The radio properties of optically obscured Spitzer sources
arXiv:0710.2343 · doi:10.1111/j.1365-2966.2007.12576.x
Abstract
This paper analyses the radio properties of a subsample of optically obscured (R>25.5) galaxies observed at 24um by the Spitzer Space Telescope within the First Look Survey. 96 F[24um]>0.35 mJy objects out of 510 are found to have a radio counterpart at 1.4 GHz, 610 MHz or at both frequencies respectively down to ~40uJy and ~200uJy. IRAC photometry sets the majority of them in the redshift interval z [1-3] and allows for a broad distinction between AGN-dominated galaxies (~47% of the radio-identified sample) and systems powered by intense star-formation (~13%), the remaining objects being impossible to classify. The percentage of radio identifications is a strong function of 24um flux. The radio number counts at both radio frequencies suggest that the physical process(es) responsible for radio activity in these objects have a common origin regardless of whether the source shows mid-IR emission compatible with being an obscured AGN or a star-forming galaxy. We also find that both candidate AGN and star-forming systems follow (although with a large scatter) the relationship between 1.4 GHz and 24um fluxes reported by Appleton et al. (2004) which identifies sources undergoing intense star formation activity. On the other hand, the inferred radio spectral indices alpha indicate that a large fraction of objects in our sample (~60% of all galaxies with estimated alpha) may belong to the population of Ultra Steep Spectrum (USS) Sources, typically 'frustrated' radio-loud AGN. We interpret our findings as a strong indication for concurrent AGN and star-forming activity, whereby the 1.4 GHz flux is of thermal origin, while that at 610 GHz mainly stems from the nuclear source.
18 pages, 16 figures, to appear in MNRAS
References in corpus (14)
- The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
- Multiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges
- Deep ATLAS radio observations of the CDFS-SWIRE field
- Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 I: the Spectra
- A population of high-redshift type-2 quasars-I. Selection Criteria and Optical Spectra
- AGN and Starburst Classification from Spitzer Mid-Infrared Spectra for High Redshift SWIRE Sources
- The Spitzer Space Telescope Extra-Galactic First Look Survey: 24 micron data reduction, catalog, and source identification
- A search for distant radio galaxies from SUMSS and NVSS: III. radio spectral energy distributions and the z-alpha correlation
- The AGN Contribution to the Mid-IR Emission of Luminous Infrared Galaxies
- Extending the infrared radio correlation
- Deep 610-MHz GMRT observations of the Spitzer extragalactic First Look Survey field - I. Observations, data analysis and source catalogue
- A highly obscured and strongly clustered galaxy population discovered with the Spitzer Space Telescope
- A population of high-redshift type-2 quasars-II. Radio Properties
- Spatial clustering of USS sources and galaxies
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- The PEP Survey: Infrared Properties of Radio-Selected AGN
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- Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies