Soft X‐Ray Properties of Flat‐Spectrum Radio Quasars

We report the soft X-ray properties of 41 flat-spectrum radio quasars (FSRQs), derived by cross-correlating literature blazar samples with the ROSAT PSPC archive of pointed observations. The redshifts of the sources span the range z = 0-3. The 0.1-2.4 keV spectra of FSRQs are well described by a single power law modified by column densities of neutral gas consistent with Galactic values. Spectral flattening/steepening at the lower energies is present in only 4/41 and 2/41 sources, respectively. The ROSAT photon indices of FSRQs span a wide range, 0.5 ≲ Γ ≲ 2.5, and have a measurable intrinsic dispersion; only in part is the spread of slopes due to a redshift effect. The rest-frame ROSAT spectral indices of FSRQs are statistically indistinguishable from low-energy peaked BL Lacs and flatter than high-energy peaked BL Lacs, although with several FSRQs having soft X-ray spectra as steep as HBLs. Similarly, while the bulk of FSRQs are intrinsically X-ray brighter than both types of BL Lacs, the X-ray luminosity distributions of the three classes have a large overlap. The ROSAT spectra of 13 FSRQs are steeper than measured with the Einstein IPC (0.3-4.5 keV), indicating a flat tail emerging at ≈ 1-2 keV at rest-frame energies. We find a trend for blazars with stronger optical emission lines to be more γ-ray-loud and to have flatter X-ray-to-γ-ray continua, possibly supporting external Compton scattering models as the primary generation mechanisms of the high-energy continuum in these objects.

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