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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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-0.... | 9.992026 | 7.407736 | 2016-07-01 | 17 | 2016MNRAS.461.4335A | [
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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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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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0.... | 11.799792 | 3.5501 | 2016-07-01 | 8 | 2016ARep...60..563S | [
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"Astrophysics - Cosmology and Nongalactic Astrophysics",
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] | 3 | [
"10.1134/S1063772916040107",
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"Shirokov, S. I.",
"Lovyagin, N. Yu.",
"Baryshev, Yu. V.",
"Gorokhov, V. L."
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"Saint-Petersburg State University, St. Petersburg, Russia",
"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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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",
"Centro de Astrobiología (INTA-CSIC), Ctra de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, S... | [
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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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"galaxies: evolution",
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] | 12 | [
"10.1093/mnras/stx091",
"10.48550/arXiv.1607.08005"
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"Shimakawa, Rhythm",
"Kodama, Tadayuki",
"Shibuya, Takatoshi",
"Kashikawa, Nobunari",
"Tanaka, Ichi",
"Matsuda, Yuichi",
"Tadaki, Ken-ichi",
"Koyama, Yusei",
"Hayashi, Masao",
"Suzuki, Tomoko L.",
"Yamamoto, Moegi"
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"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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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 | [
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] | 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"
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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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] | 3 | [
"10.1051/0004-6361/201424904",
"10.48550/arXiv.1607.07723"
] | [
"Colafrancesco, S.",
"Marchegiani, P.",
"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",
"INAF-Osservatorio Astronomico di Roma via Frascati 33, 00040, Monteporzio, Italy; School of Physics, University of the Witwater... | [
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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",
"Tinker, Jeremy L.",
"Hahn, ChangHoon",
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"Tojeiro, Rita",
"Camacho, Hugo O.",
"Lima, Marcos",
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"Sobreira, Flavia",
"da Costa, Luiz N.",
"Bautista, Julian E.",
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"Comparat, Johan",
"Daws... | [
"Center for Cosmology and Particle Physics, Department of Physics, New York University, 4 Washington Place, New York, NY 10003, USA",
"Center for Cosmology and Particle Physics, Department of Physics, New York University, 4 Washington Place, New York, NY 10003, USA",
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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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] | 16 | [
"10.1093/mnras/stw2691",
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"Ferrero, Ismael",
"Navarro, Julio F.",
"Abadi, Mario G.",
"Sales, Laura V.",
"Bower, Richard G.",
"Crain, Robert A.",
"Frenk, Carlos S.",
"Schaller, Matthieu",
"Schaye, Joop",
"Theuns, Tom"
] | [
"Instituto de Astronomía Teórica y Experimental, CONICET-UNC, Laprida 854, X5000BGR, Córdoba, Argentina; Observatorio Astronómico de Córdoba, Universidad Nacional de Córdoba, Laprida 854, X5000BGR, Córdoba, Argentina",
"Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P 5C2, Canada",
... | [
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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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"metal cooling",
... | [
"methods: numerical",
"ISM: clouds",
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"galaxies: evolution",
"galaxies: ISM",
"galaxies: star formation",
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] | 5 | [
"10.1093/mnras/stw1741",
"10.48550/arXiv.1607.05795"
] | [
"Benincasa, S. M.",
"Wadsley, J.",
"Couchman, H. M. P.",
"Keller, B. W."
] | [
"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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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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] | 10 | [
"10.3847/0004-637X/832/1/39",
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"Lu, Yi",
"Yang, Xiaohu",
"Shi, Feng",
"Mo, H. J.",
"Tweed, Dylan",
"Wang, Huiyuan",
"Zhang, Youcai",
"Li, Shijie",
"Lim, S. H."
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"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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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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"methods: data analysis",
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] | 3 | [
"10.1093/mnras/stx894",
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"Hahn, ChangHoon",
"Vakili, Mohammadjavad",
"Walsh, Kilian",
"Hearin, Andrew P.",
"Hogg, David W.",
"Campbell, Duncan"
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"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",
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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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"10.1093/mnrasl/slx022",
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"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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"... | [
"galaxies: evolution",
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] | 6 | [
"10.1093/mnras/stw1655",
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"Suzuki, T. L.",
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"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... | [
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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",
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"10.3847/0004-637X/830/2/93",
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"Ji, Alexander P.",
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"Simon, Joshua D.",
"Chiti, Anirudh"
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"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;",
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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 | [
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] | 5 | [
"10.3847/0004-6256/152/3/72",
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"Laine, Seppo",
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"Martínez-Delgado, David",
"Ashby, Matthew L. N.",
"Davies, James E.",
"Majewski, Stephen R.",
"Brodie, Jean P.",
"GaBany, R. Jay",
"Arnold, Jacob A."
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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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"the total number density",
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"mass function",
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] | 78 | [
"10.3847/0004-637X/830/2/83",
"10.48550/arXiv.1607.03909"
] | [
"Conselice, Christopher J.",
"Wilkinson, Aaron",
"Duncan, Kenneth",
"Mortlock, Alice"
] | [
"University of Nottingham, School of Physics & Astronomy, Nottingham, NG7 2RD, UK",
"University of Nottingham, School of Physics & Astronomy, Nottingham, NG7 2RD, UK",
"University of Nottingham, School of Physics & Astronomy, Nottingham, NG7 2RD, UK",
"University of Nottingham, School of Physics &... | [
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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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"measured time delays",
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"quasar lens",
"deep Hubble Space Telescope imaging",
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"GRAvItational Lenses",
"updated time-delay measurements",
"H0LiCOW",
"sight",
"Hubble",
"nearby perturbers",
"COSMOGRAIL",
"cosmological parameters",
"Keck data",
"... | [
"gravitational lensing: strong",
"cosmological parameters",
"distance scale",
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] | 28 | [
"10.1093/mnras/stw3077",
"10.48550/arXiv.1607.01403"
] | [
"Wong, Kenneth C.",
"Suyu, Sherry H.",
"Auger, Matthew W.",
"Bonvin, Vivien",
"Courbin, Frederic",
"Fassnacht, Christopher D.",
"Halkola, Aleksi",
"Rusu, Cristian E.",
"Sluse, Dominique",
"Sonnenfeld, Alessandro",
"Treu, Tommaso",
"Collett, Thomas E.",
"Hilbert, Stefan",
"Koopmans, Leon V.... | [
"National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; Institute of Astronomy and Astrophysics, Academia Sinica (ASIAA), PO Box 23-141, Taipei 10617, Taiwan",
"Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching, Germany; Institute of Astronomy and A... | [
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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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] | 33 | [
"10.1093/mnras/stw2373",
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"Beutler, Florian",
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"Chuang, Chia-Hsun",
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"Grieb, Jan Niklas",
"Hand, Nick",
"Kitaura, Francisco-Shu",
"M... | [
"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",
"Department of Physics and Astronomy, Ohio University, 251B Clippinger Labs, Athens, OH 45701, USA",
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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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] | 6 | [
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"Wu, Hao-Yi",
"Doré, Olivier",
"Teyssier, Romain",
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"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",
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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 | [
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"Carilli, C. L.",
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"Hodge, J.",
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"Bertoldi, F.",
"Riechers, D."
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"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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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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"Straatman, Caroline",
"Cowley, Michael",
"Fisher, David",
"Labbe, Ivo",
"Tomczak, Adam",
"Allen, Rebecca",
"Alcorn, Leo"
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"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",
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12473004 | 1607.00951 | Accretion of pristine gas and dilution during the formation of multiple-population globular clusters | We study the interaction of the early spherical GC wind powered by Type II supernovae (SNe II) with the surrounding ambient medium consisting of the gaseous disc of a star-forming galaxy at redshift z ≳ 2. The bubble formed by the wind eventually breaks out of the disc, and most of the wind moves directly out of the ga... | [
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"D'Ercole, A.",
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"INAF, Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna, Italy",
"INAF, Osservatorio Astronomico di Roma, Via Frascati 33, I-00040 Monteporzio Catone (Roma), Italy",
"Department of Astronomy, Indiana University, Swain West, 727 E. 3rd Street, Bloomington, IN 47405 USA"
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2409424 | 1607.02059 | HIRAX: a probe of dark energy and radio transients | The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) is a new 400{800MHz radio interferometer under development for deployment in South Africa. HIRAX will comprise 1024 six meter parabolic dishes on a compact grid and will map most of the southern sky over the course of four years. HIRAX has two primary sci... | [
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... | 12.410657 | 3.229301 | 2016-07-01 | 211 | 2016SPIE.9906E..5XN | [
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] | 11 | [
"10.1117/12.2234286",
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"Gupta, N.",
"Hilton, M.",
"Johnstone, B.",
"Karastergiou, A.",
"Kunz, M.",
"Lokhorst, D.",
"Maa... | [
"Univ. of Toronto (Canada)",
"West Virginia Univ. (United States)",
"APC, Univ. Paris Diderot, CNRS (France)",
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"National Institute for Theoretical Physics (South Africa)",
"McGill Univ. (Canada)",
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12408793 | 1607.00380 | High-energy Neutrinos from Sources in Clusters of Galaxies | High-energy cosmic rays can be accelerated in clusters of galaxies, by mega-parsec scale shocks induced by the accretion of gas during the formation of large-scale structures, or by powerful sources harbored in clusters. Once accelerated, the highest energy particles leave the cluster via almost rectilinear trajectorie... | [
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... | 5.822984 | 0.014759 | 2016-07-01 | 31 | 2016ApJ...828...37F | [
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"high-energy cosmic rays",
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"astroparticle physics",
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] | 2 | [
"10.3847/0004-637X/828/1/37",
"10.48550/arXiv.1607.00380"
] | [
"Fang, Ke",
"Olinto, Angela V."
] | [
"University of Maryland, Department of Astronomy, 1105 PSC, College Park, MD 20742, USA ; Joint Space-Science Institute, College Park, MD 20742, USA",
"Department of Astronomy & Astrophysics, Kavli Institute for Cosmological Physics, The University of Chicago, Chicago, Illinois 60637, USA"
] | [
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1622440 | 1607.07934 | Satellite quenching time-scales in clusters from projected phase space measurements matched to simulated orbits | We measure the star formation quenching efficiency and time-scale in cluster environments. Our method uses N-body simulations to estimate the probability distribution of possible orbits for a sample of observed Sloan Digital Sky Survey galaxies in and around clusters based on their position and velocity offsets from th... | [
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"galaxies: clusters: general",
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] | 13 | [
"10.1093/mnras/stw2195",
"10.48550/arXiv.1607.07934"
] | [
"Oman, Kyle A.",
"Hudson, Michael J."
] | [
"Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P 5C2, Canada; Department of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, Canada",
"Department of Physics and Astronomy, University of Waterloo, Waterloo, ON N2L 3G1, Canada; Perimeter Institute for Theoretical Ph... | [
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12408731 | 1607.04674 | Merger Hydrodynamics of the Luminous Cluster RX J1347.5-1145 | We present an analysis of the complex gas hydrodynamics in the X-ray-luminous galaxy cluster RX J1347.5-1145 caught in the act of merging with a subcluster to its southeast using a combined 186 ks Chandra exposure, 2.5 times greater than previous analyses. The primary cluster hosts a sloshing cold front spiral traced b... | [
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... | 13.647049 | 4.86576 | 2016-07-01 | 12 | 2016ApJ...830...39K | [
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"the subcluster infall shock",
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"galaxies: clusters: general",
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"galaxies: interactions",
"X-rays: galaxies: clusters",
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] | 6 | [
"10.3847/0004-637X/830/1/39",
"10.48550/arXiv.1607.04674"
] | [
"Kreisch, C. D.",
"Machacek, M. E.",
"Jones, C.",
"Randall, S. W."
] | [
"Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, D-85748 Garching bei München, Germany; Department of Physics, Washington University in St. Louis, One Brookings Drive, St. Louis, MO 63130, USA;",
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
"Har... | [
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12520904 | 1607.04218 | Self-consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations | The ultraviolet background (UVB) emitted by quasars and galaxies governs the ionization and thermal state of the intergalactic medium (IGM), regulates the formation of high-redshift galaxies, and is thus a key quantity for modeling cosmic reionization. The vast majority of cosmological hydrodynamical simulations implem... | [
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"Astrophysics - Instrumentation and Methods for Astro... | 11 | [
"10.3847/1538-4357/aa6031",
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] | [
"Oñorbe, Jose",
"Hennawi, Joseph F.",
"Lukić, Zarija"
] | [
"Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany",
"Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany",
"Lawrence Berkeley National Laboratory, Berkeley, CA 94720-8139, USA"
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3330704 | 1607.02787 | NIBLES: an H I census of stellar mass selected SDSS galaxies. I. The Nançay H I survey | To investigate galaxy properties as a function of their total stellar mass, we obtained 21 cm H I line observations at the 100-m class Nançay Radio Telescope of 2839 galaxies from the Sloan Digital Sky Survey (SDSS) in the Local Volume (900 < cz < 12 000 km s<SUP>-1</SUP>), dubbed the Nançay Interstellar Baryons ... | [
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] | 25 | [
"10.1051/0004-6361/201528048",
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"Hallet, N.",
"Joseph, T.",
"Kotze, P.",
"Kraan-Korteweg, R. C.",
"Olofsson, A. O. H.",
"Ramatsoku, M."
] | [
"GEPI, Observatoire de Paris, CNRS, Université Paris Diderot, 5 place Jules Janssen, 92190, Meudon, France ; Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU USR 704, Université d'Orléans OSUC, route de Souesmes, 18330, Nançay, France",
"University of Massachusetts, Astronomy Program, 536 LG... | [
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2414370 | 1607.03674 | High-velocity extended molecular outflow in the star-formation dominated luminous infrared galaxy ESO 320-G030 | We analyze new high spatial resolution (~60 pc) ALMA CO(2-1) observations of the isolated luminous infrared galaxy ESO 320-G030 (d = 48 Mpc) in combination with ancillary Hubble Space Telescope optical and near infrared (IR) imaging, as well as VLT/SINFONI near-IR integral field spectroscopy. We detect a high-velocity ... | [
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] | 10 | [
"10.1051/0004-6361/201628875",
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"Pereira-Santaella, M.",
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"García-Burillo, S.",
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"Cazzoli, S.",
"Emonts, B.",
"Piqueras López, J.",
"Planesas, P.",
"Storchi Bergmann, T.",
"Usero, A.",
"Villar-Martín, M."
] | [
"Centro de Astrobiología (CSIC/INTA), Ctra de Torrejón a Ajalvir, km 4, 28850, Torrejón de Ardoz, Madrid, Spain; ASTRO-UAM, UAM, Unidad Asociada CSIC, 28049, Madrid, Spain; Department of Physics, University of Oxford, Keble Road, Oxford, OX1 3RH, UK",
"Centro de Astrobiología (CSIC/INTA), Ctra de Torrejón a Ajalv... | [
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13975199 | 1607.06098 | Constraining the baryon-dark matter relative velocity with the large-scale three-point correlation function of the SDSS BOSS DR12 CMASS galaxies | We search for a galaxy clustering bias due to a modulation of galaxy number with the baryon-dark matter relative velocity resulting from recombination-era physics. We find no detected signal and place the constraint b<SUB>v</SUB> < 0.01 on the relative velocity bias for the CMASS galaxies. This bias is an important ... | [
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0.00916... | 12.322242 | 2.464336 | 2016-07-01 | 47 | 2018MNRAS.474.2109S | [
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] | 7 | [
"10.1093/mnras/stx2723",
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"Slepian, Zachary",
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"Ross, Ashley J.",
"Rossi, Graziano",
"Seo, Hee-Jong",
"Slosar, Anže",
"... | [
"Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA",
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12408761 | 1607.08616 | Empirically Constrained Predictions for Metal-line Emission from the Circumgalactic Medium | The circumgalactic medium (CGM) is one of the remaining least constrained components of galaxies and as such has significant potential for advancing galaxy formation theories. In this work, we vary the extragalactic ultraviolet background for a high-resolution cosmological simulation of a Milky-Way-like galaxy and exam... | [
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0.... | 13.353544 | 8.166255 | 2016-07-01 | 26 | 2016ApJ...827..148C | [
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] | 10 | [
"10.3847/0004-637X/827/2/148",
"10.48550/arXiv.1607.08616"
] | [
"Corlies, Lauren",
"Schiminovich, David"
] | [
"Department of Astronomy, Columbia University, New York, NY 10027, USA",
"Department of Astronomy, Columbia University, New York, NY 10027, USA"
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12472551 | 1607.06466 | The supermassive black hole and double nucleus of the core elliptical NGC 5419 | We obtained adaptive-optics assisted SINFONI observations of the central regions of the giant elliptical galaxy NGC 5419 with a spatial resolution of 0.2 arcsec (≈55 pc). NGC 5419 has a large depleted stellar core with a radius of 1.58 arcsec (430 pc). HST and SINFONI images show a point source located at the galaxy's ... | [
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] | 3 | [
"10.1093/mnras/stw1802",
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] | [
"Mazzalay, Ximena",
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"Saglia, Roberto P.",
"Wegner, Gary A.",
"Bender, Ralf",
"Erwin, Peter",
"Fabricius, Maximilian H.",
"Rusli, Stephanie P."
] | [
"Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany",
"Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, D-85741 Garching, Germany; Universitätssternwarte, Scheinerstrasse 1, D-81679 München, Germany",
"Max-Planck-Institut für extraterrestrische Physik, P... | [
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2301789 | 1607.07710 | VLA and ALMA Imaging of Intense Galaxy-wide Star Formation in z ∼ 2 Galaxies | We present ≃0.″4 resolution extinction-independent distributions of star formation and dust in 11 star-forming galaxies (SFGs) at z = 1.3-3.0. These galaxies are selected from sensitive blank-field surveys of the 2‧ × 2‧ Hubble Ultra-Deep Field at λ = 5 cm and 1.3 mm using the Karl G. Jansky Very Large Array and Atacam... | [
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"stellar masses",
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"z",
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"galaxies: active",
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"Astrophysics - Astrophysics of Galaxies",
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] | 9 | [
"10.3847/0004-637X/833/1/12",
"10.48550/arXiv.1607.07710"
] | [
"Rujopakarn, W.",
"Dunlop, J. S.",
"Rieke, G. H.",
"Ivison, R. J.",
"Cibinel, A.",
"Nyland, K.",
"Jagannathan, P.",
"Silverman, J. D.",
"Alexander, D. M.",
"Biggs, A. D.",
"Bhatnagar, S.",
"Ballantyne, D. R.",
"Dickinson, M.",
"Elbaz, D.",
"Geach, J. E.",
"Hayward, C. C.",
"Kirkpatri... | [
"Kavli Institute for the Physics and Mathematics of the universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan ; Department of Physics, Faculty of Science, Chulalongkorn University, 254 Phayathai Road, Pathumwan, Bangkok 10330, Thailand;",
"I... | [
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"2005MNRAS.363..... |
12406323 | 1607.08623 | Constraining dust extinction properties via the VVV survey | Near-infrared color-excess and extinction ratios are essential for establishing the cosmic distance scale and probing the Galaxy, particularly when analyzing targets attenuated by significant dust. A robust determination of those ratios followed from leveraging new infrared observations from the VVV survey, wherein num... | [
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"increasing Galactocentric distance",
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"dust",
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] | 2 | [
"10.1051/0004-6361/201628763",
"10.48550/arXiv.1607.08623"
] | [
"Majaess, D.",
"Turner, D.",
"Dékány, I.",
"Minniti, D.",
"Gieren, W."
] | [
"Mount Saint Vincent University, Halifax, NS B3M 2J6, Canada ; Department of Astronomy & Physics, Saint Mary's University, Halifax, NS, B3H 3C3, Canada",
"Department of Astronomy & Physics, Saint Mary's University, Halifax, NS, B3H 3C3, Canada",
"Astronomisches Rechen-Institut, Zentrum für Astronomie de... | [
"2016ApJ...830L..14M",
"2017A&A...605A.100B",
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12594074 | 1607.03127 | The stellar mass-halo mass relation of isolated field dwarfs: a critical test of ΛCDM at the edge of galaxy formation | We fit the rotation curves of isolated dwarf galaxies to directly measure the stellar mass-halo mass relation (M<SUB>⋆</SUB>-M<SUB>200</SUB>) over the mass range 5 × 10<SUP>5</SUP> ≲ M<SUB>⋆</SUB>/M<SUB>⊙</SUB> ≲ 10<SUP>8</SUP>. By accounting for cusp-core transformations due to stellar feedback, we find a monotonic re... | [
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"M",
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"10.1093/mnras/stx147",
"10.48550/arXiv.1607.03127"
] | [
"Read, J. I.",
"Iorio, G.",
"Agertz, O.",
"Fraternali, F."
] | [
"Department of Physics, University of Surrey, Guildford, GU2 7XH, Surrey, UK",
"Dipartimento di Fisica e Astronomia, Università di Bologna, Viale Berti Pichat 6/2, I-40127, Bologna, Italy; INAF - Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127, Bologna, Italy",
"Department of Physics, University of ... | [
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12473126 | 1607.04641 | A M ≳ 3 shock in `El Gordo' cluster and the origin of the radio relic | We present an X-ray and radio study of the famous `El Gordo', a massive and distant (z = 0.87) galaxy cluster. In the deep (340 ks) Chandra observation, the cluster appears with an elongated and cometary morphology, a sign of its current merging state. The GMRT radio observations at 610 MHz confirm the presence of a ra... | [
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"shock waves",
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"Astrophysics - High Energy Astrophysical Phenomena",
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] | 14 | [
"10.1093/mnras/stw2089",
"10.48550/arXiv.1607.04641"
] | [
"Botteon, A.",
"Gastaldello, F.",
"Brunetti, G.",
"Kale, R."
] | [
"Dipartimento di Fisica e Astronomia, Università di Bologna, via C. Ranzani 1, I-40127 Bologna, Italy; INAF - IRA, via P. Gobetti 101, I-40129 Bologna, Italy",
"INAF - IASF Milano, via E. Bassini 15, I-20133 Milano, Italy",
"INAF - IRA, via P. Gobetti 101, I-40129 Bologna, Italy",
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12593541 | 1607.07166 | Lyman α radiation hydrodynamics of galactic winds before cosmic reionization | The dynamical impact of Lyman α (Lyα) radiation pressure on galaxy formation depends on the rate and duration of momentum transfer between Lyα photons and neutral hydrogen gas. Although photon trapping has the potential to multiply the effective force, ionizing radiation from stellar sources may relieve the Lyα pressur... | [
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... | 13.618917 | 6.39726 | 2016-07-01 | 37 | 2017MNRAS.464.2963S | [
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"galaxies: formation",
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"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.1093/mnras/stw2591",
"10.48550/arXiv.1607.07166"
] | [
"Smith, Aaron",
"Bromm, Volker",
"Loeb, Abraham"
] | [
"Department of Astronomy, The University of Texas at Austin, Austin, TX 78712, USA",
"Department of Astronomy, The University of Texas at Austin, Austin, TX 78712, USA",
"Department of Astronomy, Harvard University, 60 Garden Street, Cambridge, MA 02138, USA"
] | [
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12409336 | 1607.02119 | Strong-lensing Analysis of the Powerful Lensing Cluster MACS J2135.2-0102 (z = 0.33) | We present a light-traces-mass (LTM) strong-lensing model of the massive lensing cluster MACS J2135.2-0102 (z = 0.33 hereafter MACS2135), known in part for hosting the cosmic eye galaxy lens. MACS2135 is also known to multiply lens a z = 2.3 sub-millimeter galaxy near the brightest cluster galaxy (BCG), as well as a pr... | [
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"dark matter",
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] | 4 | [
"10.3847/0004-637X/833/1/25",
"10.48550/arXiv.1607.02119"
] | [
"Zitrin, Adi",
"Broadhurst, Tom"
] | [
"Cahill Center for Astronomy and Astrophysics, California Institute of Technology, MC 249-17, Pasadena, CA 91125, USA ; Physics Department, Ben-Gurion University of the Negev, P.O. Box 653, Be'er-Sheva 84105, Israel ;;",
"Department of Theoretical Physics, University of Basque Country UPV/EHU, Bilbao, Spain ; IKE... | [
"2017ApJ...834...45Z",
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3778370 | 1607.03486 | Simulating galaxy formation with black hole driven thermal and kinetic feedback | The inefficiency of star formation in massive elliptical galaxies is widely believed to be caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas. Achieving a sufficiently rapid reddening of moderately massive galaxies without expelling too many baryons has however proven difficult for ... | [
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"massive elliptical galaxies",
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"supermassive black holes",
"large haloes",
"thermodynamic profiles",
"previous work",
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"AGN",
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"black hole physics",
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] | 108 | [
"10.1093/mnras/stw2944",
"10.48550/arXiv.1607.03486"
] | [
"Weinberger, Rainer",
"Springel, Volker",
"Hernquist, Lars",
"Pillepich, Annalisa",
"Marinacci, Federico",
"Pakmor, Rüdiger",
"Nelson, Dylan",
"Genel, Shy",
"Vogelsberger, Mark",
"Naiman, Jill",
"Torrey, Paul"
] | [
"Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany",
"Heidelberg Institute for Theoretical Studies, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany; Zentrum für Astronomie der Universität Heidelberg, ARI, Mönchhofstr. 12-14, D-69120 Heidelberg, Germany",... | [
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1497674 | 1607.03679 | The role of gas infall in the evolution of disc galaxies | Spiral galaxies are thought to acquire their gas through a protracted infall phase resulting in the inside-out growth of their associated discs. For field spirals, this infall occurs in the lower density environments of the cosmic web. The overall infall rate, as well as the galactocentric radius at which this infall i... | [
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"disc galaxy formation",
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"galaxies",
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"galaxies: formation",
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] | 11 | [
"10.1093/mnras/stw1723",
"10.48550/arXiv.1607.03679"
] | [
"Mollá, Mercedes",
"Díaz, Ángeles I.",
"Gibson, Brad K.",
"Cavichia, Oscar",
"López-Sánchez, Ángel-R."
] | [
"Departamento de Investigación Básica, CIEMAT, Avda. Complutense 40, E-28040 Madrid, Spain",
"Universidad Autónoma de Madrid, E-28049 Madrid, Spain; Astro-UAM, Unidad Asociada CSIC, Universidad Autónoma de Madrid, E-28049 Madrid, Spain",
"E.A. Milne Centre for Astrophysics, University of Hull, Hull HU6 7RX, Uni... | [
"2016arXiv161203348M",
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12511041 | 1607.05232 | Multitracing anisotropic non-Gaussianity with galaxy shapes | Correlations between intrinsic galaxy shapes on large scales arise due to the effect of the tidal field of the large-scale structure. Anisotropic primordial non-Gaussianity induces a distinct scale-dependent imprint in these tidal alignments on large scales. Motivated by the observational finding that the alignment str... | [
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"large scales",
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"two different shape estimators",
"a distinc... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics",
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] | 10 | [
"10.1103/PhysRevD.94.123507",
"10.48550/arXiv.1607.05232"
] | [
"Chisari, Nora Elisa",
"Dvorkin, Cora",
"Schmidt, Fabian",
"Spergel, David N."
] | [
"Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, United Kingdom",
"Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA",
"Max-Planck-Institute for Astrophysics, D-85748 Garching, Germany",
"Department of Astrophysical Sciences, Prin... | [
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12620768 | 1607.01761 | Looking through the same lens: Shear calibration for LSST, Euclid, and WFIRST with stage 4 CMB lensing | The next-generation weak lensing surveys (i.e., LSST, Euclid, and WFIRST) will require exquisite control over systematic effects. In this paper, we address shear calibration and present the most realistic forecast to date for LSST/Euclid/WFIRST and CMB lensing from a stage 4 CMB experiment ("CMB S4"). We use the cosmol... | [
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... | 12.285607 | 3.416112 | 2016-07-01 | 75 | 2017PhRvD..95l3512S | [
"most tomographic bins",
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... | [
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"Princeton University, Peyton Hall, Princeton, New Jersey 08544, USA",
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12409019 | 1607.05281 | Sizing Up the Milky Way: A Bayesian Mixture Model Meta-analysis of Photometric Scale Length Measurements | The exponential scale length (L <SUB> d </SUB>) of the Milky Way’s (MW’s) disk is a critical parameter for describing the global physical size of our Galaxy, important both for interpreting other Galactic measurements and helping us to understand how our Galaxy fits into extragalactic contexts. Unfortunately, current e... | [
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12435945 | 1607.05762 | The Effect of Nearby Voids on Galaxy Number Counts | The size, shape and degree of emptiness of void interiors sheds light on the details of galaxy formation. A particularly interesting question is whether void interiors are completely empty or contain a dwarf population. However the nearby voids that are most conducive for dwarf searches have large angular diameters, on... | [
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2774738 | 1607.03144 | The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: angular clustering tomography and its cosmological implications | We investigate the cosmological implications of studying galaxy clustering using a tomographic approach applied to the final Baryon Oscillation Spectroscopic Survey (BOSS) DR12 galaxy sample, including both auto- and cross-correlation functions between redshift shells. We model the signal of the full shape of the angul... | [
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"Universitäts-Sternwarte München, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, D-81679 Munich, Germany; Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, Giessenbachstr, D-85741 Garching, Germany",
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3811176 | 1607.01188 | Machine-learning identification of galaxies in the WISE × SuperCOSMOS all-sky catalogue | Context. The two currently largest all-sky photometric datasets, WISE and SuperCOSMOS, have been recently cross-matched to construct a novel photometric redshift catalogue on 70% of the sky. Galaxies were separated from stars and quasars through colour cuts, which may leave imperfections because different source types ... | [
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12408700 | 1607.07545 | Cosmic Shear Measurement Using Auto-convolved Images | We study the possibility of using quadrupole moments of auto-convolved galaxy images to measure cosmic shear. The autoconvolution of an image corresponds to the inverse Fourier transformation of its power spectrum. The new method has the following advantages: the smearing effect due to the point-spread function (PSF) c... | [
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"Li, Xiangchong",
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"Center for Astronomy and Astrophysics, Department of Physics and Astronomy, Shanghai Jiao Tong University, 955 Jianchuan road, Shanghai, 200240, China"
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2614419 | 1607.03636 | Sardinia Radio Telescope wide-band spectral-polarimetric observations of the galaxy cluster 3C 129 | We present new observations of the galaxy cluster 3C 129 obtained with the Sardinia Radio Telescope in the frequency range 6000-7200 MHz, with the aim to image the large-angular-scale emission at high-frequency of the radio sources located in this cluster of galaxies. The data were acquired using the recently commissio... | [
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1576892 | 1607.07190 | Oxygen abundance maps of CALIFA galaxies | We construct maps of the oxygen abundance distribution across the discs of 88 galaxies using Calar Alto Legacy Integral Field Area survey (CALIFA) Data Release 2 (DR2) spectra. The position of the centre of a galaxy (coordinates on the plate) was also taken from the CALIFA DR2. The galaxy inclination, the position angl... | [
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"Main Astronomical Observatory of National Academy of Sciences of Ukraine, 27 Zabolotnogo Str., 03680 Kiev, Ukraine; Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12-14, D-69120 Heidelberg, Germany",
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12406376 | 1607.04193 | Spectral clustering for optical confirmation and redshift estimation of X-ray selected galaxy cluster candidates in the SDSS Stripe 82 | We develop a galaxy cluster finding algorithm based on spectral clustering technique to identify optical counterparts and estimate optical redshifts for X-ray selected cluster candidates. As an application, we run our algorithm on a sample of X-ray cluster candidates selected from the third XMM-Newton serendipitous sou... | [
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] | 6 | [
"10.1016/j.ascom.2016.07.001",
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"Mahmoud, E.",
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"Shoukry, A."
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"Egypt-Japan University of Science and Technology (E-JUST), 21934 New Borg El-Arab, Alexandria, Egypt; National Research Institute of Astronomy and Geophysics (NRIAG), 11421 Helwan, Cairo, Egypt",
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1950511 | 1607.01019 | Galaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift bias | The majority of galaxies in the local Universe exhibit spiral structure with a variety of forms. Many galaxies possess two prominent spiral arms, some have more, while others display a many-armed flocculent appearance. Spiral arms are associated with enhanced gas content and star formation in the discs of low-redshift ... | [
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"Nichol, Robert C.",
"Rosslowe, Christopher K.",
"Simmons, Brooke D.",
"Smethurst, Rebecca J."
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"School of Physics and Astronomy, The University of Nottingham, University Park, Nottingham NG7 2RD, UK",
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1917404 | 1607.05903 | Improving lensing cluster mass estimate with flexion | Gravitational lensing has long been considered as a valuable tool to determine the total mass of galaxy clusters. The shear profile, as inferred from the statistics of ellipticity of background galaxies, allows us to probe the cluster intermediate and outer regions, thus determining the virial mass estimate. However, t... | [
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"Cardone, V. F.",
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"Er, X.",
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12473219 | 1607.02768 | Relating information entropy and mass variance to measure bias and non-Gaussianity | We relate the information entropy and the mass variance of any distribution in the regime of small fluctuations. We use a set of Monte Carlo simulations of different homogeneous and inhomogeneous distributions to verify the relation and also test it in a set of cosmological N-body simulations. We find that the relation... | [
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] | 7 | [
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] | [
"Pandey, Biswajit"
] | [
"Department of Physics, Visva-Bharati University, Santiniketan, Birbhum 731235, India"
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12517528 | 1607.00044 | Analysis of a custom support vector machine for photometric redshift estimation and the inclusion of galaxy shape information | <BR /> Aims: We present a custom support vector machine classification package for photometric redshift estimation, including comparisons with other methods. We also explore the efficacy of including galaxy shape information in redshift estimation. Support vector machines, a type of machine learning, utilize optimizati... | [
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"10.1051/0004-6361/201629558",
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"Jones, E.",
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] | [
"Physics Department, University of Richmond 28 Westhampton Way, University of Richmond, VA 23173, USA",
"Physics Department, University of Richmond 28 Westhampton Way, University of Richmond, VA 23173, USA"
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1345181 | 1607.02331 | SXDF-ALMA 2 arcmin<SUP>2</SUP> deep survey: Resolving and characterizing the infrared extragalactic background light down to 0.5 mJy | We present a multiwavelength analysis of five submillimeter sources (S<SUB>1.1mm</SUB> = 0.54-2.02 mJy) that were detected during our 1.1 mm deep continuum survey in the Subaru/XMM-Newton Deep Survey Field (SXDF)-UDS-CANDELS field (2 arcmin<SUP>2</SUP>, 1σ = 0.055 mJy beam<SUP>-1</SUP>) using the Atacama Large Millimet... | [
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"Matsuda, Yuichi",
... | [
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"Institute of Astronomy, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan",
"Institute of Astronomy, The University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan; Research Center for the E... | [
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4298348 | 1607.02511 | Far-infrared Line Spectra of Active Galaxies from the Herschel/PACS Spectrometer: The Complete Database | We present a coherent database of spectroscopic observations of far-IR fine-structure lines from the Herschel/Photoconductor Array Camera and Spectrometer archive for a sample of 170 local active galactic nuclei (AGNs), plus a comparison sample of 20 starburst galaxies and 43 dwarf galaxies. Published Spitzer/IRS and H... | [
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"Dasyra, Kalliopi M."
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"Istituto di Astrofisica e Planetologia Spaziali, INAF, Via Fosso del Cavaliere 100, I-00133 Roma, Italy",
"Centro de Astrobiología (CSIC/INTA), Ctra. de Torrejón a Ajalvir, km 4, E-28850 Torrejón de Ardoz... | [
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4354206 | 1607.03893 | MUSE searches for galaxies near very metal-poor gas clouds at z ∼ 3: new constraints for cold accretion models | We report on the search for galaxies in the proximity of two very metal-poor gas clouds at z ∼ 3 towards the quasar Q0956+122. With a 5-hour Multi-Unit Spectroscopic Explorer (MUSE) integration in a ∼500 × 500 kpc<SUP>2</SUP> region centred at the quasar position, we achieve a ≥80 per cent complete spectroscopic survey... | [
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] | 8 | [
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"O'Meara, John M.",
"Prochaska, J. Xavier",
"Theuns, Tom"
] | [
"Institute for Computational Cosmology and Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK",
"Institute for Astronomy, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland",
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12472774 | 1607.08245 | Evidence of bar-induced secular evolution in the inner regions of stellar discs in galaxies: what shapes disc galaxies? | We present evidence of bar-induced secular evolution in galactic discs using 3.6 μm images of nearby galaxies from the Spitzer Survey of Stellar Structure in Galaxies (S<SUP>4</SUP>G). We find that among massive galaxies (M<SUB>*</SUB>/M<SUB>⊙</SUB> > 10<SUP>10</SUP>), longer bars tend to reside in inner discs havin... | [
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] | 6 | [
"10.1093/mnras/stw1899",
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] | [
"Kim, Taehyun",
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"Athanassoula, E.",
"Bosma, Albert",
"Sheth, Kartik",
"Lee, Myung Gyoon"
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"Korea Astronomy and Space Science Institute, Daejeon, 34055, Korea; National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA; Astronomy Program, Department of Physics and Astronomy, Seoul National University, Seoul, 08826, Korea",
"European Southern Observatory, Casilla 19001, Sant... | [
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12510630 | 1607.01014 | Integrated approach to cosmology: Combining CMB, large-scale structure, and weak lensing | Recent observational progress has led to the establishment of the standard Λ CDM model for cosmology. This development is based on different cosmological probes that are usually combined through their likelihoods at the latest stage in the analysis. We implement here an integrated scheme for cosmological probes, which ... | [
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"cosmic shear",
"galaxy and shear tracers",
"SDSS",
"CMB",
"current and future wide-field ... | [
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 17 | [
"10.1103/PhysRevD.94.083517",
"10.48550/arXiv.1607.01014"
] | [
"Nicola, Andrina",
"Refregier, Alexandre",
"Amara, Adam"
] | [
"Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland",
"Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland",
"Department of Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich, Switzerland"
] | [
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12409537 | 1607.02145 | The Relation between Stellar and Dynamical Surface Densities in the Central Regions of Disk Galaxies | We use the Spitzer Photometry and Accurate Rotation Curves database to study the relation between the central surface density of stars {{{Σ }}}<SUB>\star </SUB>(0) and dynamical mass {{{Σ }}}<SUB>{{dyn</SUB>}}(0) in 135 disk galaxies (S0 to dIrr). We find that {{{Σ }}}<SUB>{{dyn</SUB>}}(0) correlates tightly with {{{Σ ... | [
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] | 10 | [
"10.3847/2041-8205/827/1/L19",
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] | [
"Lelli, Federico",
"McGaugh, Stacy S.",
"Schombert, James M.",
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] | [
"Department of Astronomy, Case Western Reserve University, Cleveland, OH 44106, USA",
"Department of Astronomy, Case Western Reserve University, Cleveland, OH 44106, USA",
"Department of Physics, University of Oregon, Eugene, OR 97403, USA",
"Department of Astronomy, Case Western Reserve University, Cleveland... | [
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12472686 | 1607.07626 | The prevalence of star formation as a function of Galactocentric radius | We present large-scale trends in the distribution of star-forming objects revealed by the Hi-GAL survey. As a simple metric probing the prevalence of star formation in Hi-GAL sources, we define the fraction of the total number of Hi-GAL sources with a 70 μm counterpart as the `star-forming fraction' or SFF. The mean SF... | [
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12406430 | 1607.04024 | Testing the two planes of satellites in the Centaurus group | Context. The existence of satellite galaxy planes poses a major challenge for the standard picture of structure formation with non-baryonic dark matter. Recently Tully et al. (2015, ApJ, 802, L25) reported the discovery of two almost parallel planes in the nearby Cen A group using mostly high-mass galaxies (M<SUB>B</SU... | [
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] | 4 | [
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1803705 | 1607.01785 | Low Gas Fractions Connect Compact Star-forming Galaxies to Their z ~ 2 Quiescent Descendants | Early quiescent galaxies at z∼ 2 are known to be remarkably compact compared to their nearby counterparts. Possible progenitors of these systems include galaxies that are structurally similar, but are still rapidly forming stars. Here, we present Karl G. Jansky Very Large Array (VLA) observations of the CO(1-0) line to... | [
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"10.3847/0004-637X/832/1/19",
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"Spilker, Justin S.",
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"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA",
"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA;",
"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA",
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12594214 | 1607.06099 | Testing galaxy quenching theories with scatter in the stellar-to-halo mass relation | We use the scatter in the stellar-to-halo mass relation to constrain galaxy evolution models. If the efficiency of converting accreted baryons into stars varies with time, haloes of the same present-day mass but different formation histories will have different z = 0 galaxy stellar mass. This is one of the sources of s... | [
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0.01... | 11.847643 | 6.250027 | 2016-07-01 | 21 | 2017MNRAS.467.3533T | [
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] | 4 | [
"10.1093/mnras/stx287",
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] | [
"Tinker, Jeremy L."
] | [
"Center for Cosmology and Particle Physics, Department of Physics, New York University, New York, 10012 NY, USA"
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5079377 | 1607.01446 | GASS 3505: the prototype of H I-excess, passive galaxies | We present our multiwavelength analysis of a prototype H I-excess galaxy, GASS 3505, selected based on having a large gas content (M_{H I} = 10^{9.9} M<SUB>⊙</SUB>) compared to its little associated star formation activity (∼0.1 M<SUB>⊙</SUB> yr<SUP>-1</SUP>) in the GALEX Arecibo SDSS Survey (GASS). Very Large Array ob... | [
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"galaxies: evolution",
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] | 9 | [
"10.1093/mnras/stw1675",
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"Geréb, K.",
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"Cortese, L.",
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] | [
"Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia",
"ICRAR, M468, The University of Western Australia, 35 Stirling Highway, Crawley, Western Australia 6009, Australia",
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12521647 | 1607.03107 | Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5 < z < 2.5 | In this paper, we investigate the relationship between star formation and structure, using a mass-complete sample of 27,893 galaxies at 0.5 < z < 2.5 selected from 3D-HST. We confirm that star-forming galaxies are larger than quiescent galaxies at fixed stellar mass ({M}<SUB>\star </SUB>). However, in contrast wi... | [
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0.02902... | 12.120652 | 6.656841 | 2016-07-01 | 103 | 2017ApJ...838...19W | [
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] | 29 | [
"10.3847/1538-4357/aa6258",
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"Whitaker, Katherine E.",
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"Giavalisco, Mauro",
"Labbé, Ivo",
"Momcheva, Ivelina G.",
"Nelson, Erica J.",
"Skelton, Rosalind"
] | [
"Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA ; Department of Physics, University of Connecticut, Storrs, CT 06269, USA ;;",
"Steward Observatory, Department of Astronomy, University of Arizona, AZ 85721, USA ; Department of Astrophysics, Princeton University, Princeton, NJ 08544, ... | [
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12516945 | 1607.02120 | Survey strategy optimization for the Atacama Cosmology Telescope | In recent years there have been significant improvements in the sensitivity and the angular resolution of the instruments dedicated to the observation of the Cosmic Microwave Background (CMB). ACTPol is the first polarization receiver for the Atacama Cosmology Telescope (ACT) and is observing the CMB sky with arcmin re... | [
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] | 6 | [
"10.1117/12.2232824",
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"De Bernardis, F.",
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"Ho, S. P.",
"Huffenberger, K.",
"Koopman, B. J.",
... | [
"Cornell Univ. (United States)",
"Cornell Univ. (United States)",
"The Pennsylvania State Univ. (United States)",
"Univ. of Oxford (United Kingdom)",
"CITA, Univ. of Toronto (Canada)",
"Univ. of Oxford (United Kingdom)",
"Princeton Univ. (United States)",
"Princeton Univ. (United States)",
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2516836 | 1607.03112 | Illuminating gas inflows/outflows in the MUSE deepest fields: Lyα nebulae around forming galaxies at z ≃ 3.3 | We report the identification of extended Lyα nebulae at z ≃ 3.3 in the Hubble Ultra Deep Field (HUDF, ≃40 kpc × 80 kpc) and behind the Hubble Frontier Field galaxy cluster MACSJ0416 (≃40 kpc), spatially associated with groups of star-forming galaxies. VLT/MUSE integral field spectroscopy reveals a complex structure wit... | [
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... | 13.708366 | 6.567662 | 2016-07-01 | 47 | 2017MNRAS.465.3803V | [
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910166 | 1607.08833 | The Sunyaev-Zel'dovich effect at 5″: RX J1347.5-1145 imaged by ALMA | We present the first image of the thermal Sunyaev-Zel'dovich effect (SZE) obtained by the Atacama Large Millimeter/submillimeter Array (ALMA). Combining 7-m and 12-m arrays in Band 3, we create an SZE map toward a galaxy cluster RX J1347.5-1145 with 5″ resolution (corresponding to a physical size of 20 h<SUP>-1</SUP> k... | [
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12434930 | 1607.03418 | The Homogeneity Scale of the universe | In this study, we probe the cosmic homogeneity with the BOSS CMASS galaxy sample in the redshift region of $0.43 < z < 0.7$. We use the normalised counts-in-spheres estimator $\mathcal{N}(<r)$ and the fractal correlation dimension $\mathcal{D}_{2}(r)$ to assess the homogeneity scale of the universe. We verify ... | [
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12594591 | 1607.06467 | On the contribution of active galactic nuclei to the high-redshift metagalactic ionizing background | Motivated by the claimed detection of a large population of faint active galactic nuclei (AGNs) at high redshift, recent studies have proposed models in which AGNs contribute significantly to the z > 4 H I ionizing background. In some models, AGNs are even the chief sources of reionization. If proved true, these mod... | [
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... | 13.770774 | 6.053023 | 2016-07-01 | 71 | 2017MNRAS.468.4691D | [
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] | 9 | [
"10.1093/mnras/stx711",
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"D'Aloisio, Anson",
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"Astronomy Department, University of Washington, Seattle, WA 98195, USA",
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"Astronomy Department, University of Washington, Seattle, WA 98195, USA",
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2774770 | 1607.03148 | The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: on the measurement of growth rate using galaxy correlation functions | We present a measurement of the linear growth rate of structure, f, from the Sloan Digital Sky Survey III (SDSS-III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 (DR12) using convolution Lagrangian perturbation theory (CLPT) with Gaussian streaming redshift space distortions (GSRSD) to model the two-p... | [
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"Salazar-Albornoz, Sal... | [
"Department of Physics, Carnegie Mellon University, 5000 Forbes Ave., Pittsburgh, PA 15213, USA; The McWilliams Center for Cosmology, Carnegie Mellon University, 5000 Forbes Ave., Pittsburgh, PA 15213, USA",
"Department of Physics, Carnegie Mellon University, 5000 Forbes Ave., Pittsburgh, PA 15213, USA; The McWil... | [
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1102884 | 1607.03462 | A refined mass distribution of the cluster MACS J0416.1-2403 from a new large set of spectroscopic multiply lensed sources | We report the spectroscopic confirmation of 22 new multiply lensed sources behind the Hubble Frontier Field (HFF) galaxy cluster MACS J0416.1-2403 (MACS 0416), using archival data from the Multi Unit Spectroscopic Explorer (MUSE) on the VLT. Combining with previous spectroscopic measurements of 15 other multiply imaged... | [
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] | 14 | [
"10.1051/0004-6361/201629297",
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"Caminha, G. B.",
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"Delgado-Correal, C.",
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"Lombardi, M.",
"Meneghetti, M.",
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"Tozzi, P."
] | [
"Dipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, via Saragat 1, 44122, Ferrara, Italy",
"Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, 20133, Milano, Italy; Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 21... | [
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12406929 | 1607.02432 | Redshift Measurement and Spectral Classification for eBOSS Galaxies with the redmonster Software | We describe the redmonster automated redshift measurement and spectral classification software designed for the extended Baryon Oscillation Spectroscopic Survey (eBOSS) of the Sloan Digital Sky Survey IV (SDSS-IV). We describe the algorithms, the template standard and requirements, and the newly developed galaxy templa... | [
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"Myers, Adam D.",
"Newman, Jeffrey A.",
"Prakash, Abhishek",
"Carnero-Rosell, Aurelio",
"Seo, Hee-Jon... | [
"Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA",
"Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA; National Optical Astronomy Observatory, 950 N. Cherry Avenue, Tucson, AZ 85719, USA",
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12521085 | 1607.01788 | Hydrodynamical Coupling of Mass and Momentum in Multiphase Galactic Winds | Using a set of high-resolution hydrodynamical simulations run with the Cholla code, we investigate how mass and momentum couple to the multiphase components of galactic winds. The simulations model the interaction between a hot wind driven by supernova explosions and a cooler, denser cloud of interstellar or circumgala... | [
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"Schneider, Evan E.",
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"Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA",
"Department of Astronomy and Astrophysics, University of California, Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, USA"
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2611753 | 1607.02212 | A Global Model for Circumgalactic and Cluster-core Precipitation | We provide an analytic framework for interpreting observations of multiphase circumgalactic gas that is heavily informed by recent numerical simulations of thermal instability and precipitation in cool-core galaxy clusters. We start by considering the local conditions required for the formation of multiphase gas via tw... | [
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"Voit, G. Mark",
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"Donahue, Megan"
] | [
"Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA",
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12436753 | 1607.06669 | Multiwavelength and parsec-scale properties of extragalactic jets | Extragalactic jets originating from the central supermassive black holes of active galaxies are powerful, highly relativistic plasma outflows, emitting light from the radio up to the gamma-ray regime. The details of their formation, composition and emission mechanisms are still not completely clear. The combination of ... | [
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12522505 | 1607.01049 | Synchrotron Emission from Dark Matter Annihilation: Predictions for Constraints from Non-detections of Galaxy Clusters with New Radio Surveys | The annihilation of dark matter particles is expected to yield a broad radiation spectrum via the production of Standard Model particles in astrophysical environments. In particular, electrons and positrons from dark matter annihilation produce synchrotron radiation in the presence of magnetic fields. Galaxy clusters a... | [
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"Storm, Emma",
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"Splettstoesser, Megan",
"Profumo, Stefano"
] | [
"GRAPPA, Universiteit van Amsterdam, Science Park 904, 1098XH Amsterdam, The Netherlands",
"Department of Physics, University of California, 1156 High Street, Santa Cruz, CA 95064, USA ; Santa Cruz Institute for Particle Physics, University of California, 1156 High Street, Santa Cruz, CA 95064, USA",
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12473091 | 1607.07258 | The small observed scale of AGN-driven outflows, and inside-out disc quenching | Observations of massive outflows with detectable central active galactic nuclei (AGN) typically find them within radii ≲10 kpc. We show that this apparent size restriction is a natural result of AGN driving if this process injects total energy only of the order of the gas binding energy to the outflow, and the AGN vari... | [
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] | 5 | [
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"Zubovas, Kastytis",
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"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... | [
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2641915 | 1607.06154 | The evolution of the galaxy content of dark matter haloes | We use the halo occupation distribution (HOD) framework to characterize the predictions from two independent galaxy formation models for the galactic content of dark matter haloes and its evolution with redshift. Our galaxy samples correspond to a range of fixed number densities defined by stellar mass and span 0 ≤ z ≤... | [
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... | 11.840914 | 4.844034 | 2016-07-01 | 24 | 2017MNRAS.465.2833C | [
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"Contreras, S.",
"Zehavi, I.",
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"Institúto Astrofísica, Pontifica Universidad Católica de Chile, 7820436 Santiago, Chile; Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK",
"Department of Astronomy, Case Western Reserve University, Cleveland, OH 44106, USA; Institute for Computation... | [
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12406246 | 1607.02541 | Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy. A detailed modelling of the Galactic disk | <BR /> Aims: Galaxy mass models based on simple and analytical functions for density and potential pairs have been widely proposed in the literature. Disk models that are constrained solely by kinematic data only provide information about the global disk structure very near the Galactic plane. We attempt to circumvent ... | [
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... | [
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] | 16 | [
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"Barros, D. A.",
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"Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Cidade Universitária, 05508-090, São Paulo, SP, Brasil",
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2826726 | 1607.03553 | The connection between galaxy environment and the luminosity function slopes of star-forming regions | We present the first study of GALEX far-ultraviolet (FUV) luminosity functions of individual star-forming regions within a sample of 258 nearby galaxies spanning a large range in total stellar mass and star formation properties. We identify ∼65 000 star-forming regions (I.e. FUV sources), measure each galaxy's luminosi... | [
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] | 10 | [
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"Cook, David O.",
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"Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071, USA; California Institute of Technology, 1200 East California Blvd, Pasadena, CA 91125, USA",
"Department of Physics and Astronomy, University of Wyoming, Laramie, WY 82071, USA",
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1914662 | 1607.02143 | Demonstrating Diversity in Star-formation Histories with the CSI Survey | We present coarse but robust star-formation histories (SFHs) derived from spectrophotometric data of the Carnegie-Spitzer-IMACS Survey, for 22,494 galaxies at 0.3\lt z\lt 0.9 with stellar masses of 10<SUP>9</SUP> M <SUB>⊙</SUB> to 10<SUP>12</SUP> M <SUB>⊙</SUB>. Our study moves beyond “average” SFHs and distribution fu... | [
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] | 6 | [
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"Dressler, Alan",
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"Poggianti, Bianca M.",
"Mulchaey, John S.",
"Vulcani, Benedetta",
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"Williams, Rik J.",
"McCarthy, Patrick J."
] | [
"The Observatories of the Carnegie Institution for Science, 813 Santa Barbara St., Pasadena, CA 91101, USA",
"The Observatories of the Carnegie Institution for Science, 813 Santa Barbara St., Pasadena, CA 91101, USA",
"Department of Physics and Astronomy, University of California, Los Angeles, 475 Portola Pl, L... | [
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1759487 | 1607.08257 | Optical and radio astrometry of the galaxy associated with FRB 150418 | A fading radio source, coincident in time and position with the fast radio burst FRB 150418, has been associated with the galaxy WISE J071634.59-190039.2. Subsequent observations of this galaxy have revealed that it contains a persistent, but variable, radio source. We present e-Multi-Element Radio Linked Interferomete... | [
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"a weak radio",
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] | 10 | [
"10.1093/mnrasl/slw151",
"10.48550/arXiv.1607.08257"
] | [
"Bassa, C. G.",
"Beswick, R.",
"Tingay, S. J.",
"Keane, E. F.",
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"Johnston, S.",
"Totani, T.",
"Tominaga, N.",
"Yasuda, N.",
"Stappers, B. W.",
"Barr, E. D.",
"Kramer, M.",
"Possenti, A."
] | [
"ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, NL-7990 AA Dwingeloo, the Netherlands",
"Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester M13 9PL, UK",
"International Centre for Radio Astronomy Research (ICRAR), Curtin University, Ben... | [
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2774793 | 1607.03145 | The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: observational systematics and baryon acoustic oscillations in the correlation function | We present baryon acoustic oscillation (BAO) scale measurements determined from the clustering of 1.2 million massive galaxies with redshifts 0.2 < z < 0.75 distributed over 9300 deg<SUP>2</SUP>, as quantified by their redshift-space correlation function. In order to facilitate these measurements, we define, desc... | [
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"cosmology: observations",
"large-scale structure of Universe",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 21 | [
"10.1093/mnras/stw2372",
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] | [
"Ross, Ashley J.",
"Beutler, Florian",
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"Vargas-Magaña, Mariana",
"Cuesta, Antonio J.",
"Percival, Will J.",
"Burden, Angela",
"Sánchez, Ariel G.",
"Grieb, Jan Niklas",
"Reid, Beth",
"Brownstein, Joel R.",
"Dawson, Kyle S.",
... | [
"Center for Cosmology and AstroParticle Physics, The Ohio State University, Columbus, OH 43210, USA; Institute of Cosmology & Gravitation, Dennis Sciama Building, University of Portsmouth, Portsmouth PO1 3FX, UK",
"Institute of Cosmology & Gravitation, Dennis Sciama Building, University of Portsmouth, Por... | [
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1803189 | 1607.06088 | A Synoptic Map of Halo Substructures from the Pan-STARRS1 3π Survey | We present a panoramic map of the entire Milky Way halo north of δ ∼ -30° (∼30 000 deg<SUP>2</SUP>), constructed by applying the matched-filter technique to the Pan-STARRS1 3π Survey data set. Using single-epoch photometry reaching to g ∼22, we are sensitive to stellar substructures with heliocentric distances between ... | [
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] | 9 | [
"10.1093/mnras/stw2134",
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] | [
"Bernard, Edouard J.",
"Ferguson, Annette M. N.",
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"Martínez-Delgado, David",
"Sesar, Branimir",
"Wyse, Rosemary F. G.",
"Burgett, William S.",
"Chambers, Kenneth C... | [
"Université Côte d'Azur, OCA, CNRS, Lagrange, France; SUPA, Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK",
"SUPA, Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK",
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1916373 | 1607.00384 | The Grism Lens-amplified Survey from Space (Glass). IX. The Dual Origin of Low-mass Cluster Galaxies as Revealed by New Structural Analyses | Using deep Hubble Frontier Fields imaging and slitless spectroscopy from the Grism Survey from Space, we study 2200 cluster and 1748 field galaxies at 0.2≤slant z≤slant 0.7 to determine the impact of environment on galaxy size and structure at stellar masses {log}{M}<SUB>* </SUB>/{M}<SUB>⊙ </SUB>> 7.8, an unpreceden... | [
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0.0175694... | 12.274179 | 6.201817 | 2016-07-01 | 45 | 2017ApJ...835..254M | [
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"galaxies: clusters: general",
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"cD",
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] | 13 | [
"10.3847/1538-4357/835/2/254",
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"Morishita, Takahiro",
"Abramson, Louis E.",
"Treu, Tommaso",
"Vulcani, Benedetta",
"Schmidt, Kasper B.",
"Dressler, Alan",
"Poggianti, Bianca M.",
"Malkan, Matthew A.",
"Wang, Xin",
"Huang, Kuang-Han",
"Trenti, Michele",
"Bradač, Maruša",
"Hoag, Austin"
] | [
"Department of Physics and Astronomy, UCLA, 430 Portola Plaza, Los Angeles, CA 90095-1547, USA; Astronomical Institute, Tohoku University, Aramaki, Aoba, Sendai 980-8578, Japan; Institute for International Advanced Research and Education, Tohoku University, Aramaki, Aoba, Sendai 980-8578, Japan;",
"Department of ... | [
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13386071 | 1607.06325 | Testing theories of gravity and supergravity with inflation and observations of the cosmic microwave background | Cosmological and astrophysical observations lead to the emerging picture of a universe that is spatially flat and presently undertaking an accelerated expansion. The observations supporting this picture come from a range of measurements encompassing estimates of galaxy cluster masses, the Hubble diagram derived from ty... | [
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... | 10.699969 | 0.921153 | 2016-07-01 | 11 | 2017IJMPD..2630023C | [
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"Ricci curvature R",
"gravity",
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] | 4 | [
"10.1142/S0218271817300233",
"10.48550/arXiv.1607.06325"
] | [
"Chakravarty, G. K.",
"Mohanty, S.",
"Lambiase, G."
] | [
"Physical Research Laboratory, Ahmedabad 380009, India",
"Physical Research Laboratory, Ahmedabad 380009, India",
"Dipartimento di Fisica “E. R. Caianiello”, Università degli Studi di Salerno, Via Giovanni Paolo II, Fisciano, Italy"
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2471992 | 1607.07445 | The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end | Galaxies fall into two clearly distinct types: `blue-sequence' galaxies which are rapidly forming young stars, and `red-sequence' galaxies in which star formation has almost completely ceased. Most galaxies more massive than 3 × 10<SUP>10</SUP> M<SUB>⊙</SUB> follow the red sequence, while less massive central galaxies ... | [
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] | 37 | [
"10.1093/mnras/stw2735",
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] | [
"Bower, Richard G.",
"Schaye, Joop",
"Frenk, Carlos S.",
"Theuns, Tom",
"Schaller, Matthieu",
"Crain, Robert A.",
"McAlpine, Stuart"
] | [
"Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK",
"Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands",
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2262974 | 1607.02056 | Shear nulling after PSF Gaussianisation: Moment-based weak lensing measurements with subpercent noise bias | Context. Current optical imaging surveys for cosmology cover large areas of sky. Exploiting the statistical power of these surveys for weak lensing measurements requires shape measurement methods with subpercent systematic errors. <BR /> Aims: We introduce a new weak lensing shear measurement algorithm, shear nulling a... | [
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] | 6 | [
"10.1051/0004-6361/201629263",
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] | [
"Herbonnet, Ricardo",
"Buddendiek, Axel",
"Kuijken, Konrad"
] | [
"Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands",
"Argelander-Institut für Astronomie, Rheinische Friedrich-Wilhelms-Universität Bonn, Auf dem Hügel 71, 53121, Bonn, Germany",
"Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands"
] | [
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12408929 | 1607.04670 | The Tidal Filament of NGC 4660 | NGC 4660, in the Virgo cluster, is a well-studied elliptical galaxy which has a strong disk component (D/T approximately 0.2-0.3). The central regions, including the disk component, have stellar populations approximately 12-13 Gyr in age, based on SAURON studies. However, we report the discovery of a long, narrow tidal... | [
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... | 10.974728 | 7.634358 | 2016-07-01 | 5 | 2016ApJ...830...66K | [
"tidal dwarf galaxies",
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"deep co-added Schmidt plate images",
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"little evidence",
"enhanced star formation",
"age",
"perigalactic passages",
"a strong disk component",
"merger",
"the last few Gyr",
"stellar populations",
"the disk comp... | [
"galaxies: evolution",
"galaxies: fundamental parameters",
"galaxies: individual: NGC 4660",
"galaxies: photometry",
"galaxies: stellar content",
"galaxies: structure",
"Astrophysics - Astrophysics of Galaxies"
] | 7 | [
"10.3847/0004-637X/830/2/66",
"10.48550/arXiv.1607.04670"
] | [
"Kemp, S. N.",
"Martínez-Robles, C.",
"Márquez-Lugo, R. A.",
"Zepeda-García, D.",
"Franco-Hernández, R.",
"Nigoche-Netro, A.",
"Ramos-Larios, G.",
"Navarro, S. G.",
"Corral, L. J."
] | [
"Instituto de Astronomía y Meteorología, Universidad de Guadalajara, Av. Vallarta 2602, Arcos Vallarta, 44130, Guadalajara, Mexico",
"CUCEI, Universidad de Guadalajara, Av. Revolución No. 1500 S.R., 44420 Guadalajara, Jalisco, Mexico",
"CUCEI, Universidad de Guadalajara, Av. Revolución No. 1500 S.R., 44420 Guad... | [
"2017MNRAS.466.4259B",
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12434351 | 1607.01181 | Compact Massive Object in Galaxies | The central regions of galaxies show the presence of super massive black holes and/or very dense stellar clusters. Both objects seem to follow similar host-galaxy correlations, suggesting that they are members of the same family of Compact Massive Objects. We investigate here a huge data collection of Compact Massive O... | [
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... | 9.506412 | 6.98839 | 2016-07-01 | 0 | 2016arXiv160701181M | [
"Compact Massive Objects properties",
"Compact Massive Objects",
"absolute magnitude",
"velocity dispersion",
"super massive black holes",
"galaxies",
"similar host-galaxy correlations",
"mass",
"members",
"their host galaxies",
"very dense stellar clusters",
"the same family",
"a huge data ... | [
"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.48550/arXiv.1607.01181"
] | [
"Melo, I. Tosta e",
"Capuzzo-Dolcetta, R."
] | [
"-",
"-"
] | null | [
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] |
12407018 | 1607.01304 | Cool Subdwarf Investigations. III. Dynamical Masses of Low-metallicity Subdwarfs | We report dynamical mass measurements for the components of the previously known double-lined spectroscopic subdwarfs G 006-026 B and C using the Fine Guidance Sensors on the Hubble Space Telescope. To build the empirical mass-luminosity relation for low-metallicity subdwarfs, we collect four other subdwarf systems wit... | [
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-0.... | 6.988027 | 12.153144 | 2016-07-01 | 10 | 2016AJ....152..153J | [
"low metallicity",
"metallicity measurements",
"dynamical mass measurements",
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"low-mass subdwarfs",
"theoretical models",
"much work",
"various metallicities",
"the Hubble Space Telescope",
"subdwarf",
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"astrometry",
"binaries: spectroscopic",
"solar neighborhood",
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"stars: fundamental parameters",
"Astrophysics - Solar and Stellar Astrophysics"
] | 5 | [
"10.3847/0004-6256/152/6/153",
"10.48550/arXiv.1607.01304"
] | [
"Jao, Wei-Chun",
"Nelan, Edmund P.",
"Henry, Todd J.",
"Franz, Otto G.",
"Wasserman, Lawrence H."
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"-",
"Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA",
"RECONS Institute, Chambersburg, PA 17201, USA ;;",
"Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001, USA",
"Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001, USA"
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12472427 | 1607.08761 | Tidal bridge and tidal dwarf candidates in the interacting system Arp194 | Arp194 is a system of recently collided galaxies, where the southern galaxy (S) passed through the gaseous disc of the northern galaxy (N) which in turn consists of two close components. This system is of special interest due to the presence of regions of active star formation in the bridge between galaxies, the bright... | [
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] | 4 | [
"10.1093/mnras/stw1905",
"10.48550/arXiv.1607.08761"
] | [
"Zasov, Anatoly V.",
"Saburova, Anna S.",
"Egorov, Oleg V.",
"Afanasiev, Viktor L."
] | [
"Sternberg Astronomical Institute, Moscow M.V. Lomonosov State University, Universitetskij pr., 13, Moscow 119991, Russia; Faculty of Physics, Moscow M.V. Lomonosov State University, Leninskie gory 1, Moscow 119991, Russia",
"Sternberg Astronomical Institute, Moscow M.V. Lomonosov State University, Universitetski... | [
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12473407 | 1607.08784 | Modelling the impact of intrinsic size and luminosity correlations on magnification estimation | Spatial correlations of the observed sizes and luminosities of galaxies can be used to estimate the magnification that arises through weak gravitational lensing. However, the intrinsic properties of galaxies can be similarly correlated through local physical effects, and these present a possible contamination to the we... | [
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-0.... | 12.285136 | 3.732703 | 2016-07-01 | 4 | 2016MNRAS.463..740C | [
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... | [
"gravitational lensing: weak",
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"Astrophysics - Astrophysics of Galaxies"
] | 4 | [
"10.1093/mnras/stw2052",
"10.48550/arXiv.1607.08784"
] | [
"Ciarlariello, Sandro",
"Crittenden, Robert"
] | [
"Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth PO1 3FX, UK",
"Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth PO1 3FX, UK"
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12409074 | 1607.03965 | Distribution of Cold (≲300 K) Atomic Gas in Galaxies: Results from the GBT H I Absorption Survey Probing the Inner Halos (ρ < 20 kpc) of Low-z Galaxies | We present the Green Bank Telescope absorption survey of cold atomic hydrogen (≲300 K) in the inner halo of low-redshift galaxies. The survey aims to characterize the cold gas distribution and to address where the condensation—the process where ionized gas accreted by galaxies condenses into cold gas within the disks o... | [
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... | [
"galaxies: halos",
"galaxies: ISM",
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] | 3 | [
"10.3847/0004-637X/829/2/128",
"10.48550/arXiv.1607.03965"
] | [
"Borthakur, Sanchayeeta"
] | [
"Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, 21218, USA; The Astronomy Department, University of California, Berkeley, CA USA"
] | [
"2017MNRAS.465..588D",
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12406481 | 1607.04068 | Radio continuum and X-ray emission from the most extreme far-IR-excess galaxy <ASTROBJ>NGC 1377</ASTROBJ>. An extremely obscured AGN revealed | Context. Galaxies which strongly deviate from the radio-far infrared (FIR) correlation are of great importance for studies of galaxy evolution as they may be tracing early, short-lived stages of starbursts and active galactic nuclei (AGNs). The most extreme FIR-excess galaxy NGC 1377 has long been interpreted as a youn... | [
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-0... | 13.834854 | 8.210515 | 2016-07-01 | 12 | 2016A&A...594A.114C | [
"star formation",
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"NGC",
"Soft X-ray emission",
"new radio observations",
"CO",
"Soft X-ray",
"the collimated CO outflow",
"a powerfu... | [
"radio continuum: galaxies",
"X-rays: galaxies",
"galaxies: active",
"galaxies: starburst",
"galaxies: jets",
"galaxies: individual: NGC 1377",
"Astrophysics - Astrophysics of Galaxies"
] | 5 | [
"10.1051/0004-6361/201628997",
"10.48550/arXiv.1607.04068"
] | [
"Costagliola, F.",
"Herrero-Illana, R.",
"Lohfink, A.",
"Pérez-Torres, M.",
"Aalto, S.",
"Muller, S.",
"Alberdi, A."
] | [
"Chalmers University of Technology, Onsala Space Observatory, 439 92, Onsala, Sweden ; INAF-Istituto di Radioastronomia - Italian ARC, via Gobetti 101, 40129, Bologna, Italy",
"Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía, s/n, 18008, Granada, Spain",
"Institute of Astronomy, Univ... | [
"2017A&A...608A..22A",
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2640489 | 1607.05717 | The far infra-red SEDs of main sequence and starburst galaxies | We compare observed far infrared/sub-millimetre (FIR/sub-mm) galaxy spectral energy distributions (SEDs) of massive galaxies (M<SUB>⋆</SUB> ≳ 10<SUP>10</SUP> h<SUP>-1</SUP> M<SUB>⊙</SUB>) derived through a stacking analysis with predictions from a new model of galaxy formation. The FIR SEDs of the model galaxies are ca... | [
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-0... | 12.782627 | 7.464051 | 2016-07-01 | 26 | 2017MNRAS.467.1231C | [
"galaxy formation",
"higher redshifts",
"massive galaxies",
"Galaxies",
"galaxies",
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"redshifts",
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"SUB>⋆</SUB",
"the model galaxies",
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"... | [
"galaxies: formation",
"galaxies: evolution",
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"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 10 | [
"10.1093/mnras/stx165",
"10.48550/arXiv.1607.05717"
] | [
"Cowley, William I.",
"Béthermin, Matthieu",
"Lagos, Claudia del P.",
"Lacey, Cedric G.",
"Baugh, Carlton M.",
"Cole, Shaun"
] | [
"Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham, DH1 3LE, UK; Kapteyn Astronomical Institute, University of Groningen, P.O. Box 800, 9700 AV Groningen, The Netherlands",
"European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany",
"... | [
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"2019MNRAS.482.4... | [
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4299539 | 1607.02137 | Fundamental Parameters of Main-Sequence Stars in an Instant with Machine Learning | Owing to the remarkable photometric precision of space observatories like Kepler, stellar and planetary systems beyond our own are now being characterized en masse for the first time. These characterizations are pivotal for endeavors such as searching for Earth-like planets and solar twins, understanding the mechanisms... | [
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-0... | 7.510996 | 11.811775 | 2016-07-01 | 72 | 2016ApJ...830...31B | [
"substantial computational effort",
"fundamental stellar parameters",
"stellar evolution",
"solar twins",
"Galaxy",
"Kepler",
"masse",
"masses",
"other methods",
"many more stellar parameters",
"stellar and planetary systems",
"existing methods",
"much less computation time",
"classical an... | [
"methods: statistical",
"stars: abundances",
"stars: fundamental parameters",
"stars: low-mass",
"stars: oscillations",
"stars: solar-type",
"Astrophysics - Solar and Stellar Astrophysics",
"Astrophysics - Instrumentation and Methods for Astrophysics",
"Computer Science - Artificial Intelligence"
] | 16 | [
"10.3847/0004-637X/830/1/31",
"10.48550/arXiv.1607.02137"
] | [
"Bellinger, Earl P.",
"Angelou, George C.",
"Hekker, Saskia",
"Basu, Sarbani",
"Ball, Warrick H.",
"Guggenberger, Elisabeth"
] | [
"Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, D-37077 Göttingen, Germany ; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark ; Institut für Informatik, Georg-August-Universität Göttingen, Goldschmidtstrasse 7, ... | [
"2017ApJ...835..172L",
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"2018ApJ...859..... | [
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12473156 | 1607.02190 | The elusive stellar halo of the Triangulum galaxy | The stellar haloes of large galaxies represent a vital probe of the processes of galaxy evolution. They are the remnants of the initial bouts of star formation during the collapse of the protogalactic cloud, coupled with imprint of ancient and ongoing accretion events. Previously, we have reported the tentative detecti... | [
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... | 9.882044 | 7.715018 | 2016-07-01 | 11 | 2016MNRAS.461.4374M | [
"galaxy evolution",
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"L",
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"a total halo luminosity",
"The stellar haloes",
"the stellar halo",
"substructure",
"a large-scale smooth stellar halo",
"lt",
"contamination",
"ancient and ongoing accretion events",
"more robust search algo... | [
"galaxies: haloes",
"galaxies: individual: M33",
"Local Group",
"Astrophysics - Astrophysics of Galaxies",
"Astrophysics - Cosmology and Nongalactic Astrophysics"
] | 5 | [
"10.1093/mnras/stw1657",
"10.48550/arXiv.1607.02190"
] | [
"McMonigal, B.",
"Lewis, G. F.",
"Brewer, B. J.",
"Irwin, M. J.",
"Martin, N. F.",
"McConnachie, A. W.",
"Ibata, R. A.",
"Ferguson, A. M. N.",
"Mackey, A. D.",
"Chapman, S. C."
] | [
"Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, Sydney, NSW 2006, Australia",
"Sydney Institute for Astronomy, School of Physics, A28, The University of Sydney, Sydney, NSW 2006, Australia",
"Department of Statistics, The University of Auckland, Private Bag 92019, Auckland 114... | [
"2017ASSL..434...31C",
"2017MNRAS.464.3825P",
"2018A&A...612A..35G",
"2019MNRAS.484.1756M",
"2021ApJS..253...53W",
"2022ApJ...924..116G",
"2022ApJ...932...44G",
"2022ApJ...933..201L",
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"2023ApJ...958..157C",
"2024arXiv240314234O"
] | [
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"2007ApJ...671.1591I",
"2008AJ....135.1482S",
"2008ApJ...685L.121B",
"2008ApJS..178...89D",
"2009ApJ...698L.... |
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