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- W1618151446 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." @default.
- W1618151446 created "2016-06-24" @default.
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- W1618151446 date "2009-01-01" @default.
- W1618151446 modified "2023-09-25" @default.
- W1618151446 title "The IR to X-rays SED of the Heavily Obscured Quasar IRAS 09104+4109" @default.
- W1618151446 doi "https://doi.org/10.1063/1.3149424" @default.
- W1618151446 hasPublicationYear "2009" @default.
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