Showing 1–20 of 32 results
/ Date/ Name
Nov 1, 2011Optical Spectroscopic Survey of High Latitude WISE Selected SourcesDec 5, 2011Direct Evidence for Termination of Obscured Star Formation by Radiatively Driven Outflows in Reddened QSOsApr 28, 2009Structures of Local Galaxies Compared to High Redshift Star-forming GalaxiesAug 11, 2014The FUV to Near-IR Morphologies of Luminous Infrared Galaxies in the GOALS SampleAug 2, 2019The Contribution of Galaxies to the $3.4\,\mathrm{μm}$ Cosmic Infrared Background as Measured Using WISEFeb 15, 2023Observational evidence for cosmological coupling of black holes and its implications for an astrophysical source of dark energyMay 3, 2012Mid-Infrared Selection of AGN with the Wide-Field Infrared Survey Explorer. I. Characterizing WISE-Selected AGN in COSMOSMay 17, 2012A New Population of High Redshift, Dusty Lyman-Alpha Emitters and Blobs Discovered by WISEDec 5, 2011Direct Evidence for Termination of Obscured Star Formation by Radiatively Driven Outflows in FeLoBAL QSOsJun 10, 2014Submillimetre observations of WISE-selected high-redshift, luminous, dusty galaxiesFeb 24, 2016Women in physics in the United States: recruitment and retentionJun 12, 2017Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like ClusterJun 17, 2016The Geometry of the Infrared and X-ray Obscurer in a Dusty Hyperluminous QuasarJan 28, 2025Molecular Gas Heating, Star Formation Rate Relations, and AGN Feedback in Infrared-luminous Galaxy MergersDec 13, 2022A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2Aug 27, 2012The First Hyper-Luminous Infrared Galaxy Discovered by WISENov 1, 2013WISE Discovery of Hyper Luminous Galaxies at z=2-4 and Their Implications for Galaxy and AGN EvolutionMay 7, 2017The role of the most luminous, obscured AGN in galaxy assembly at z~2Nov 17, 2025How accurately can obscured galaxy luminosities be measured using spectral energy distribution fitting of near- through far-infrared observations?Apr 29, 2022Stellar and black hole assembly in z<0.3 infrared-luminous mergers: intermittent starbursts vs. super-Eddington accretion