Constraining the NH distribution of AGNs at high column densities and high X-ray luminosites is crucial to provide a reliable MIR/X-ray luminosity ratio distribution and compare it with the expectations of dust reprocessing models. Here we present the IR to X-rays broad band SED of of the hyperluminous infrared galaxy and Type 2 quasar IRAS 09104+4109 (z=0.442), taking into account our recent result suggesting the likely Compton-thin nature of its absorber.
The IR to X-rays SED of the heavily obscured quasar IRAS 09104+4109 / Lanzuisi G.; Piconcelli E.; Fiore F.; Feruglio C.; Maiolino R.; Vignali C.. - STAMPA. - 1126:(2009), pp. 242-244. (Intervento presentato al convegno Simbol-X: focusing on the hard X-ray Universe tenutosi a Parigi nel 2-5 Dicembre 2008).
The IR to X-rays SED of the heavily obscured quasar IRAS 09104+4109
LANZUISI, GIORGIO;VIGNALI, CRISTIAN
2009
Abstract
Constraining the NH distribution of AGNs at high column densities and high X-ray luminosites is crucial to provide a reliable MIR/X-ray luminosity ratio distribution and compare it with the expectations of dust reprocessing models. Here we present the IR to X-rays broad band SED of of the hyperluminous infrared galaxy and Type 2 quasar IRAS 09104+4109 (z=0.442), taking into account our recent result suggesting the likely Compton-thin nature of its absorber.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
