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- W830476095 abstract "We present the results of a 100~ks Suzaku observation of the BLRG 3C390.3. The observations were performed to attempt to disentangle the contributions to the X-ray emission of this galaxy from an AGN and a jet component, via variability and/or the spectrum. The source was detected at high energies up to 80 keV, with a complex 0.3--80~keV spectrum. Preliminary analysis of the data shows significant flux variability, with the largest amplitudes at higher energies. Deconvolution of the spectrum shows that, besides a standard Seyfert-like spectrum dominating the 0.3--8keV emission, an additional, hard power law component is required, dominating the emission above 10 keV. We attribute this component to a variable jet." @default.
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- W830476095 date "2007-05-14" @default.
- W830476095 modified "2023-09-27" @default.
- W830476095 title "Suzaku Observations of the Broad-Line Radio Galaxy 3C390.3" @default.
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