Constraining the Connection Between the Far-UV and X-ray Continuum Using a Sample of 11 Quasars

Details Constraining the Connection Between the Far-UV and X-ray Continuum Using a Sample of 11 Quasars Constraining the Connection Between the Far-UV and X-ray Continuum Using a Sample of 11 Quasars

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..141h&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Computer Science

Scientific paper

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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