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Signals from the Noise: Image Stacking for Quasars in the FIRST Survey

White, Richard L. and Helfand, David J. and Becker , Robert H. and Glikman, Eilat and de Vries, Wim (2007) Signals from the Noise: Image Stacking for Quasars in the FIRST Survey. Astrophysical Journal, 654 (1). pp. 99-114. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20091118-111436893

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Abstract

We present a technique to explore the radio sky into the nanojansky regime by employing image stacking using the FIRST survey. We first discuss the nonintuitive relationship between the mean and median values of a non-Gaussian distribution that is dominated by noise, followed by an analysis of the systematic effects present in FIRST's 20 cm VLA snapshot images. Image stacking allows us to recover the properties of source populations with flux densities a factor of 30 or more below the rms noise level. Mean estimates of radio flux density, luminosity, etc. are derivable for any source class having arcsecond positional accuracy. We use this technique to compute the mean radio properties for 41,295 quasars from the SDSS DR3 catalog. There is a tight correlation between optical and radio luminosity, with the radio luminosity increasing as the 0.85 power of optical luminosity. This implies declining radio loudness with optical luminosity: the most luminous objects (M_(UV) = -28.5) have average radio-to-optical ratios 3 times lower than the least luminous objects (M_(UV) = -20). There is also a striking correlation between optical color and radio loudness: quasars that are either redder or bluer than the norm are brighter radio sources, with objects 0.8 mag redder than the SDSS composite spectrum having radio loudness ratios that are higher by a factor of 10. We explore the long-standing question of whether a radio-loud/radio-quiet dichotomy exists in quasars, finding that optical selection effects probably dominate the distribution function of radio loudness, which has at most a modest (~20%) inflection between the radio-loud and radio-quiet ends of the distribution. We also find, surprisingly, that broad absorption line quasars have higher mean radio flux densities, with the greatest disparity arising in the rare low-ionization BAL subclass.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/507700DOIUNSPECIFIED
http://www.iop.org/EJ/abstract/0004-637X/654/1/99PublisherUNSPECIFIED
Additional Information:© 2007 American Astronomical Society. Print publication: Issue 1 (2007 January 1); received 2006 May 2; accepted for publication 2006 July 14. Thanks to Gordon Richards for helpful comments on a draft of this paper. The authors acknowledge the support of the National Science Foundation under grants AST 00-98355 (R. H. B.) and AST 00-98259 (D. J. H. and E.G.). The work of R. H. B. was also supported in part under the auspices of the US Department of Energy by Lawrence Livermore National Laboratory under contractW- 7405-ENG-48. R. L.W. acknowledges the support of the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy under NASA contract NAS5-26555.
Funders:
Funding AgencyGrant Number
NSFAST 00-98355
NSFAST 00-98259
U. S. Department of Energy by Lawrence Livermore National LaboratoryW-7405-ENG-48
NASANAS5-26555
Subject Keywords:catalogs; quasars: absorption lines; quasars: general; radio continuum: general; surveys
Record Number:CaltechAUTHORS:20091118-111436893
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20091118-111436893
Official Citation:Signals from the Noise: Image Stacking for Quasars in the FIRST Survey Richard L. White, David J. Helfand, Robert H. Becker, Eilat Glikman, and Wim de Vries 2007 ApJ 654 99-114 doi: 10.1086/507700
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:16747
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:18 Nov 2009 21:34
Last Modified:27 Mar 2014 19:44

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