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Table · dataset · 2022

COSMOS-XS. II. Ultra-faint radio population

Listed in IVOA Registry (Virtual Observatory)

Ultra-deep radio surveys are an invaluable probe of dust-obscured star formation, but require a clear understanding of the relative contribution from radio active galactic nuclei (AGNs) to be used to their fullest potential.

Description

We study the composition of the {mu}Jy radio population detected in the Karl G. Jansky Very Large Array COSMOS-XS survey based on a sample of 1540 sources detected at 3GHz over an area of ~350arcmin^2^.

This ultra-deep survey consists of a single pointing in the well-studied COSMOS field at both 3 and 10GHz and reaches rms sensitivities of 0.53 and 0.41{mu}Jy/beam, respectively. We find multiwavelength counterparts for 97% of radio sources, based on a combination of near-UV/optical to sub-millimeter data, and through a stacking analysis at optical/near-IR wavelengths we further show that the sources lacking such counterparts are likely to be high-redshift in nature (typical z~4-5).

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Utilizing the multiwavelength data over COSMOS, we identify AGNs through a variety of diagnostics and find these to make up 23.2~1.3% of our sample, with the remainder constituting uncontaminated star-forming galaxies. However, more than half of the AGNs exhibit radio emission consistent with originating from star formation, with only 8.8~0.8% of radio sources showing a clear excess in radio luminosity. At flux densities of ~30{mu}Jy at 3GHz, the fraction of star formation-powered sources reaches ~90%, and this fraction is consistent with unity at even lower flux densities.

Overall, our findings imply that ultra-deep radio surveys such as COSMOS-XS constitute a highly effective means of obtaining clean samples of star formation-powered radio sources.

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Catalogue records · 2

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Stated by source
Radio
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Galactic astronomy 75%
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/apj/903/13915 d agoJSON v1
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