2000ApJ...543..535T

We present BeppoSAX observations of three γ-ray-emitting quasars, namely, 0836+710, 1510-089, and 2230+114. The three objects have been detected up to ∼100 keV showing extremely flat power-law spectra above 2 keV (energy index α_2–10=0.3-0.5). The soft X-ray spectrum of 0836+710 implies either an absorption column density higher than the Galactic one or an intrinsically very hard slope (α_0.1–1=-0.2) below 1 keV. 1510-089 shows a soft excess, with the low-energy spectrum steeper (α_0.1–1=1.6) than the high-energy power law. The results are discussed in the framework of current inverse Compton models for the high-energy emission of flat-spectrum radio quasars and are used to estimate the physical quantities in the jet-emitting region and to shed light on the energy transport mechanisms in jets. Finally we discuss the estimates of the jet luminosity in the context of the Blandford & Znajek mechanism for jet production.