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The Pedigrees of DOGs (Dust-Obscured Galaxies)

2009/05/27 by Arjun Dey, Dey, Arjun, the NDWFS/MIPS Collaboration +1
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomy and Astrophysical Research #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #Gamma-ray bursts and supernovae #astro-ph.CO

paper · pdf · doi:10.48550/arxiv.0905.4531

To appear in proceedings of "The Starburst-AGN Connection Conference", Oct 27-31 2008, Shanghai (ASP Conference Series). 6 pages

arxiv created 2009/05/27 · openalex publication_date 2009/05/27 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

A simple mid-infrared-to-optical color criterion of R-[24]>14 Vega mag results in a robust selection of approximately half of the redshift 2 ultraluminous infrared galaxy (ULIRG) population. These `Dust-Obscured Galaxies', or DOGs, have many properties that suggest that they are good candidates for systems in a transition phase between gas-rich mergers and QSOs.

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