IR SEDs of AGNs and Search for Compton-thick Accretion in AKARI NEP DEEP Field

Details IR SEDs of AGNs and Search for Compton-thick Accretion in AKARI NEP DEEP Field IR SEDs of AGNs and Search for Compton-thick Accretion in AKARI NEP DEEP Field

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..170m&link_type=abstract

XMM-Newton Proposal ID #05045902

Astronomy and Astrophysics

Astronomy

Cosmology, Extragalactic Deep Fields And Area Surveys, Akari Nep Deep, Akari Nep Deep, Xmm-Newton Proposal 05045902

Scientific paper

We propose to make two XMM-Newton medium-deep exposures on AKARI (Astro-F) NEP Deep Field, which is a subject of a key legacy survey with the infrared satellite AKARI. Its continuous 2-24 micron photometry in 9 bands, filling the Spitzer s gap at the 15 micron band, makes it an unique and powerful tool for infrared discrimination of AGNs, normal, and star-forming galaxies. We intend to use XMM-Newton to characterize the IR Spectral Energy Distribution (SED) of the AGNs component and its ratio with X-ray unabsorbed luminosity. We further intend to search for Compton-thick AGNs using the IR SED and X-ray upper limits.

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