Showing 2017 · astro-ph.GAShow all

18 papers · 2 filters

astro-ph.GA2017★ 246 cited

Galaxy growth in a massive halo in the first billion years of cosmic history

D. P. Marrone, J. S. Spilker, C. C. Hayward +34

According to the current understanding of cosmic structure formation, the precursors of the most massive structures in the Universe began to form shortly after the Big Bang, in reg…

astro-ph.GA2017★ 82 cited

Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback

Hui Li, Oleg Y. Gnedin, Nickolay Y. Gnedin

The implementation of star formation and stellar feedback in cosmological simulations plays a critical role in shaping galaxy properties. In the first paper of the series, we prese…

astro-ph.GA2017★ 92 cited

Quasar Accretion Disk Sizes From Continuum Reverberation Mapping From the Dark Energy Survey

D. Mudd, P. Martini, Y. Zu +69

We present accretion disk size measurements for 15 luminous quasars at derived from light curves from the Dark Energy Survey. We measure the disk sizes…

astro-ph.GA2017★ 55 cited

Observational signatures of a warped disk associated with cold-flow accretion

Hadi Rahmani, Céline Péroux, Ramona Augustin +9

We present MUSE observations of the field of the quasar Q0152020 whose spectrum shows a Lyman limit system (LLS) at redshift , with a metallicity Z $\gtrsim…

astro-ph.GA2017★ 33 cited

The Behavior of Selected Diffuse Interstellar Bands with Molecular Fraction in Diffuse Atomic and Molecular Clouds

Haoyu Fan, Daniel E. Welty, Donald G. York +10

We study the behavior of eight diffuse interstellar bands (DIBs) in different interstellar environments, as characterized by the fraction of hydrogen in molecular form [(H)]…

astro-ph.GA2017★ 22 cited

Deep SOAR follow-up photometry of two Milky Way outer-halo companions discovered with Dark Energy Survey

E. Luque, B. Santiago, A. Pieres +48

We report the discovery of a new star cluster, DES 3, in the constellation of Indus, and deeper observations of the previously identified satellite DES J0222.75217 (Eridanus III…

astro-ph.GA2017★ 26 cited

DES Science Portal: Computing Photometric Redshifts

Julia Gschwend, Aurelio Carnero Rosell, Ricardo Ogando +68

A significant challenge facing photometric surveys for cosmological purposes is the need to produce reliable redshift estimates. The estimation of photometric redshifts (photo-zs)…

astro-ph.GA2017★ 21 cited

DES15E2mlf: A Spectroscopically Confirmed Superluminous Supernova that Exploded 3.5 Gyr After the Big Bang

Y. -C. Pan, R. J. Foley, M. Smith +63

We present the Dark Energy Survey (DES) discovery of DES15E2mlf, the most distant superluminous supernova (SLSN) spectroscopically confirmed to date. The light curves and Gemini sp…

astro-ph.GA2017★ 37 cited

Milky Way Tomography with K and M Dwarf Stars: the Vertical Structure of the Galactic Disk

Deborah Ferguson, Susan Gardner, Brian Yanny

We use the number density distributions of K and M dwarf stars with vertical height from the Galactic disk, determined using observations from the Sloan Digital Sky Survey, to prob…

astro-ph.GA2017

Extreme variability quasars from the Sloan Digital Sky Survey and the Dark Energy Survey

Nick Rumbaugh, Yue Shen, Eric Morganson +49

We perform a systematic search for long-term extreme variability quasars (EVQs) in the overlapping Sloan Digital Sky Survey (SDSS) and 3-Year Dark Energy Survey (DES) imaging, whic…

astro-ph.GA2017★ 149 cited

ISM properties of a Massive Dusty Star-Forming Galaxy discovered at z ~ 7

M. L. Strandet, A. Weiß, C. De Breuck +28

We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy (DSFG) to date, SPT-S…

astro-ph.GA2017★ 127 cited

The physical origin of long gas depletion times in galaxies

Vadim A. Semenov, Andrey V. Kravtsov, Nickolay Y. Gnedin

We present a model that explains why galaxies form stars on a time scale significantly longer than the time scales of processes governing the evolution of interstellar gas. We show…

astro-ph.GA2017★ 5 cited

Candidate members of the Pal 5, GD-1, Cetus Polar, and Orphan tidal stellar halo streams from Sdss DR9, Lamost DR3 and APOGEE catalogues

Guang-Wei Li, Brian Yanny, Hao-Tong Zhang +8

We present candidate members of the Pal 5, GD-1, Cetus Polar, and Orphan tidal stellar streams found in LAMOST DR3, SDSS DR9 and APOGEE catalogs. In LAMOST DR3, we find 20, 4, 24 h…

astro-ph.GA2017★ 36 cited

Exploring Halo Substructure with Giant Stars. XV. Discovery of a Connection between the Monoceros Ring and the Triangulum-Andromeda Overdensity?

Ting S. Li, Allyson A. Sheffield, Kathryn V. Johnston +9

Thanks to modern sky surveys, over twenty stellar streams and overdensity structures have been discovered in the halo of the Milky Way. In this paper, we present an analysis of spe…

astro-ph.GA2017★ 28 cited

Models of the strongly lensed quasar DES J0408-5354

Adriano Agnello, Huan Lin, L. Buckley-Geer +82

We present gravitational lens models of the multiply imaged quasar DES J0408-5354, recently discovered in the Dark Energy Survey (DES) footprint, with the aim of interpreting its r…

astro-ph.GA2017★ 39 cited

Discovery of the Lensed Quasar System DES J0408-5354

H. Lin, E. Buckley-Geer, A. Agnello +78

We report the discovery and spectroscopic confirmation of the quad-like lensed quasar system DES J0408-5354 found in the Dark Energy Survey (DES) Year 1 (Y1) data. This system was…

astro-ph.GA2017★ 27 cited

Environmental dependence of the galaxy stellar mass function in the Dark Energy Survey Science Verification Data

J. Etherington, D. Thomas, C. Maraston +61

Measurements of the galaxy stellar mass function are crucial to understand the formation of galaxies in the Universe. In a hierarchical clustering paradigm it is plausible that the…

astro-ph.GA2017★ 129 cited

Eight new luminous z > 6 quasars selected via SED model fitting of VISTA, WISE and Dark Energy Survey Year 1 Observations

S. L. Reed, R. G. McMahon, P. Martini +60

We present the discovery and spectroscopic confirmation with the ESO NTT and Gemini South telescopes of eight new 6.0 < z < 6.5 quasars with z < 21.0. These quasars were pho…