CaltechAUTHORS
Published May 10, 2010 | Version Published
Journal Article Open

No Evolution in the IR–Radio Relation for IR-luminous Galaxies at z < 2 in the COSMOS Field

Creators

  • 1. ROR icon Max Planck Institute for Astronomy
  • 2. ROR icon California Institute of Technology
  • 3. ROR icon National Radio Astronomy Observatory
  • 4. ROR icon Infrared Processing and Analysis Center
  • 5. ROR icon University of Paris
  • 6. ROR icon Laboratoire d'Astrophysique de Marseille
  • 7. ROR icon ETH Zurich
  • 8. ROR icon Max Planck Institute for Plasma Physics
  • 9. ROR icon NOIRLab
  • 10. ROR icon University of Hawaii at Manoa

Abstract

Previous observational studies of the infrared (IR)-radio relation out to high redshift employed any detectable star-forming systems at a given redshift within the restricted area of cosmological survey fields. Consequently, the evolution inferred relies on a comparison between the average IR/radio properties of (1) very IR-luminous high-z sources and (2) more heterogeneous low(er)-z samples that often lack the strongest IR emitters. In this Letter, we consider populations of objects with comparable luminosities over the last 10 Gyr by taking advantage of deep IR (especially Spitzer 24 μm) and Very Large Array 1.4 GHz observations of the COSMOS field. Consistent with recent model predictions, both Ultra Luminous Infrared Galaxies and galaxies on the bright end of the evolving IR luminosity function do not display any change in their average IR/radio ratios out to z ~ 2 when corrected for bias. Uncorrected data suggested ~0.3 dex of positive evolution.

Additional Information

© 2010 American Astronomical Society. Received 2010 January 12; accepted 2010 March 22; published 2010 April 12. Partly based on observations collected at the European Organization for Astronomical Research in the Southern Hemisphere, Chile, ESO program ID 175.A-0839. M.T.S. acknowledges DFG-funding (grant SCHI 536/3-2) and thanks Gianni Zamorani and Rob Ivison for reading and commenting on the manuscript. This work is partly based on observations made with the Spitzer Space Telescope, which is operated by NASA/JPL/ Caltech. The National Radio Astronomy Observatory (NRAO) is operated by Associated Universities, Inc., under cooperative agreement with the National Science Foundation. Facilities: VLA, Spitzer (IRAC, MIPS), VLT:Melipal, Subaru (SuprimeCam)

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Additional details

Identifiers

Eprint ID
18548
Resolver ID
CaltechAUTHORS:20100603-113404879

Funding

Deutsche Forschungsgemeinschaft (DFG)
SCHI 536/3-2

Dates

Created
2010-06-04
Created from EPrint's datestamp field
Updated
2021-11-08
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Caltech Custom Metadata

Caltech groups
Infrared Processing and Analysis Center (IPAC)