Publication Date:
2014-08-06
Description:
We present 90 cm Very Large Array imaging of the COSMOS field, comprising a circular area of 3.14 square degrees at 8.0arcsec x 6.0arcsec angular resolution with an average rms of 0.5 mJy beam –1 . The extracted catalogue contains 182 sources (down to 5.5), 30 of which are multicomponent sources. Using Monte Carlo artificial source simulations, we derive the completeness of the catalogue, and we show that our 90 cm source counts agree very well with those from previous studies. Using X-ray, NUV–NIR and radio COSMOS data to investigate the population mix of our 90 cm radio sample, we find that our sample is dominated by active galactic nuclei. The average 90–20 cm spectral index ( S α , where S is the flux density at frequency and α the spectral index) of our 90 cm selected sources is –0.70, with an interquartile range from –0.90 to –0.53. Only a few ultra-steep-spectrum sources are present in our sample, consistent with results in the literature for similar fields. Our data do not show clear steepening of the spectral index with redshift. Nevertheless, our sample suggests that sources with spectral indices steeper than –1 all lie at z 1, in agreement with the idea that ultra-steep-spectrum radio sources may trace intermediate-redshift galaxies ( z 1).
Print ISSN:
0035-8711
Electronic ISSN:
1365-2966
Topics:
Physics
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