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Are Compton-Thick AGN the Missing Link Between Mergers and Black Hole Growth?
Dale D. Kocevski, Murray Brightman, Kirpal Nandra +12
We examine the host morphologies of heavily obscured active galactic nuclei (AGN) at to test whether obscured supermassive black hole growth at this epoch is preferentiall…
Dusty galaxies and the degeneracy between their dust distributions and the attenuation formula
Kyle Penner, Mark Dickinson, Benjamin Weiner +7
Do spatial distributions of dust grains in galaxies have typical forms, as do spatial distributions of stars? We investigate whether or not the distributions resemble uniform foreg…
The composite nature of Dust-Obscured Galaxies (DOGs) at z~2-3 in the COSMOS field: I. A Far-Infrared View
L. Riguccini, E. Le Floc'h, J. R. Mullaney +19
Dust-Obscured galaxies (DOGs) are bright 24 um-selected sources with extreme obscuration at optical wavelengths. They are typically characterized by a rising power-law continuum of…
Rest-frame Optical Emission Lines in Far-Infrared Selected Galaxies at z<1.7 from the FMOS-COSMOS Survey
Jeyhan S. Kartaltepe, D. B. Sanders, J. D. Silverman +15
We have used FMOS on Subaru to obtain near-infrared spectroscopy of 123 far-infrared selected galaxies in COSMOS and obtain the key rest-frame optical emission lines. This is the l…
A higher efficiency of converting gas to stars push galaxies at z ~ 1.6 well above the star-forming main sequence
J. D. Silverman, E. Daddi, G. Rodighiero +18
Local starbursts have a higher efficiency of converting gas into stars, as compared to typical star-forming galaxies at a given stellar mass, possibly indicative of different modes…
Beyond Spheroids and Discs: Classifications of CANDELS Galaxy Structure at 1.4 < z < 2 via Principal Component Analysis
Michael A. Peth, Jennifer M. Lotz, Peter E. Freeman +15
Important but rare and subtle processes driving galaxy morphology and star-formation may be missed by traditional spiral, elliptical, irregular or Sérsic bulge/disk classifications…