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Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0
Kameswara Bharadwaj Mantha, Daniel H. McIntosh, Ryan Brennan +37
The rate of major galaxy-galaxy merging is theoretically predicted to steadily increase with redshift during the peak epoch of massive galaxy development (). We us…
CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies at z~2
Dale D. Kocevski, Guillermo Barro, S. M. Faber +31
We examine the fraction of massive (), compact star-forming galaxies (cSFGs) that host an active galactic nucleus (AGN) at . These cSFGs are likely…
The Origins of UV-optical Color Gradients in Star-forming Galaxies at z ~ 2: Predominant Dust Gradients But Negligible sSFR Gradients
F. S. Liu, Dongfei Jiang, S. M. Faber +13
The rest-frame UV-optical (i.e., ) color is sensitive to both low-level recent star formation (specific star formation rate - sSFR) and dust. In this Letter, we extend our p…
Weak Galactic Winds in Active Galactic Nuclei Post-starburst Host Galaxies at z ~ 0.1
Hassen M. Yesuf, S. M. Faber, David C. Koo +1
Post-starburst (PSB) galaxies may be in rapid transition from star-forming to quiescence and are excellent candidates to constrain active galactic nuclei (AGN) feedback models. We…
CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies
Yicheng Guo, Eric F. Bell, Yu Lu +17
We investigate the environmental quenching of galaxies, especially those with stellar masses (M*), beyond the local universe. Essentially all local low-mass quen…
UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles
Weichen Wang, S. M. Faber, F. S. Liu +10
This paper uses radial colour profiles to infer the distributions of dust, gas and star formation in z=0.4-1.4 star-forming main sequence galaxies. We start with the standard UVJ-b…