Sargent, M. T. and Schinnerer, E. and Murphy, E. and Carilli, C. L. and Helou, G. and Aussel, H. and Le Floc'h, E. and Frayer, D. T. and Ilbert, O. and Oesch, P. and Salvato, M. and Smolčić, V. and Kartaltepe, J. and Sanders, D. B. (2010) No Evolution in the IR–Radio Relation for IR-luminous Galaxies at z < 2 in the COSMOS Field. Astrophysical Journal Letters, 714 (2). L190-L195. ISSN 0004-637X http://resolver.caltech.edu/CaltechAUTHORS:20100603-113404879
![[img]](http://authors.library.caltech.edu/style/images/fileicons/application_pdf.png)
|
PDF
- Published Version
See Usage Policy. 1270Kb |
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20100603-113404879
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.
| Item Type: | Article | ||||
|---|---|---|---|---|---|
| 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) | ||||
| Funders: |
| ||||
| Subject Keywords: | cosmology: observations; galaxies: active; galaxies: evolution; infrared: galaxies; radio continuum: galaxies; surveys | ||||
| Classification Code: | PACS: 98.54.Ep; 95.85.Bh; 98.80.Es; 98.62.Py; 95.85.Hp | ||||
| Record Number: | CaltechAUTHORS:20100603-113404879 | ||||
| Persistent URL: | http://resolver.caltech.edu/CaltechAUTHORS:20100603-113404879 | ||||
| Related URLs: | |||||
| Official Citation: | M. T. Sargent et al 2010 ApJ 714 L190 doi: 10.1088/2041-8205/714/2/L190 | ||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||
| ID Code: | 18548 | ||||
| Collection: | CaltechAUTHORS | ||||
| Deposited By: | Jason Perez | ||||
| Deposited On: | 04 Jun 2010 18:12 | ||||
| Last Modified: | 26 Dec 2012 12:06 |
Repository Staff Only: item control page
