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Spectral energy distributions and multiwavelength selection of type 1 quasars
Journal article   Open access

Spectral energy distributions and multiwavelength selection of type 1 quasars

Gordon T. Richards, Mark Lacy, Lisa J. Storrie-Lombardi, Patrick B. Hall, S. C. Gallagher, Dean C. Hines, Xiaohui Fan, Casey Papovich, Daniel E. Vanden Berk, George B. Trammell, …
The Astrophysical journal. Supplement series, v 166(2), pp 470-497
01 Oct 2006
url
https://resolver.caltech.edu/CaltechAUTHORS:20110719-112238177View
Accepted (AM)Open Access (License Unspecified) Open
url
https://doi.org/10.1086/506525View
Published, Version of Record (VoR) Open

Abstract

Astronomy & Astrophysics Physical Sciences Science & Technology
We present an analysis of the mid-infrared (MIR) and optical properties of type 1 (broad-line) quasars detected by the Spitzer Space Telescope. The MIR color- redshift relation is characterized to z similar to 3, with predictions to z = 7. We demonstrate how combining MIR and optical colors can yield even more efficient selection of active galactic nuclei (AGNs) than MIR or optical colors alone. Composite spectral energy distributions (SEDs) are constructed for 259 quasars with both Sloan Digital Sky Survey and Spitzer photometry, supplemented by near-IR, GALEX, VLA, and ROSAT data, where available. We discuss how the spectral diversity of quasars influences the determination of bolometric luminosities and accretion rates; assuming the mean SEDcan lead to errors as large as 50% for individual quasars when inferring a bolometric luminosity from an optical luminosity. Finally, we show that careful consideration of the shape of the mean quasar SED and its redshift dependence leads to a lower estimate of the fraction of reddened/obscured AGNs missed by optical surveys as compared to estimates derived from a single mean MIR to optical flux ratio.

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