The population of faint radio sources in the GOODS-South field

Details The population of faint radio sources in the GOODS-South field The population of faint radio sources in the GOODS-South field

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..125a&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Physics

Galaxies: Evolution, Galaxies: Starburst, Radio Continuum: Galaxies

Scientific paper

Insensitive to dust obscuration, radio wavelengths are ideal to select star-forming galaxies free of dust induced biases. Using the superb optical and X-ray data available in the GOODS-South field, the diversity of sub-mJy and microJansky radio sources is analysed. The superb HST ACS image quality allows investigations on the relation of star-formation to morphology in radio-selected star-forming galaxies, to faint optical magnitudes - an example of such analyses is given. The nature of the optically/X-ray unidentified microJansky radio sources is discussed.

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