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Paper: Constraining the Connection Between the Far-UV and X-ray Continuum Using a Sample of 11 Quasars
Volume: 373, The Central Engine of Active Galactic Nuclei
Page: 141
Authors: Haro-Corzo, S.A.R.; Krongold, Y.; Binette, L.
Abstract: Using HST-FOS and Chandra-ACIS archived spectra of 11 quasars, we put constraints on how the far-UV and X-ray spectra may connect in the extreme-UV. We find that for 9 out of the 11 quasars, the interpolation of our UV best fit lies below or near to the observed X-ray flux, and that the soft X-ray excess component does not constitute a extension of the big blue bump.
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