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19 April 2024
 
  » arxiv » astro-ph/0402386

 Article overview


FIRST-2MASS Sources Below the APM Detection Threshold: A Population of Highly Reddened Quasars
Eilat Glikman ; Michael D. Gregg ; Mark Lacy ; David J. Helfand ; Robert H. Becker ; Richard L. White ;
Date 16 Feb 2004
Journal Astrophys.J. 607 (2004) 60-75
Subject astro-ph
Affiliation2,3), Mark Lacy , David J. Helfand , Robert H. Becker (2,3), Richard L. White ( Columbia Univeristy, U.C. Davis, IGPP, LLNL, Spitzer Science Center, STScI
AbstractWe have constructed a sample of bright near-infrared sources which are detected at radio wavelengths but undetected on the POSS I plates in order to search for a population of dust-obscured quasars. Optical and infrared spectroscopic followup of the sample has led to the discovery of seventeen heavily reddened quasars (B-K>6.5), fourteen of which are reported here for the first time. This has allowed us to define a region in the R-K, J-K color plane in which 50% of the radio-selected objects are highly reddened quasars. We compare the surface density of this previously overlooked population to that of UVX- radio-selected quasars, finding that they make up ~20% of the total quasar population for K < 15.5.
Source arXiv, astro-ph/0402386
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