The COSMOS survey from the radio perspective

Details The COSMOS survey from the radio perspective The COSMOS survey from the radio perspective

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..107s&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

Astronomy and Astrophysics

Astronomy

Radio Continuum, Galaxies, Surveys

Scientific paper

The COSMOS HST treasury project is a pan-chromatic imaging and spectroscopic survey of a 2 square-degree field designed to probe galaxy and SMBH (super-massive black hole) evolution as a function of cosmic environment. It is the largest contiguous field ever mapped by HST. Numerous state-of-the-art imaging campaigns at all wavelengths (X-ray to cm) are underway for the COSMOS HST field. The field is currently imaged at 1.4 GHz with the NRAO Very Large Array (VLA) as part of the VLA-COSMOS large project, a pilot project provided the initial astrometry for the entire COSMOS survey. The aim of the large VLA-COSMOS project is to study dust-obscured star formation and evolution of AGNs as a function of redshift and environment.

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