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Obscured and Unobscured Active Galactic Nuclei in the Spitzer Space Telescope First Look Survey

Lacy, M. and Storrie-Lombardi, L. J. and Sajina, A. and Appleton, P. N. and Armus, L. and Chapman, S. C. and Choi, P. I. and Fadda, D. and Fang, F. and Frayer, D. T. and Heinrichsen, I. and Helou, G. and Im, M. and Marleau, F. R. and Masci, F. and Shupe, D. L. and Soifer, B. T. and Surace, J. and Teplitz, H. I. and Wilson, G. and Yan, L. (2004) Obscured and Unobscured Active Galactic Nuclei in the Spitzer Space Telescope First Look Survey. Astrophysical Journal Supplement Series, 154 (1). pp. 166-169. ISSN 0067-0049. doi:10.1086/422816.

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Selection of active galactic nuclei (AGNs) in the infrared facilitates the discovery of AGNs whose optical emission is extinguished by dust. In this paper, we use the Spitzer Space Telescope First Look Survey (FLS) to assess the fraction of AGNs with mid-infrared (MIR) luminosities that are comparable to quasars and that are missed in optical quasar surveys because of dust obscuration. We begin by using the Sloan Digital Sky Survey (SDSS) database to identify 54 quasars within the 4 deg^2 extragalactic FLS. These quasars occupy a distinct region in MIR color space by virtue of their strong, red continua. This has allowed us to define an MIR color criterion for selecting AGN candidates. About 2000 FLS objects have colors that are consistent with them being AGNs, but most are much fainter in the MIR than the SDSS quasars, which typically have 8 μm flux densities S_(8.0) ~ 1 mJy. We have investigated the properties of 43 objects with S_(8.0) ≥ 1 mJy that satisfy our AGN color selection. This sample should contain both unobscured quasars as well as AGNs that are absent from the SDSS survey because of extinction in the optical. After removing 16 known quasars, three probable normal quasars, and eight spurious or confused objects from the initial sample of 43, we are left with 16 objects that are likely to be obscured quasars or luminous Seyfert 2 galaxies. This suggests that the numbers of obscured and unobscured AGNs are similar in samples selected in the MIR at S_(8.0) ~ 1 mJy.

Item Type:Article
Related URLs:
URLURL TypeDescription Paper
Lacy, M.0000-0002-3032-1783
Storrie-Lombardi, L. J.0000-0002-5987-5210
Sajina, A.0000-0002-1917-1200
Appleton, P. N.0000-0002-7607-8766
Armus, L.0000-0003-3498-2973
Fadda, D.0000-0002-3698-7076
Frayer, D. T.0000-0003-1924-1122
Helou, G.0000-0003-3367-3415
Im, M.0000-0002-8537-6714
Masci, F.0000-0002-8532-9395
Shupe, D. L.0000-0003-4401-0430
Surace, J.0000-0001-7291-0087
Teplitz, H. I.0000-0002-7064-5424
Wilson, G.0000-0002-6572-7089
Yan, L.0000-0003-1710-9339
Additional Information:© 2004 The American Astronomical Society. Received 2004 March 26; accepted 2004 April 28. We thank Michael Gregg for assistance with the Lick observations, Susan Ridgway for advice and comments, B. Januzzi and A. Ford for the R-band survey, and J. Condon for the Very Large Array survey. We thank the SDSS team for targeting the FLS region in the DR1. This work is based on observations made with the Spitzer Space Telescope, operated by the Jet Propulsion Laboratory (JPL), California Institute of Technology, under NASA contract 1407. Support was provided by NASA through JPL. The SDSS Archive is funded by the Alfred P. Sloan Foundation, the Participating Institutions, NASA, the National Science Foundation, the US Department of Energy, the Japanese Monbukagakusho, and the Max Planck Society.
Group:Infrared Processing and Analysis Center (IPAC)
Funding AgencyGrant Number
Alfred P. Sloan FoundationUNSPECIFIED
Participating InstitutionsUNSPECIFIED
Department of Energy (DOE)UNSPECIFIED
Japanese MonbukagakushoUNSPECIFIED
Max Planck SocietyUNSPECIFIED
Subject Keywords:galaxies: Seyfert; infrared: galaxies; quasars: general
Issue or Number:1
Record Number:CaltechAUTHORS:20170327-155242177
Persistent URL:
Official Citation:M. Lacy et al 2004 ApJS 154 166
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:75445
Deposited By: Tony Diaz
Deposited On:27 Mar 2017 23:20
Last Modified:15 Nov 2021 16:33

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