activity
20022026
most citedOverview of the DESI Legacy Imaging Surveys

1.9k citations · 32.3k across the 376 of their papers we have counts for

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Showing 2011Show all

9 papers · 1 filter

astro-ph.CO2011★ 30 cited

Evolution of the Stellar Mass-Metallicity Relation Since z=0.75

John Moustakas, Dennis Zaritsky, Michael Brown +9

We measure the gas-phase oxygen abundances of ~3000 star-forming galaxies at z=0.05-0.75 using optical spectrophotometry from the AGN and Galaxy Evolution Survey (AGES), a spectros…

astro-ph.CO2011★ 50 cited

CLASH: Discovery of a Bright z~6.2 Dwarf Galaxy Quadruply Lensed by MACS J0329.6-0211

A. Zitrin, J. Moustakas, L. Bradley +22

We report the discovery of a z_{phot}=6.18^{+0.05}_{-0.07} (95% confidence level) dwarf galaxy, lensed into four images by the galaxy cluster MACS J0329.6-0211 (z_{l}=0.45). The ga…

astro-ph.CO2011★ 620 cited

Dust-Corrected Star Formation Rates of Galaxies. II. Combinations of Ultraviolet and Infrared Tracers

Cai-Na Hao, Robert C. Kennicutt, Benjamin D. Johnson +3

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total infrared to FUV luminosity ratio (IRX) and the FUV-NUV color. We find that the IRX-correc…

astro-ph.CO2011★ 27 cited

Calibrating the Star Formation Rate at z=1 from Optical Data

Nick Mostek, Alison L. Coil, John Moustakas +2

We present a star-formation rate calibration based on optical data that is consistent with average observed rates in both the red and blue galaxy populations at z~1. The motivation…

astro-ph.CO2011★ 9 cited

A Search for Young Stars in the S0 Galaxies of a Super-Group at z=0.37

Dennis W. Just, Dennis Zaritsky, Kim-Vy H. Tran +3

We analyze GALEX UV data for a system of four gravitationally-bound groups at z=0.37, SG1120, which is destined to merge into a Coma-mass cluster by z=0, to study how galaxy proper…

astro-ph.CO2011★ 311 cited

PRIMUS: The dependence of AGN accretion on host stellar mass and color

James Aird, Alison L. Coil, John Moustakas +7

We present evidence that the incidence of active galactic nuclei (AGNs) and the distribution of their accretion rates do not depend on the stellar masses of their host galaxies, co…