Mid-infrared galaxy luminosity function from AGN Virtual Observatory Resource

Authors
  1. Dai X.
  2. Assef R.J.
  3. Kochanek C.S.
  4. Brodwin M.
  5. Brown M.J.I.
  6. Caldwell N.,Cool R.J.
  7. Dey A.
  8. Eisenhardt P.
  9. Eisenstein D.
  10. Gonzalez A.H.,Jannuzi B.T.
  11. Jones C.
  12. Murray S.S.
  13. Stern D.
  14. Published by
    CDS
Abstract

We present galaxy luminosity functions at 3.6, 4.5, 5.8, and 8.0um measured by combining photometry from the IRAC Shallow Survey with redshifts from the AGN and Galaxy Evolution Survey (AGES) of the NOAO Deep Wide-Field Survey Bootes field. The well defined IRAC samples contain 3800-5800 galaxies for the 3.6-8.0um bands with spectroscopic redshifts and z<0.6. We obtained relatively complete luminosity functions in the local redshift bin of z<0.2 for all four IRAC channels that are well fitted by Schechter functions.

Keywords
  1. active-galactic-nuclei
  2. infrared-photometry
Bibliographic source Bibcode
2009ApJ...697..506D
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/697/506
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/697/506
Document Object Identifer DOI
doi:10.26093/cds/vizier.16970506

Access

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/697/506
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/697/506
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/697/506
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
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History

2012-01-16T09:13:18Z
Resource record created
2012-01-16T09:13:18Z
Created
2012-01-29T12:22:49Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr