activity
19972021
most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 15.3k across the 144 of their papers we have counts for

collaborators

145 papers

astro-ph.GA2021★ 36 cited

Kinematics and Star Formation of High-Redshift Hot Dust-Obscured Quasars as Seen by ALMA

Tanio Diaz-Santos, Roberto J. Assef, Peter R. M. Eisenhardt +9

Hot, dust-obscured galaxies (Hot DOGs) are a population of hyper-luminous obscured quasars identified by WISE. We present ALMA observations of the [CII] fine-structure line and und…

astro-ph.IM2020★ 318 cited

The CatWISE2020 Catalog

Federico Marocco, Peter R. M. Eisenhardt, John W. Fowler +20

The CatWISE2020 Catalog consists of 1,890,715,640 sources over the entire sky selected from WISE and NEOWISE survey data at 3.4 and 4.6 m (W1 and W2) collected from 2010 Jan. 7…

astro-ph.SR2020★ 171 cited

The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs

J. Davy Kirkpatrick, Christopher R. Gelino, Jacqueline K. Faherty +49

We present final Spitzer trigonometric parallaxes for 361 L, T, and Y dwarfs. We combine these with prior studies to build a list of 525 known L, T, and Y dwarfs within 20 pc of th…

astro-ph.GA2020★ 35 cited

Fast Outflows in Hot Dust-Obscured Galaxies with Keck/NIRES

Luke Finnerty, Kirsten Larson, B. T. Soifer +10

We present rest-frame optical spectroscopic observations of 24 Hot Dust-Obscured Galaxies (Hot DOGs) at redshifts 1.7-4.6 with KECK/NIRES. Our targets are selected based on their e…

astro-ph.GA2020★ 8 cited

The Massive and Distant Clusters of WISE Survey. VIII. Radio Activity in Massive Galaxy Clusters

Wenli Mo, Anthony Gonzalez, Mark Brodwin +6

We present a study of the central radio activity of galaxy clusters at high redshift. Using a large sample of galaxy clusters at from the Massive and Distant Clusters o…

astro-ph.GA2020★ 15 cited

Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation

Stacey Alberts, Kyoung-Soo Lee, Alexandra Pope +13

Massive galaxy clusters undergo strong evolution from z~1.6 to z~0.5, with overdense environments at high-z characterized by abundant dust-obscured star formation and stellar mass…