Chasing Highly Obscured Qso2 In The Cosnos Field

Details Chasing Highly Obscured Qso2 In The Cosnos Field Chasing Highly Obscured Qso2 In The Cosnos Field

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21347106b&link_type=abstract

American Astronomical Society, AAS Meeting #213, #471.06; Bulletin of the American Astronomical Society, Vol. 41, p.423

Astronomy and Astrophysics

Astronomy

Scientific paper

We know today that the evolution of galaxies cannot be fully understood without taking into account their central SMBHs and the feedbacks induced by its active phases. Yet, despite much observational effort, the census of accreting SMBH through the cosmic epochs is still incomplete, and feedback mechanism between the AGN and its host galaxy remain little constrained. We will show how deep multiwavelength observations (from radio to X-rays) of the COSMOS and CDFS fields can be used to uncover a relatively large population of the long sought high luminosity but highly obscured, ``Compton thick QSOs'' at z=1-3, thus completing the AGN census in this redshift range.

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