AGN disk emission through X-ray and UV absorbers - iucaa
AGN disk emission through X-ray and UV absorbers - iucaa
AGN disk emission through X-ray and UV absorbers - iucaa
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Multi-wavelength SED for <strong>AGN</strong>• Red filled squares areobserved data points.• Near simultaneous X-<strong>ray</strong> <strong>and</strong>Optical data.SpitzerCompositeQSO• Infrared from Spitzer,2MASS <strong>and</strong> IRAS.IRAS2MASSHETCh<strong>and</strong>ra• Green filled squares are`average SED for <strong>AGN</strong>’ in <strong>UV</strong>(Telfer et.al. 2002).• The blue lines are arbitrary,simplistic joins between E<strong>UV</strong><strong>and</strong> X-<strong>ray</strong>.16 January 2011 Wide B<strong>and</strong> X-<strong>ray</strong> astronomy 5
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