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X‐Ray Spectral Survey of WGACAT Quasars. I. Spectral Evolution and Low‐Energy Cutoffs

  • Authors: Fabrizio Fiore, Martin Elvis, Paolo Giommi, and Paolo Padovani

Fiore et al. 1998 The Astrophysical Journal 492 79.

  • Provider: AAS Journals

Caption: Fig. 3.

"Soft" effective spectral index (αS) plotted against the "hard" effective spectral index (αH) for (a) radio‐quiet quasars, and (b) radio‐loud quasars. Radio‐loud flat‐spectrum radio sources are identified by circles, steep radio spectrum sources by squares. High‐redshift quasars (z > 2.2) are shown with filled symbols. Three‐point spectra illustrate the radically different spectral shapes in different parts of the diagrams.

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