corresponding eigenv... | [
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0... | 5.069378 | 3.10706 | 2016-07-01 | 19 | 2016MNRAS.463.3381G | [
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] | 4 | [
"10.1093/mnras/stw2309",
"10.48550/arXiv.1607.07874"
] | [
"Gourgouliatos, Konstantinos N.",
"Hollerbach, Rainer"
] | [
"Department of Applied Mathematics, University of Leeds, Leeds LS2 9JT, UK",
"Department of Applied Mathematics, University of Leeds, Leeds LS2 9JT, UK"
] | [
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12510816 | 1607.05040 | Effective theory for electroweak doublet dark matter | We perform a detailed study of an effective field theory which includes the standard model particle content extended by a pair of Weyl fermionic SU(2) doublets with opposite hypercharges. A discrete symmetry guarantees that a linear combination of the doublet components is stable and can act as a candidate particle for... | [
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"10.1103/PhysRevD.94.095008",
"10.48550/arXiv.1607.05040"
] | [
"Dedes, A.",
"Karamitros, D.",
"Spanos, V. C."
] | [
"Department of Physics, Division of Theoretical Physics, University of Ioannina, GR 45110 Ioannina, Greece",
"Department of Physics, Division of Theoretical Physics, University of Ioannina, GR 45110 Ioannina, Greece",
"Section of Nuclear & Particle Physics, Department of Physics, National and Kapodistrian U... | [
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3829677 | 1607.05089 | Absolute kinematics of radio-source components in the complete S5 polar cap sample. IV. Proper motions of the radio cores over a decade and spectral properties | We have carried out a high-precision astrometric analysis of two very-long-baseline-interferometry (VLBI) epochs of observation of the 13 extragalactic radio sources in the complete S5 polar cap sample. The VLBI epochs span a time baseline of ten years and enable us to achieve precisions in the proper motions of the so... | [
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"10.1051/0004-6361/201628149",
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"Martí-Vidal, I.",
"Abellán, F. J.",
"Marcaide, J. M.",
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"Pérez-Torres, M. A.",
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] | [
"Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 43992, Onsala, Sweden",
"Departament d'Astronomia i Astrofísica, Universitat de València, C/Dr. Moliner 50, 46100, Burjassot, Spain",
"Departament d'Astronomia i Astrofísica, Universitat de València, C/Dr. Moli... | [
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12408911 | 1607.03982 | Galaxy Groups in the 2Mass Redshift Survey | A galaxy group catalog is constructed from the 2MASS Redshift Survey (2MRS) with the use of a halo-based group finder. The halo mass associated with a group is estimated using a “GAP” method based on the luminosity of the central galaxy and its gap with other member galaxies. Tests using mock samples show that this met... | [
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... | 12.206766 | 5.244895 | 2016-07-01 | 26 | 2016ApJ...832...39L | [
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"dark matter",
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] | 10 | [
"10.3847/0004-637X/832/1/39",
"10.48550/arXiv.1607.03982"
] | [
"Lu, Yi",
"Yang, Xiaohu",
"Shi, Feng",
"Mo, H. J.",
"Tweed, Dylan",
"Wang, Huiyuan",
"Zhang, Youcai",
"Li, Shijie",
"Lim, S. H."
] | [
"Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Nandan Road 80, Shanghai 200030, China",
"Center for Astronomy and Astrophysics, Shanghai Jiao Tong University, Shanghai 200240, China ; IFSA Collaborative Innovation Center, Shanghai Jiao Tong University, Shanghai 200240, ... | [
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12436396 | 1607.06105 | A Monodromy from London | We focus on the massive gauge theory formulation of axion monodromy inflation. We argue that a gauge symmetry hidden in these models is the key protection mechanism from dangerous corrections from both field theory and gravitational dynamics. The effective theory of large field inflation is a dual to a massive U(1) 4-f... | [
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... | 10.572262 | -1.467464 | 2016-07-01 | 17 | 2016arXiv160706105K | [
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"a gauge theory",
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"High Energy Physics - Theory",
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"10.48550/arXiv.1607.06105"
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"Kaloper, Nemanja",
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12583815 | 1607.08610 | Bouncing cosmology inspired by regular black holes | In this article, we present a bouncing cosmology inspired by a family of regular black holes. This scale-dependent cosmology deviates from the cosmological principle by means of a scale factor which depends on the time and the radial coordinate as well. The model is isotropic but not perfectly homogeneous. That is, thi... | [
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] | 6 | [
"10.1007/s10714-017-2288-6",
"10.48550/arXiv.1607.08610"
] | [
"Neves, J. C. S."
] | [
"Instituto de Matemática, Estatística e Computação Científica, Universidade Estadual de Campinas, Campinas, SP, Brazil"
] | [
"2018AN....339..298N",
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12509665 | 1607.01677 | Current and future constraints on Bekenstein-type models for varying couplings | Astrophysical tests of the stability of dimensionless fundamental couplings, such as the fine-structure constant α and the proton-to-electron mass ratio μ , are an optimal probe of new physics. There is a growing interest in these tests, following indications of possible spacetime variations at the few parts per millio... | [
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0... | 9.209813 | 0.311204 | 2016-07-01 | 12 | 2016PhRvD..94b3503L | [
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] | 3 | [
"10.1103/PhysRevD.94.023503",
"10.48550/arXiv.1607.01677"
] | [
"Leite, A. C. O.",
"Martins, C. J. A. P."
] | [
"Centro de Astrofísica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal; Instituto de Astrofísica e Ciências do Espaço, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal; Faculdade de Ciências, Universidade do Porto, Rua do Campo Alegre, 4150-007 Porto, Portugal",
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12593997 | 1607.01394 | Merger-driven evolution of the effective stellar initial mass function of massive early-type galaxies | The stellar initial mass function (IMF) of early-type galaxies is the combination of the IMF of the stellar population formed in situ and that of accreted stellar populations. Using as an observable the effective IMF α<SUB>IMF</SUB>, defined as the ratio between the true stellar mass of a galaxy and the stellar mass in... | [
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"stars: luminosity function",
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"Astrophysics - Astrophysics of Galaxies",
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] | 3 | [
"10.1093/mnras/stw2919",
"10.48550/arXiv.1607.01394"
] | [
"Sonnenfeld, Alessandro",
"Nipoti, Carlo",
"Treu, Tommaso"
] | [
"Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan; Department of Physics and Astronomy, University of California, Los Angeles, 430 Portola Plaza, Los Angeles, CA 90025, USA",
"Department of Physics and Astronomy, Bologna University, viale Berti-Pichat 6/2, I-40127 Bologna, Italy",
... | [
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12473435 | 1607.04264 | Evidence for the magnetar nature of 1E 161348-5055 in RCW 103 | We report on the detection of a bright, short, structured X-ray burst coming from the supernova remnant RCW 103 on 2016 June 22 caught by the Swift/Burst Alert Telescope (BAT) monitor, and on the follow-up campaign made with Swift/X-ray Telescope, Swift/UV/Optical Telescope, and the optical/near-infrared (NIR) Gamma-Ra... | [
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... | 5.192254 | 4.426284 | 2016-07-01 | 55 | 2016MNRAS.463.2394D | [
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"X-rays: general",
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"10.1093/mnras/stw2023",
"10.48550/arXiv.1607.04264"
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"D'Aì, A.",
"Evans, P. A.",
"Burrows, D. N.",
"Kuin, N. P. M.",
"Kann, D. A.",
"Campana, S.",
"Maselli, A.",
"Romano, P.",
"Cusumano, G.",
"La Parola, V.",
"Barthelmy, S. D.",
"Beardmore, A. P.",
"Cenko, S. B.",
"De Pasquale, M.",
"Gehrels, N.",
"Greiner, J.",
"Kennea, J. A.",
"Klo... | [
"INAF/IASF Palermo, via Ugo La Malfa 153, I-90146 Palermo, Italy",
"Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK",
"Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, USA",
"Mullard Space Science Laboratory,... | [
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12464691 | 1607.02442 | The tau of galaxy clusters | The recent emergence of detections of the kinetic Sunyeav-Zel'dovich (kSZ) effect through cross-correlation techniques is encouraging for the prospects of future cosmic microwave background (CMB) experiments. Extracting information on the large-scale velocity fields and constraining cosmological parameters from such kS... | [
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0... | 13.300249 | 2.775191 | 2016-07-01 | 65 | 2016JCAP...08..058B | [
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] | 15 | [
"10.1088/1475-7516/2016/08/058",
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] | [
"Battaglia, N."
] | [
"Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, U.S.A."
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"2016PhRvD..94d3522A",
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12473523 | 1607.05324 | Dark matter inside early-type galaxies as function of mass and redshift | We study the behaviour of the dynamical and stellar mass inside the effective radius (r<SUB>e</SUB>) of early-type galaxies (ETGs). We use several samples of ETGs - ranging from 19 000 to 98 000 objects - from the ninth data release of the Sloan Digital Sky Survey. We consider Newtonian dynamics, different light profil... | [
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] | 3 | [
"10.1093/mnras/stw1661",
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"Nigoche-Netro, A.",
"Ramos-Larios, G.",
"Lagos, P.",
"Ruelas-Mayorga, A.",
"de la Fuente, E.",
"Kemp, S. N.",
"Navarro, S. G.",
"Corral, L. J.",
"Hidalgo-Gámez, A. M."
] | [
"Instituto de Astronomía y Meteorología, Universidad de Guadalajara, Guadalajara, Jalisco 44130, México",
"Instituto de Astronomía y Meteorología, Universidad de Guadalajara, Guadalajara, Jalisco 44130, México",
"Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, Rua das Estrelas, P-4150-762 ... | [
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3458517 | 1607.03114 | V346 Normae: first post-outburst observations of an FU Orionis star | During their formation phase, stars gain most of their mass in violent episodic accretion events, such as observed in FU Orionis (FUor) and EXor stars. V346 Normae is a well-studied FUor that underwent a strong outburst beginning around 1980. Here, we report on photometric and spectroscopic observations, which show tha... | [
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"accretion",
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"stars: pre-main sequence",
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"Astrophysics - Solar and Stellar Astrophysics"
] | 6 | [
"10.1093/mnrasl/slw126",
"10.48550/arXiv.1607.03114"
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"Kraus, S.",
"Caratti o Garatti, A.",
"Garcia-Lopez, R.",
"Kreplin, A.",
"Aarnio, A.",
"Monnier, J. D.",
"Naylor, T.",
"Weigelt, G."
] | [
"School of Physics, Astrophysics Group, University of Exeter, Stocker Road, Exeter EX4 4QL, UK",
"Dublin Institute for Advanced Studies, School of Cosmic Physics, Astronomy and Astrophysics Section, 31 Fitzwilliam Place, Dublin 2, Ireland",
"Dublin Institute for Advanced Studies, School of Cosmic Physics, Astro... | [
"2017A&A...597L..10K",
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1683108 | 1607.06394 | Outbursts in ultracompact X-ray binaries | Context. Very faint X-ray binaries appear to be transient in many cases with peak luminosities much fainter than that of usual soft X-ray transients, but their nature still remains elusive. <BR /> Aims: We investigate the possibility that this transient behaviour is due to the same thermal/viscous instability which is ... | [
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... | 6.496911 | 6.344964 | 2016-07-01 | 14 | 2016A&A...594A..87H | [
"bright soft X-ray transients",
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... | [
"accretion",
"accretion disks",
"X-rays: binaries",
"instabilities",
"Astrophysics - High Energy Astrophysical Phenomena"
] | 3 | [
"10.1051/0004-6361/201628434",
"10.48550/arXiv.1607.06394"
] | [
"Hameury, J. -M.",
"Lasota, J. -P."
] | [
"Observatoire Astronomique de Strasbourg, Université de Strasbourg, CNRS UMR 7550, 67000, Strasbourg, France",
"Institut d'Astrophysique de Paris, CNRS et Sorbonne Universités, UPMC Paris 06, UMR 7095, 98bis Bd Arago, 75014, Paris, France; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Barty... | [
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"2017MNRAS.464..398D",
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3221474 | 1607.01782 | Approximate Bayesian computation in large-scale structure: constraining the galaxy-halo connection | Standard approaches to Bayesian parameter inference in large-scale structure assume a Gaussian functional form (chi-squared form) for the likelihood. This assumption, in detail, cannot be correct. Likelihood free inferences such as approximate Bayesian computation (ABC) relax these restrictions and make inference possi... | [
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0.024... | 11.644382 | 3.301285 | 2016-07-01 | 44 | 2017MNRAS.469.2791H | [
"consistent HOD parameter constraints",
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"galaxy number density",
"Gaussian form",
"galaxies",
"dark matter haloes",
"inference",
"free inferences",
"the HOD parameters",
"ABC",
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"methods: data analysis",
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"galaxies: haloes",
"dark matter",
"large-scale structure of Universe",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 3 | [
"10.1093/mnras/stx894",
"10.48550/arXiv.1607.01782"
] | [
"Hahn, ChangHoon",
"Vakili, Mohammadjavad",
"Walsh, Kilian",
"Hearin, Andrew P.",
"Hogg, David W.",
"Campbell, Duncan"
] | [
"Center for Cosmology and Particle Physics, Department of Physics, New York University, 726 Broadway, New York, NY 10003, USA",
"Center for Cosmology and Particle Physics, Department of Physics, New York University, 726 Broadway, New York, NY 10003, USA",
"Center for Cosmology and Particle Physics, Department o... | [
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1267015 | 1607.06488 | Global Energetics of Solar Flares. III. Nonthermal Energies | This study entails the third part of a global flare energetics project, in which Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) data of 191 M and X-class flare events from the first 3.5 years of the Solar Dynamics Observatory mission are analyzed. We fit a thermal and a nonthermal component to RHESSI spectra, y... | [
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0.044347... | 13.258176 | 15.646975 | 2016-07-01 | 58 | 2016ApJ...832...27A | [
"thermal energies",
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"low-energy cutoff energies",
"SUB",
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"The nonthermal energy",
"the nonthermal energy",
"the thermal energy",
"The total dissipated magnetic energy",
"the total nonthermal energy E <SUB",
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"radiation mechanisms: nonthermal",
"Sun: flares",
"Sun: particle emission",
"Sun: X-rays",
"gamma rays",
"Astrophysics - Solar and Stellar Astrophysics"
] | 8 | [
"10.3847/0004-637X/832/1/27",
"10.48550/arXiv.1607.06488"
] | [
"Aschwanden, Markus J.",
"Holman, Gordon",
"O'Flannagain, Aidan",
"Caspi, Amir",
"McTiernan, James M.",
"Kontar, Eduard P."
] | [
"Lockheed Martin, Solar and Astrophysics Laboratory, Org. A021S, Bldg. 252, 3251 Hanover Street, Palo Alto, CA 94304, USA",
"Code 671, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA",
"Astrophysics Research Group, School of Physics, Trinity College Dublin, Dublin 2, Ireland",
"Planetary Science Di... | [
"2017Ap&SS.362..113F",
"2017ApJ...836...17A",
"2017ApJ...841..124V",
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12594329 | 1607.05442 | Density and metallicity of the Milky Way circumgalactic gas | The halo of the Milky Way circumgalactic gas extends up to the virial radius of the Galaxy, ∼250 kpc. The halo properties may be deduced from X-ray spectroscopic observations and from studies of the ram-pressure stripping of satellite dwarf galaxies. The former method is more precise, but its results depend crucially o... | [
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... | 12.595534 | 8.25086 | 2016-07-01 | 7 | 2017MNRAS.468L..36T | [
"satellite dwarf galaxies",
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"r.",
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"∼250",
"studies",
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"the galactocentric distance",
"The corresponding gas density profile",
"density",
"the gas metallicity",
"r",
"the circu... | [
"ISM: structure",
"Galaxy: halo",
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"Astrophysics - Astrophysics of Galaxies",
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] | 6 | [
"10.1093/mnrasl/slx022",
"10.48550/arXiv.1607.05442"
] | [
"Troitsky, Sergey"
] | [
"Institute for Nuclear Research of the Russian Academy of Sciences, 60th October Anniversary prospect 7a, 117312 Moscow, Russia; Moscow Institute for Physics and Technology, Institutskii per. 9, 141700 Dolgoprudny, Moscow Region, Russia"
] | [
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12472567 | 1607.02054 | [O III] emission line as a tracer of star-forming galaxies at high redshifts: comparison between Hα and [O III] emitters at z=2.23 in HiZELS | We investigate the properties of z = 2.23 Hα and [O III] λ5007 emitters using the narrow-band-selected samples obtained from the High-z Emission Line Survey. We construct two samples of the Hα and [O III] emitters and compare their integrated physical properties. We find that the distribution of stellar masses, dust ex... | [
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0.00... | 12.829719 | 7.016621 | 2016-07-01 | 24 | 2016MNRAS.462..181S | [
"Hα emission",
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"high redshift",
"specific SFRs",
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"[O III",
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"UV</SUB",
"the full galaxy sample",
"emitters",
"the High-z Emission Line Survey",
"the highest star-forming activity",
"... | [
"galaxies: evolution",
"galaxies: high-redshift",
"Astrophysics - Astrophysics of Galaxies"
] | 6 | [
"10.1093/mnras/stw1655",
"10.48550/arXiv.1607.02054"
] | [
"Suzuki, T. L.",
"Kodama, T.",
"Sobral, D.",
"Khostovan, A. A.",
"Hayashi, M.",
"Shimakawa, R.",
"Koyama, Y.",
"Tadaki, K. -i.",
"Tanaka, I.",
"Minowa, Y.",
"Yamamoto, M.",
"Smail, I.",
"Best, P. N."
] | [
"Department of Astronomical Science, SOKENDAI (The Graduate University for Advanced Studies), Mitaka, Tokyo 181-8588, Japan; Optical and Infrared Astronomy Division, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan",
"Department of Astronomical Science, SOKENDAI (The Graduate University f... | [
"2017ApJ...849...39S",
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12409154 | 1607.07447 | Complete Element Abundances of Nine Stars in the r-process Galaxy Reticulum II | We present chemical abundances derived from high-resolution Magellan/Magellan Inamori Kyocera Echelle spectra of the nine brightest known red giant members of the ultra-faint dwarf galaxy Reticulum II (Ret II). These stars span the full metallicity range of Ret II (-3.5 < [Fe/H] < -2). Seven of the nine stars hav... | [
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0.... | 7.951599 | 8.825322 | 2016-07-01 | 158 | 2016ApJ...830...93J | [
"other ultra-faint dwarf galaxies",
"Ret II",
"Reticulum II",
"Galaxies",
"every other ultra-faint dwarf galaxy",
"r-process halo stars",
"stars",
"r-process enhanced stars",
"r-process elements",
"known r-process pattern",
"lighter elements",
"additional r-process sites",
"r-process materia... | [
"galaxies: dwarf",
"galaxies: individual: Ret II",
"Local Group",
"nuclear reactions",
"nucleosynthesis",
"abundances",
"stars: abundances",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Solar and Stellar Astrophysics"
] | 26 | [
"10.3847/0004-637X/830/2/93",
"10.48550/arXiv.1607.07447"
] | [
"Ji, Alexander P.",
"Frebel, Anna",
"Simon, Joshua D.",
"Chiti, Anirudh"
] | [
"Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA ; Joint Institute for Nuclear Astrophysics—Center for Evolution of the Elements, East Lansing, MI:48824, USA;",
"Department of Physics and Kavli Institute for Astrophysic... | [
"2016ApJ...832..149B",
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5170993 | 1607.02781 | Infrared Observations of the Quintuplet Proper Members using SOFIA/FORCAST and Gemini/TReCS | Since their discovery, the Quintuplet proper members (QPMs) have been somewhat mysterious in nature. Originally dubbed the “cocoon stars” due to their cool featureless spectra, high-resolution near-infrared imaging observations have shown that at least two of the objects exhibit “pinwheel” nebulae consistent with binar... | [
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-... | 8.697518 | 8.321824 | 2016-07-01 | 5 | 2016ApJ...827..136H | [
"enhanced mass loss",
"r}<SUP>-2</SUP",
"high-resolution imaging data",
"typical dusty Wolf-Rayet stars",
"binary systems",
"radial density profiles",
"TReCS",
"constant mass-loss rates",
"the Faint Object Infrared Camera",
"conjunction",
"nature",
"extended structures",
"∼0.1″-0.2″",
"QPM... | [
"Galaxy: center",
"stars: evolution",
"stars: massive",
"stars: Wolf-Rayet",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Solar and Stellar Astrophysics"
] | 4 | [
"10.3847/0004-637X/827/2/136",
"10.48550/arXiv.1607.02781"
] | [
"Hankins, M. J.",
"Lau, R. M.",
"Morris, M. R.",
"Sanchez-Bermudez, J.",
"Pott, J. U.",
"Adams, J. D.",
"Herter, T. L."
] | [
"Astronomy Department, 202 Space Sciences Building, Cornell University, Ithaca, NY 14853-6801, USA",
"Astronomy Department, 202 Space Sciences Building, Cornell University, Ithaca, NY 14853-6801, USA; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA... | [
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"2020ApJ...894...55H",
"2020ApJ...898...74L",
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12408595 | 1607.03567 | Constraining Warm Dark Matter Mass with Cosmic Reionization and Gravitational Waves | We constrain the warm dark matter (WDM) particle mass with observations of cosmic reionization and CMB optical depth. We suggest that the gravitational waves (GWs) from stellar-mass black holes (BHs) could give a further constraint on WDM particle mass for future observations. The star formation rates (SFRs) of Populat... | [
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0.015... | 8.770711 | -0.721419 | 2016-07-01 | 15 | 2016ApJ...829...29T | [
"WDM particle mass",
"keV",
"Pop III BHs",
"Pop III",
"future observations",
"WDM",
"CMB optical depth",
"stellar BHs",
"low frequencies",
"observation",
"observations",
"Pop I/II BHs",
"Population III",
"the WDM particle mass",
"BHs",
"m}<SUB>{{x</SUB>}}=1",
"m}<SUB>{{x</SUB>}}=3",
... | [
"cosmology: theory",
"dark ages",
"reionization",
"first stars",
"dark matter",
"gravitational waves",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 6 | [
"10.3847/0004-637X/829/1/29",
"10.48550/arXiv.1607.03567"
] | [
"Tan, Wei-Wei",
"Wang, F. Y.",
"Cheng, K. S."
] | [
"School of Astronomy and Space Science, Nanjing University, Nanjing 210093, China ; Key laboratory of Modern Astronomy and Astrophysics (Nanjing University), Nanjing 210093, China;",
"School of Astronomy and Space Science, Nanjing University, Nanjing 210093, China ; Key laboratory of Modern Astronomy and Astrophy... | [
"2016Nanot..27X5602C",
"2017ApJ...836..107H",
"2017ChPhB..26h8101Z",
"2017PhRvD..96j3539L",
"2018JCAP...08..045D",
"2018MNRAS.477.2154B",
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"2019MNRAS.489..487S",
"2019Nanot..30W5703T",
"2020JCAP...03..042B",
"2020PDU....2800476N",
"2020SeScT..35b5020S",
"2021MNRAS.506.5... | [
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2583156 | 1607.05732 | Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages | There is still much debate surrounding how the most massive, central galaxies in the local universe have assembled their stellar mass, especially the relative roles of in situ growth versus later accretion via mergers. In this paper, we set firmer constraints on the evolutionary pathways of the most massive central gal... | [
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"dark matter accretion histories",
"stellar mass",
"stellar initial mass function",
"massive galaxies",
"star formation rate",
"stellar ages",
"merger rates",
"later accretion",
"mass M<SUB",
"the mass accretion history",
"mergers",
"situ growth",
"M<SUB",
"their host dark matter",
"star... | [
"galaxies: abundances",
"galaxies: evolution",
"galaxies: formation",
"galaxies: statistics",
"galaxies: structure",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 6 | [
"10.1093/mnras/stw1771",
"10.48550/arXiv.1607.05732"
] | [
"Buchan, Stewart",
"Shankar, Francesco"
] | [
"School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK",
"School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK"
] | [
"2017ApJ...840...34S",
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"2020MNRAS.491..634G",
"2022MNRAS.510.5639M",
"2022MNRAS.511..506C",
"2023ApJ...954...97B",
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12406183 | 1607.02975 | The faint end of the 250 μm luminosity function at z < 0.5 | <BR /> Aims: We aim to study the 250 μm luminosity function (LF) down to much fainter luminosities than achieved by previous efforts. <BR /> Methods: We developed a modified stacking method to reconstruct the 250 μm LF using optically selected galaxies from the SDSS survey and Herschel maps of the GAMA equatorial field... | [
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"Wang, L.",
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"Dye, S.",
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"Farrah, D.",
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"Loveday, J.",
"Maddox, S.",
"Oliver, S.",
"Viero, M."
] | [
"SRON Netherlands Institute for Space Research, Landleven 12, 9747 AD, Groningen, The Netherlands ; Kapteyn Astronomical Institute, University of Groningen, Postbus 800, 9700 AV, Groningen, The Netherlands; ICC & CEA, Department of Physics, Durham University, Durham, DH1 3LE, UK",
"ICC & CEA, Department o... | [
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12473475 | 1607.02144 | Black holes in stellar-mass binary systems: expiating original spin? | We investigate systematically whether accreting black hole systems are likely to reach global alignment of the black hole spin and its accretion disc with the binary plane. In low-mass X-ray binaries (LMXBs), there is only a modest tendency to reach such global alignment, and it is difficult to achieve fully: except fo... | [
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0.... | 6.792903 | 6.535344 | 2016-07-01 | 14 | 2016MNRAS.462..464K | [
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] | 5 | [
"10.1093/mnras/stw1598",
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] | [
"King, Andrew",
"Nixon, Chris"
] | [
"Theoretical Astrophysics Group, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK; Astronomical Institute Anton Pannekoek, University of Amsterdam, Science Park 904, NL-1098 XH Amsterdam, Netherlands; Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, Nethe... | [
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12594146 | 1607.08250 | Dust traps as planetary birthsites: basics and vortex formation | We present a simple model for low-mass planet formation and subsequent evolution within 'transition' discs. We demonstrate quantitatively that the predicted and observed structures of such discs are prime birthsites of planets. Planet formation is likely to proceed through pebble accretion, should a planetary embryo (M... | [
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] | 2 | [
"10.1093/mnras/stx302",
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] | [
"Owen, James E.",
"Kollmeier, Juna A."
] | [
"Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540, USA",
"Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540, USA; Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101, USA"
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4331519 | 1607.07918 | Investigating the dusty torus of Seyfert galaxies using SOFIA/FORCAST photometry | We present 31.5 μm imaging photometry of 11 nearby Seyfert galaxies observed from the Stratospheric Observatory For Infrared Astronomy (SOFIA) using the Faint Object infraRed CAmera for the SOFIA Telescope (FORCAST). We tentatively detect extended 31 μm emission for the first time in our sample. In combination with thi... | [
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"10.1093/mnras/stw1780",
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"Fuller, L.",
"Lopez-Rodriguez, E.",
"Packham, C.",
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"Radomski, J.",
"Ichikawa, K.",
"García-Bernete, I.",
"González-Martín, O.",
"Díaz-Santos, T.",
"Martínez-Paredes, M."
] | [
"Department of Physics & Astronomy, University of Texas at San Antonio, One UTSA Circle, San Antonio, TX 78249, USA",
"Department of Astronomy, University of Texas at Austin, 2515 Speedway, Stop C1402, Austin, TX 78712, USA; McDonald Observatory, University of Texas at Austin, 2515 Speedway, Stop C1402, Austi... | [
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12510124 | 1607.03973 | Observable cosmological vector mode in the dark ages | The second-order vector mode is inevitably induced from the coupling of first-order scalar modes in cosmological perturbation theory and might hinder a possible detection of primordial gravitational waves from inflation through 21 cm lensing observations. Here, we investigate the weak lensing signal in 21 cm photons em... | [
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"the cosmological vector and tensor modes",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 2 | [
"10.1103/PhysRevD.94.063523",
"10.48550/arXiv.1607.03973"
] | [
"Saga, Shohei"
] | [
"Department of Physics and Astrophysics, Nagoya University, Aichi 464-8602, Japan"
] | [
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3016013 | 1607.06621 | Signatures of nonlinear mode interactions in the pulsating hot B subdwarf star KIC 10139564 | Context. The unprecedented photometric quality and time coverage offered by the Kepler spacecraft has opened up new opportunities to search for signatures of nonlinear effects that affect oscillation modes in pulsating stars. <BR /> Aims: The data accumulated on the pulsating hot B subdwarf KIC 10139564 are used to exp... | [
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] | 2 | [
"10.1051/0004-6361/201629132",
"10.48550/arXiv.1607.06621"
] | [
"Zong, W.",
"Charpinet, S.",
"Vauclair, G."
] | [
"Université de Toulouse, UPS-OMP, IRAP, 31400, Toulouse, France ; CNRS, IRAP, 14 avenue Edouard Belin, 31400, Toulouse, France",
"Université de Toulouse, UPS-OMP, IRAP, 31400, Toulouse, France ; CNRS, IRAP, 14 avenue Edouard Belin, 31400, Toulouse, France",
"Université de Toulouse, UPS-OMP, IRAP, 31400, Toulous... | [
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2263112 | 1607.04412 | High-precision astrometry towards ELTs | With the aim of paving the road for future accurate astrometry with MICADO at the European-ELT, we performed an astrometric study using two different but complementary approaches to investigate two critical components that contribute to the total astrometric accuracy. First, we tested the predicted improvement in the a... | [
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"Gemini South",
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"view",
"the only currently available Multi-Conjugate Adaptive Optics",
"a crowded Galactic globu... | [
"Astrophysics - Instrumentation and Methods for Astrophysics"
] | 3 | [
"10.1117/12.2232478",
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"Massari, Davide",
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"Tolstoy, Eline",
"McConnachie, Alan",
"Stuik, Remko",
"Schreiber, Laura",
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"Clénet, Yann",
"Davies, Richard",
"Gratadour, Damien",
"Kuijken, Konrad",
"Navarro, Ramon",
"Pott, Jörg-Uwe",
"Rodeghiero, Gabriele",
"Turri, Paolo",
... | [
"INAF - Osservatorio Astronomico di Bologna (Italy)",
"INAF - Osservatorio Astronomico di Bologna (Italy)",
"Univ. of Groningen (Netherlands)",
"Herzberg Astronomy and Astrophysics, National Research Council Canada (Canada)",
"Leiden Observatory (Netherlands)",
"INAF - Osservatorio Astronomico di Bologna ... | [
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5398407 | 1607.07377 | Frames of most uniform Hubble flow | It has been observed [1,2] that the locally measured Hubble parameter converges quickest to the background value and the dipole structure of the velocity field is smallest in the reference frame of the Local Group of galaxies. We study the statistical properties of Lorentz boosts with respect to the Cosmic Microwave Ba... | [
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0... | 11.508515 | 1.900224 | 2016-07-01 | 12 | 2016JCAP...10..016K | [
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"the boost velocities",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 9 | [
"10.1088/1475-7516/2016/10/016",
"10.48550/arXiv.1607.07377"
] | [
"Kraljic, David",
"Sarkar, Subir"
] | [
"Rudolf Peierls Centre for Theoretical Physics, University of Oxford, 1 Keble Road, Oxford, OX1 3NP, U.K.",
"Rudolf Peierls Centre for Theoretical Physics, University of Oxford, 1 Keble Road, Oxford, OX1 3NP, U.K.; Niels Bohr International Academy, University of Copenhagen, Blegdamsvej 17, 2100 Copenhagen, Denmar... | [
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3360123 | 1607.03554 | Metallicity and Age of the Stellar Stream around the Disk Galaxy NGC 5907 | Stellar streams have become central to studies of the interaction histories of nearby galaxies. To characterize the most prominent parts of the stellar stream around the well-known nearby (d = 17 Mpc) edge-on disk galaxy NGC 5907, we have obtained and analyzed new, deep gri Subaru/Suprime-Cam and 3.6 μm Spitzer/Infrare... | [
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... | 9.794573 | 7.481621 | 2016-07-01 | 13 | 2016AJ....152...72L | [
"Stellar streams",
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"stellar mass ratio",
"3.6 μm Spitzer/Infrared Array Camera observations",
"the stellar stream",
"Spitzer/Infrared Array Camera",
"minor/major merger formation models",
"new, deep gri Subaru/Suprime-Cam",
"a single-burst stellar population synthesis model",
"t... | [
"galaxies: evolution",
"galaxies: interactions",
"galaxies: structure",
"Astrophysics - Astrophysics of Galaxies"
] | 5 | [
"10.3847/0004-6256/152/3/72",
"10.48550/arXiv.1607.03554"
] | [
"Laine, Seppo",
"Grillmair, Carl J.",
"Capak, Peter",
"Arendt, Richard G.",
"Romanowsky, Aaron J.",
"Martínez-Delgado, David",
"Ashby, Matthew L. N.",
"Davies, James E.",
"Majewski, Stephen R.",
"Brodie, Jean P.",
"GaBany, R. Jay",
"Arnold, Jacob A."
] | [
"Spitzer Science Center-Caltech, MS 314-6, Pasadena, CA 91125, USA",
"Spitzer Science Center-Caltech, MS 314-6, Pasadena, CA 91125, USA",
"Spitzer Science Center-Caltech, MS 314-6, Pasadena, CA 91125, USA",
"CRESST/UMBC/NASA GSFC, Code 665, Greenbelt, MD 20771, USA",
"Department of Physics and Astronomy, Sa... | [
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2417729 | 1607.03886 | Kepler Flares. IV. A Comprehensive Analysis of the Activity of the dM4e Star GJ 1243 | We present a comprehensive study of the active dM4e star GJ 1243. We use previous observations and ground-based echelle spectroscopy to determine that GJ 1243 is a member of the Argus association of field stars, suggesting it is ∼ 30{--}50 {{Myr}} old. We analyze 11 months of 1 minute cadence data from Kepler, presenti... | [
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12409068 | 1607.03909 | The Evolution of Galaxy Number Density at z < 8 and Its Implications | The evolution of the number density of galaxies in the universe, and thus also the total number of galaxies, is a fundamental question with implications for a host of astrophysical problems including galaxy evolution and cosmology. However, there has never been a detailed study of this important measurement, nor a clea... | [
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1187815 | 1607.03412 | An innovative silicon photomultiplier digitizing camera for gamma-ray astronomy | The single-mirror small-size telescope (SST-1M) is one of the three proposed designs for the small-size telescopes (SSTs) of the Cherenkov Telescope Array (CTA) project. The SST-1M will be equipped with a 4 m-diameter segmented reflector dish and an innovative fully digital camera based on silicon photo-multipliers. Si... | [
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2775547 | 1607.01403 | H0LiCOW - IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology | Strong gravitational lenses with measured time delays between the multiple images allow a direct measurement of the time-delay distance to the lens, and thus a measure of cosmological parameters, particularly the Hubble constant, H<SUB>0</SUB>. We present a blind lens model analysis of the quadruply imaged quasar lens ... | [
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12511007 | 1607.04226 | Arrival times of gravitational radiation peaks for binary inspiral | Modeling of gravitational waves (GWs) from binary black hole inspiral brings together early post-Newtonian waveforms and late quasinormal ringing waveforms. Attempts to bridge the two limits without recourse to numerical relativity involve predicting the time of the peak GW amplitude. This prediction will require solvi... | [
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4842242 | 1607.06479 | The cold dark matter content of Galactic dwarf spheroidals: no cores, no failures, no problem | We examine the dark matter content of satellite galaxies in Lambda-CDM cosmological hydrodynamical simulations of the Local Group from the APOSTLE project. We find excellent agreement between simulation results and estimates for the 9 brightest Galactic dwarf spheroidals (dSphs) derived from their stellar velocity disp... | [
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12626389 | 1607.03540 | Binary neutron star mergers: a review of Einstein’s richest laboratory | In a single process, the merger of binary neutron star systems combines extreme gravity, the copious emission of gravitational waves, complex microphysics and electromagnetic processes, which can lead to astrophysical signatures observable at the largest redshifts. We review here the recent progress in understanding wh... | [
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"Graduate School of Science, Osaka University, Toyonaka, 560-0043, Japan",
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12593803 | 1607.03149 | The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Fourier space | We analyse the baryon acoustic oscillation (BAO) signal of the final Baryon Oscillation Spectroscopic Survey (BOSS) data release (DR12). Our analysis is performed in the Fourier space, using the power spectrum monopole and quadrupole. The data set includes 1198 006 galaxies over the redshift range 0.2 < z < 0.75.... | [
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"10.1093/mnras/stw2373",
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"Institute of Cosmology and Gravitation, Dennis Sciama Building, University of Portsmouth, Portsmouth PO1 3FX, UK; Lawrence Berkeley National Lab, 1 Cyclotron Rd, Berkeley, CA 94720, USA",
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12408270 | 1607.01290 | Caught in the Act: Direct Detection of Galactic Bars in the Buckling Phase | The majority of massive disk galaxies, including our own, have stellar bars with vertically thick inner region, known as “boxy/peanut-shaped” (B/P) bulges. The most commonly suggested mechanism for the formation of B/P bulges is a violent vertical “buckling” instability in the bar, something that has been seen in N-bod... | [
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-... | 10.250896 | 6.736901 | 2016-07-01 | 41 | 2016ApJ...825L..30E | [
"real galaxies",
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"stellar kinematic asymmetries",
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"two nearby galaxies",
"N-body simulations",
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"agreement",
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"galaxies: bulges",
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] | 12 | [
"10.3847/2041-8205/825/2/L30",
"10.48550/arXiv.1607.01290"
] | [
"Erwin, Peter",
"Debattista, Victor P."
] | [
"Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching, Germany ; Universitäts-Sternwarte München, Scheinerstrasse 1, D-81679 München, Germany;",
"Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK"
] | [
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12472902 | 1607.06365 | Viscous time lags between starburst and AGN activity | There is strong observational evidence indicating a time lag of order of some 100 Myr between the onset of starburst and AGN activity in galaxies. Dynamical time lags have been invoked to explain this. We extend this approach by introducing a viscous time lag the gas additionally needs to flow through the AGN's accreti... | [
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-... | 15.912522 | 7.675403 | 2016-07-01 | 9 | 2016MNRAS.462.2246B | [
"stellar velocity dispersion",
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"strong observational evidence",
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"the observed time lags",
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"Myr",
"order",
"a time lag",
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"a viscous time",
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"galaxies: active",
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"galaxies: nuclei",
"quasars: general",
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] | 2 | [
"10.1093/mnras/stw1804",
"10.48550/arXiv.1607.06365"
] | [
"Blank, Marvin",
"Duschl, Wolfgang J."
] | [
"Institut für Theoretische Physik und Astrophysik, Christian-Albrechts-Universität zu Kiel, Leibnizstr. 15, D-24118 Kiel, Germany",
"Institut für Theoretische Physik und Astrophysik, Christian-Albrechts-Universität zu Kiel, Leibnizstr. 15, D-24118 Kiel, Germany; Steward Observatory, The University of Arizona, 933... | [
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12472835 | 1607.06686 | The analemma criterion: accidental quasi-satellites are indeed true quasi-satellites | In the Solar system, a quasi-satellite is an object that follows a heliocentric path with an orbital period that matches almost exactly with that of a host body (planetary or not). The trajectory is of such nature that, without being gravitationally attached, the value of the angular separation between host and quasi-s... | [
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"satellite",
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"-",
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"geosynchronous orbits",
"quasi",
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"dwarf planet Pluto",
"its transient quasi-satellite status",
"the hosts sidereal orbital period",
"a host b... | [
"methods: numerical",
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"minor planets",
"asteroids: general",
"asteroids: individual: 15810 (1994 JR<SUB>1</SUB>)",
"asteroids: individual: 63252 (2001 BL<SUB>41</SUB>)",
"Astrophysics - Earth and Planetary Astrophysics"
] | 9 | [
"10.1093/mnras/stw1833",
"10.48550/arXiv.1607.06686"
] | [
"de la Fuente Marcos, C.",
"de la Fuente Marcos, R."
] | [
"Apartado de Correos 3413, E-28080 Madrid, Spain",
"Apartado de Correos 3413, E-28080 Madrid, Spain"
] | [
"2018MNRAS.473.3434D",
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12583834 | 1607.00775 | The magnetic part of the Weyl tensor, and the expansion of discrete universes | We examine the effect that the magnetic part of the Weyl tensor has on the large-scale expansion of space. This is done within the context of a class of cosmological models that contain regularly arranged discrete masses, rather than a continuous perfect fluid. The natural set of geodesic curves that one should use to ... | [
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... | 10.419729 | 0.264016 | 2016-07-01 | 16 | 2017GReGr..49...30C | [
"cosmological models",
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"the magnetic part",
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"values",
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"space",
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"a non-zero magnetic part",
"geodesic curves",
... | [
"Black holes",
"Cosmology",
"Silent universes",
"General Relativity and Quantum Cosmology",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 3 | [
"10.1007/s10714-017-2192-0",
"10.48550/arXiv.1607.00775"
] | [
"Clifton, Timothy",
"Gregoris, Daniele",
"Rosquist, Kjell"
] | [
"School of Physics and Astronomy, Queen Mary University of London, London, UK",
"Department of Mathematics and Statistics, Dalhousie University, Halifax, Canada",
"Department of Physics, Stockholm University, Stockholm, Sweden"
] | [
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12409147 | 1607.05961 | Projection Effects in Coronal Dimmings and Associated EUV Wave Event | We investigate the high-speed (v > 1000 km s<SUP>-1</SUP>) extreme-ultraviolet (EUV) wave associated with an X1.2 flare and coronal mass ejection (CME) from NOAA active region 11283 on 2011 September 6 (SOL2011-09-06T22:12). This EUV wave features peculiar on-disk signatures in particular, we observe an intermittent... | [
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"localized coronal dimming regions",
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"the enhanced EUV wave",
"MK"... | [
"Sun: activity",
"Sun: corona",
"Sun: coronal mass ejections: CMEs",
"Sun: flares",
"Astrophysics - Solar and Stellar Astrophysics"
] | 7 | [
"10.3847/0004-637X/830/2/92",
"10.48550/arXiv.1607.05961"
] | [
"Dissauer, K.",
"Temmer, M.",
"Veronig, A. M.",
"Vanninathan, K.",
"Magdalenić, J."
] | [
"IGAM/Institute of Physics, University of Graz, Universitätsplatz 5/II, A-8010 Graz, Austria",
"IGAM/Institute of Physics, University of Graz, Universitätsplatz 5/II, A-8010 Graz, Austria",
"IGAM/Institute of Physics, University of Graz, Universitätsplatz 5/II, A-8010 Graz, Austria; Kanzelhöhe Observatory/Insti... | [
"2017SoPh..292...93T",
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14122128 | 1607.02546 | Interpreting the cosmic far-infrared background anisotropies using a gas regulator model | Cosmic far-infrared background (CFIRB) is a powerful probe of the history of star formation rate (SFR) and the connection between baryons and dark matter across cosmic time. In this work, we explore to which extent the CFIRB anisotropies can be reproduced by a simple physical framework for galaxy evolution, the gas reg... | [
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... | 13.257123 | 7.083963 | 2016-07-01 | 9 | 2018MNRAS.475.3974W | [
"star formation rate",
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"gas ejection",
"cosmic time",
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"gas",
"dark matter",
"galaxy evolution",
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"Planck",
"CFIRB",
"continuity equations",
"baryons",
"ultraviolet and optical surveys",
... | [
"galaxies: haloes",
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"submillimetre: diffuse background",
"submillimetre: galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics",
"Astrophysics - Astrophysics of Galaxies"
] | 6 | [
"10.1093/mnras/sty071",
"10.48550/arXiv.1607.02546"
] | [
"Wu, Hao-Yi",
"Doré, Olivier",
"Teyssier, Romain",
"Serra, Paolo"
] | [
"California Institute of Technology, MC 367-17, Pasadena, CA 91125, USA; Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA;",
"California Institute of Technology, MC 367-17, Pasadena, CA 91125, USA; Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA",
"Institute for ... | [
"2016ApJ...833..153S",
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"2019A&A...621A..32M",
"2020ApJ...890..140S",
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12594106 | 1607.05199 | Gravitational wave signals from 3D neutrino hydrodynamics simulations of core-collapse supernovae | We present gravitational wave (GW) signal predictions from four 3D multigroup neutrino hydrodynamics simulations of core-collapse supernovae of progenitors with 11.2, 20 and 27 M<SUB>⊙</SUB>. GW emission in the pre-explosion phase strongly depends on whether the post-shock flow is dominated by the standing accretion sh... | [
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"PNS convection",
"PNS",
"2D models",
"convection",
"3D. Resonant excitation",
"mass motions",
"asymmetric mass motions",
"GW emission",
"the PNS convection zone",
"high-frequency surface g modes",
"smaller downflow velocities",
"enhanced low-frequency emission",
"high-frequency variability"... | [
"gravitational waves",
"hydrodynamics",
"instabilities",
"supernovae: general",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Solar and Stellar Astrophysics"
] | 18 | [
"10.1093/mnras/stx618",
"10.48550/arXiv.1607.05199"
] | [
"Andresen, H.",
"Müller, B.",
"Müller, E.",
"Janka, H. -Th."
] | [
"Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching, Germany; Physik Department, Technische Universität München, James-Franck-Str. 1, D-85748 Garching, Germany",
"Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK; Monash ... | [
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12408923 | 1607.02400 | GRB 090510: A Genuine Short GRB from a Binary Neutron Star Coalescing into a Kerr-Newman Black Hole | In a new classification of merging binary neutron stars (NSs) we separate short gamma-ray bursts (GRBs) into two subclasses. The ones with {E}<SUB>{iso</SUB>}≲ {10}<SUP>52</SUP> erg coalesce to form a massive NS and are indicated as short gamma-ray flashes (S-GRFs). The hardest, with {E}<SUB>{iso</SUB>}≳ {10}<SUP>52</S... | [
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-0... | 16.102983 | 0.608687 | 2016-07-01 | 21 | 2016ApJ...831..178R | [
"GeV emission",
"genuine short GRBs",
"GRBs",
"GRB",
"BH",
"E}<SUB>{iso</SUB>}=(3.95+/- 0.21)×",
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"The GeV emission",
"short gamma-ray bursts",
"short gamma-ray flashes",
"thermal spectra",
"binary neutron stars",
"their observed overall energetics",
"the prompt emission",
"E}<S... | [
"gamma-ray burst: general",
"gamma-ray burst: individual: GRB 090510",
"Astrophysics - High Energy Astrophysical Phenomena",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 9 | [
"10.3847/0004-637X/831/2/178",
"10.48550/arXiv.1607.02400"
] | [
"Ruffini, R.",
"Muccino, M.",
"Aimuratov, Y.",
"Bianco, C. L.",
"Cherubini, C.",
"Enderli, M.",
"Kovacevic, M.",
"Moradi, R.",
"Penacchioni, A. V.",
"Pisani, G. B.",
"Rueda, J. A.",
"Wang, Y."
] | [
"Dipartimento di Fisica, Sapienza Università di Roma and ICRA, Piazzale Aldo Moro 5, I-00185 Roma, Italy ; ICRANet, Piazza della Repubblica 10, I-65122 Pescara, Italy ; Université de Nice Sophia-Antipolis, Grand Château Parc Valrose, Nice, CEDEX 2, France ; ICRANet-Rio, Centro Brasileiro de Pesquisas Fisicas, Rua D... | [
"2016ApJ...832..136R",
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12472712 | 1607.07822 | Blazar flaring patterns (B-FlaP) classifying blazar candidate of uncertain type in the third Fermi-LAT catalogue by artificial neural networks | The Fermi-Large Area Telescope (LAT) is currently the most important facility for investigating the GeV γ-ray sky. With Fermi-LAT, more than three thousand γ-ray sources have been discovered so far. 1144 (∼40 per cent) of the sources are active galaxies of the blazar class, and 573 (∼20 per cent) are listed as blazar c... | [
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0.0... | 16.485292 | 4.53846 | 2016-07-01 | 48 | 2016MNRAS.462.3180C | [
"classification",
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"BCUs",
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"BCU",
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"ground-based optical observatories",
"Cherenkov"... | [
"methods: statistical",
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"gamma-rays: galaxies",
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] | 12 | [
"10.1093/mnras/stw1830",
"10.48550/arXiv.1607.07822"
] | [
"Chiaro, G.",
"Salvetti, D.",
"La Mura, G.",
"Giroletti, M.",
"Thompson, D. J.",
"Bastieri, D."
] | [
"Dip. Fisica and Astronomia G. Galilei - Università di Padova, I-35131 Padova, Italy",
"INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica, I-20133 Milano, Italy",
"Dip. Fisica and Astronomia G. Galilei - Università di Padova, I-35131 Padova, Italy",
"INAF-Institute of Radioastronomy, I-40129 Bologna, Ita... | [
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12471923 | 1607.06129 | Braking indices of pulsars obtained in the presence of an effective force | Braking indices of pulsars present a scientific challenge as their theoretical calculation is still an open problem. In this paper, we report results of a study regarding such calculation which adapts the canonical model (which admits that pulsars are rotating magnetic dipoles) basically by introducing a compensating c... | [
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"10.1093/mnras/stw1636",
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] | [
"Magalhaes, N. S.",
"Okada, A. S.",
"Frajuca, C."
] | [
"Department of Exact and Earth Sciences, Federal University of Sao Paulo Rua Sao Nicolau 210, Diadema, SP 09913-030, Brazil",
"Scientific Initiation Program, Federal University of Sao Paulo Rua Sao Nicolau 210, Diadema, SP 09913-030, Brazil",
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12595569 | 1607.01824 | The infrared-dark dust content of high redshift galaxies | We present a theoretical model aimed at explaining the IRX-β relation for high redshift (z ≳ 5) galaxies. Recent observations have shown that early Lyman-Break Galaxies, although characterized by a large ultraviolet (UV) attenuation (e.g. flat UV β slopes), show a striking far-infrared (FIR) deficit, I.e. they are `inf... | [
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"10.1093/mnras/stx1898",
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"Ferrara, A.",
"Hirashita, H.",
"Ouchi, M.",
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"Scuola Normale Superiore, Piazza dei Cavalieri 7, I-56126 Pisa, Italy; Kavli IPMU, WPI, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan",
"Institute of Astronomy and Astrophysics, Academia Sinica, No. 1, Sec. 4, Roosevelt Rd., Taipei 10617, Taiwan",
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12473132 | 1607.08591 | Tidal spin down rates of homogeneous triaxial viscoelastic bodies | We use numerical simulations to measure the sensitivity of the tidal spin-down rate of a homogeneous triaxial ellipsoid to its axis ratios by comparing the drift rate in orbital semimajor axis to that of a spherical body with the same mass, volume and simulated rheology. We use a mass-spring model approximating a visco... | [
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"10.1093/mnras/stw2094",
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] | [
"Quillen, Alice C.",
"Kueter-Young, Andrea",
"Frouard, Julien",
"Ragozzine, Darin"
] | [
"Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA",
"Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA; Physics Department, Siena College, Loudonville, NY 12211, USA,",
"US Naval Observatory, 3450 Massachusetts Ave NW, Washington DC 2039... | [
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5100913 | 1607.06773 | The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Implications for Spectral Line Intensity Mapping at Millimeter Wavelengths and CMB Spectral Distortions | We present direct estimates of the mean sky brightness temperature in observing bands around 99 and 242 GHz due to line emission from distant galaxies. These values are calculated from the summed line emission observed in a blind, deep survey for spectral line emission from high redshift galaxies using ALMA (the ALMA s... | [
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] | 9 | [
"10.3847/1538-4357/833/1/73",
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"Carilli, C. L.",
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"Wagg, J.",
"Popping, G.",
"Cortes, P.",
"Hodge, J.",
"Weiss, A.",
"Bertoldi, F.",
"Riechers, D."
] | [
"National Radio Astronomy Observatory, P.O. Box 0, Socorro, NM 87801, USA ; Astrophysics Group, Cavendish Laboratory, JJ Thomson Avenue, Cambridge CB3 0HE, UK;",
"Jodrell Bank Centre for Astrophysics, University of Manchester, Oxford Road, M13 9PL, UK",
"Max-Planck Institute for Astronomy, D-69117 Heidelberg, G... | [
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12434275 | 1607.01365 | Second order singular pertubative theory for gravitational lenses | The extension of the singular perturbative approach to the second order is presented in this paper. The general expansion to the second order is derived. The second order expansion is considered as a small correction to the first order expansion. Using this approach it is demonstrated that the second order expansion is... | [
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0.... | 12.600745 | 3.706642 | 2016-07-01 | 1 | 2016arXiv160701365A | [
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] | 3 | [
"10.48550/arXiv.1607.01365"
] | [
"Alard, C."
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"-"
] | [
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12593827 | 1607.07296 | Matter density perturbation and power spectrum in running vacuum model | We investigate the matter density perturbation δ<SUB>m</SUB> and power spectrum P(k) in the running vacuum model, with the cosmological constant being a function of the Hubble parameter, given by Λ = Λ<SUB>0</SUB> + 6σHH<SUB>0</SUB> + 3νH<SUP>2</SUP>, in which the linear and quadratic terms of H would originate from th... | [
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... | 10.913698 | 0.603303 | 2016-07-01 | 5 | 2017MNRAS.464.2462G | [
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"dark energy",
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] | 4 | [
"10.1093/mnras/stw2549",
"10.48550/arXiv.1607.07296"
] | [
"Geng, Chao-Qiang",
"Lee, Chung-Chi"
] | [
"Chongqing University of Posts and Telecommunications, Chongqing 400065, China; National Center for Theoretical Sciences, Hsinchu, Taiwan 30043, Republic of China; Department of Physics, National Tsing Hua University, Hsinchu, Taiwan 30013, Republic of China",
"National Center for Theoretical Sciences, Hsinchu, T... | [
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12408329 | 1607.02150 | Foreground Bias from Parametric Models of Far-IR Dust Emission | We use simple toy models of far-IR dust emission to estimate the accuracy to which the polarization of the cosmic microwave background can be recovered using multi-frequency fits, if the parametric form chosen for the fitted dust model differs from the actual dust emission. Commonly used approximations to the far-IR du... | [
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"cosmology: observations",
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] | 3 | [
"10.3847/0004-637X/826/2/101",
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] | [
"Kogut, A.",
"Fixsen, D. J."
] | [
"Code 665, Goddard Space Flight Center, Greenbelt, MD 20771, USA",
"Code 665, Goddard Space Flight Center, Greenbelt, MD 20771, USA; University of Maryland, College Park, MD 20742, USA"
] | [
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2426651 | 1607.00013 | ZFIRE: A KECK/MOSFIRE Spectroscopic Survey of Galaxies in Rich Environments at z ∼ 2 | We present an overview and the first data release of ZFIRE, a spectroscopic redshift survey of star-forming galaxies that utilizes the MOSFIRE instrument on Keck-I to study galaxy properties in rich environments at 1.5 < z < 2.5. ZFIRE measures accurate spectroscopic redshifts and basic galaxy properties derived ... | [
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"photometric redshifts",
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] | 18 | [
"10.3847/0004-637X/828/1/21",
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] | [
"Nanayakkara, Themiya",
"Glazebrook, Karl",
"Kacprzak, Glenn G.",
"Yuan, Tiantian",
"Tran, Kim-Vy",
"Spitler, Lee",
"Kewley, Lisa",
"Straatman, Caroline",
"Cowley, Michael",
"Fisher, David",
"Labbe, Ivo",
"Tomczak, Adam",
"Allen, Rebecca",
"Alcorn, Leo"
] | [
"Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia",
"Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia",
"Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawth... | [
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1797939 | 1607.03427 | Propeller Effect in the Transient X-Ray Pulsar SMC X-2 | We report the results of the monitoring campaign of the transient X-ray pulsar SMC X-2 performed with the Swift/XRT telescope over the period of 2015 September-2016 January during the Type II outburst. During this event, the bolometric luminosity of the source ranged from ≃10<SUP>39</SUP> down to several ×10<SUP>34</SU... | [
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] | 8 | [
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"Lutovinov, Alexander A.",
"Tsygankov, Sergey S.",
"Krivonos, Roman A.",
"Molkov, Sergey V.",
"Poutanen, Juri"
] | [
"Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia; Moscow Institute of Physics and Technology, Moscow region, Dolgoprudnyi, Russia",
"Tuorla Observatory, Department of Physics and Astronomy, University of Turku, Väisäläntie 20, FI-21500 Piikkiö, Finland",
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12409546 | 1607.08818 | An Opportunistic Search for Extraterrestrial Intelligence (SETI) with the Murchison Widefield Array | A spectral line image cube generated from 115 minutes of MWA data that covers a field of view of 400 sq, deg. around the Galactic Center is used to perform the first Search for ExtraTerrestrial Intelligence (SETI) with the Murchison Widefield Array (MWA). Our work constitutes the first modern SETI experiment at low rad... | [
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"Tingay, S. J.",
"Tremblay, C.",
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"International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, WA 6102, Australia ; Istituto di Radioastronomia, Istituto Nazionale di Astrofisica, I-40129 Bologna, Italy",
"International Centre for Radio Astronomy Research (ICRAR), Curtin University, Bentley, WA 6102, Australia",
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11492362 | 1607.06458 | Constraining the dark energy equation of state with H II galaxies | We use the H II galaxies L-σ relation and the resulting Hubble expansion cosmological probe of a sample of just 25 high-z (up to z ∼ 2.33) H II galaxies, in a joint likelihood analysis with other well tested cosmological probes (cosmic microwave background, CMB, Baryon Acoustic Oscillations, BAOs) in an attempt to cons... | [
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0... | 11.586074 | 1.305392 | 2016-07-01 | 64 | 2016MNRAS.462.2431C | [
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"Instituto Nacional de Astrofísica Óptica y Electrónica, AP 51 y 216, 72000 Puebla, México; Cavendish Laboratory, University of Cambridge, 19 J. J. Thomson Ave, Cambridge CB3 0HE, UK; Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK",
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2073369 | 1607.06172 | The Primordial Inflation Polarization Explorer (PIPER) | The Primordial Inflation Polarization ExploreR (PIPER) is a balloon-borne telescope designed to measure the polarization of the Cosmic Microwave Background on large angular scales. PIPER will map 85% of the sky at 200, 270, 350, and 600 GHz over a series of 8 conventional balloon flights from the northern and southern ... | [
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... | [
"Johns Hopkins Univ. (United States)",
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12408854 | 1607.06491 | Radiation and Polarization Signatures of the 3D Multizone Time-dependent Hadronic Blazar Model | We present a newly developed time-dependent three-dimensional multizone hadronic blazar emission model. By coupling a Fokker-Planck-based lepto-hadronic particle evolution code, 3DHad, with a polarization-dependent radiation transfer code, 3DPol, we are able to study the time-dependent radiation and polarization signat... | [
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"Zhang, Haocheng",
"Diltz, Chris",
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12500420 | 1607.00879 | Origin of the characteristic X-ray spectral variations of IRAS 13224-3809 | The narrow-line Seyfert 1 galaxy (NLS1) IRAS 13224-3809 is known to exhibit significant X-ray spectral variation, a sharp spectral drop at ∼7 keV, strong soft excess emission, and a hint of an iron L-edge feature, which is very similar to the NLS1 1H 0707-495. We have proposed the "Variable Double Partial Covering (VDP... | [
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"Yamasaki, Hiroki",
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