The contribution of X-ray selected sources to the Sub-millimeter Background

Details The contribution of X-ray selected sources to the Sub-millimeter Background The contribution of X-ray selected sources to the Sub-millimeter Background

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..270s&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

1

Active Galaxies: Sub-Millimeter, X-Ray

Scientific paper

The connection between the sub-millimeter (sub-mm) and hard X-ray background (XRB) has been studied by comparing data at 2-10 keV and at 850 mu m for a sample of 54 sources. At the limiting fluxes reached in our sample most of the background ( ~ 70%) in the two bands has been resolved into discrete sources. We find that sources making most of the X-ray background do not contribute significantly to the sub-mm background.

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