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20082026
most citedThe DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts

740 citations · 9.4k across the 189 of their papers we have counts for

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Showing 2019 · astro-ph.GAShow all

15 papers · 2 filters

astro-ph.GA2019★ 159 cited

The ALPINE-ALMA [CII] Survey: Multi-Wavelength Ancillary Data and Basic Physical Measurements

A. L. Faisst, D. Schaerer, B. C. Lemaux +37

We present the ancillary data and basic physical measurements for the galaxies in the ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey - the first large multi-wa…

astro-ph.GA2019★ 170 cited

The ALPINE-ALMA [CII] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe

M. Ginolfi, G. C. Jones, M. Bethermin +29

We study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158 um emission in a large sample of normal star-forming galaxies at 4 < z < 6 from the AL…

astro-ph.GA2019★ 15 cited

The Properties of Radio and Mid-infrared Detected Galaxies and the Effect of Environment on the Co-evolution of AGN and Star Formation at

Lu Shen, Brian C. Lemaux, Lori M. Lubin +10

In this study we investigate 179 radio-IR galaxies drawn from a sample of spectroscopically-confirmed galaxies that are detected in radio and mid-infrared (MIR) in the redshift ran…

astro-ph.GA2019★ 18 cited

The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Follow-Up Optical Imaging

Emmet Golden-Marx, E. L. Blanton, R. Paterno-Mahler +6

Here we present new red sequence overdensity measurements for 77 fields in the high- Clusters Occupied by Bent Radio AGN (COBRA) survey, based on - and -band imaging taken…

astro-ph.GA2019★ 7 cited

The most massive, passive, and oldest galaxies at 0.5 < z < 2.1: Downsizing signature from galaxies selected from MgUV index

R. Thomas, O. Le Fèvre, G. Zamorani +10

Aims. We seek is to identify old and massive galaxies at 0.5<z<2.1 on the basis of the magnesium index MgUV and then study their physical properties. We computed the MgUV index bas…

astro-ph.GA2019★ 31 cited

RELICS: Spectroscopy of gravitationally-lensed reionization-era analogs and implications for CIII] detections at

Ramesh Mainali, Daniel P Stark, Mengtao Tang +17

Recent observations have revealed the presence of strong CIII] emission (EW Å) in galaxies, the origin of which remains unclear. In an effort to understand…

astro-ph.GA2019★ 42 cited

The ALPINE-ALMA [CII] Survey: A Triple Merger at z~4.56

G. C. Jones, M. Bethermin, Y. Fudamoto +29

We report the detection of [CII]158um emission from a system of three closely-separated sources in the COSMOS field at z~4.56, as part of the ALMA Large Program to INvestigate CII…

astro-ph.GA2019★ 27 cited

Hubble Frontier Field Photometric Catalogues of Abell 370 and RXC J2248.7-4431: Multiwavelength photometry, photometric redshifts, and stellar properties

Marusa Bradac, Kuang-Han Huang, Marco Castellano +15

This paper presents multiwavelength photometric catalogues of the last two Hubble Frontier Fields (HFF), the massive galaxy clusters Abell 370 and RXC J2248.7-4431. The photometry…

astro-ph.GA2019★ 45 cited

Stellar Properties of z ~ 8 Galaxies in the Reionization Lensing Cluster Survey

Victoria Strait, Marusa Bradac, Dan Coe +18

Measurements of stellar properties of galaxies when the universe was less than one billion years old yield some of the only observational constraints of the onset of star formation…

astro-ph.GA2019★ 43 cited

How Do Galaxies trace a large scale structure?: A case study around a massive protocluster at

Ke Shi, Yun Huang, Kyoung-Soo Lee +7

In the hierarchical theory of galaxy formation, a galaxy overdensity is a hallmark of a massive cosmic structure. However, it is less well understood how different types of galaxie…

astro-ph.GA2019★ 33 cited

Establishing a New Technique for Discovering Large-Scale Structure Using the ORELSE Survey

D. Hung, B. C. Lemaux, R. R. Gal +10

The Observations of Redshift Evolution in Large Scale Environments (ORELSE) survey is an ongoing imaging and spectroscopic campaign initially designed to study the effects of envir…

astro-ph.GA2019

Astro2020 Science White Paper: Assembly of the Most Massive Clusters at Cosmic Noon

Jeyhan Kartaltepe, Caitlin Casey, Mark Dickinson +5

Galaxy evolution is driven by many complex interrelated processes as galaxies accrete gas, form new stars, grow their stellar masses and central black holes, and subsequently quenc…

astro-ph.GA2019★ 210 cited

RELICS: Reionization Lensing Cluster Survey

Dan Coe, Brett Salmon, Marusa Bradac +54

Large surveys of galaxy clusters with the Hubble and Spitzer Space Telescopes, including CLASH and the Frontier Fields, have demonstrated the power of strong gravitational lensing…

astro-ph.GA2019★ 48 cited

The UV and Ly Luminosity Functions of galaxies and the Star Formation Rate Density at the end of HI reionization from the VIMOS Ultra-Deep Survey (VUDS)

Y. Khusanova, O. Le Fèvre, P. Cassata +25

We establish a robust statistical description of the star-forming galaxy population at the end of cosmic HI reionization () from a large sample of 52 galaxies with…

astro-ph.GA2019★ 182 cited

Constraining the neutral fraction of hydrogen in the IGM at redshift 7.5

Austin Hoag, Maruša Bradač, Kuang-Han Huang +8

We present a large spectroscopic campaign with Keck/MOSFIRE targeting Lyman-alpha emission (Ly) from intrinsically faint Lyman-break Galaxies (LBGs) behind 12 efficient galaxy c…