Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-05-19
Astronomy and Astrophysics
Astrophysics
8 pages, TeX, 2 postscript figures; to appear in ApJ Letters
Scientific paper
10.1086/310787
We present a high-quality X-ray spectrum in the 3--53 keV rest-frame band of the radio-loud quasar 1508+5714, by far the brightest known X-ray source at z > 4. A simple power-law model with an absorption column density equal to the Galactic value in the direction of the source provides an excellent and fully adequate fit to the data; the measured power-law photon index Gamma = 1.42 (+0.13,-0.10). Upper limits to Fe K alpha line emission and Compton-reflection components are derived. We offer evidence for both X-ray and radio variability in this object and provide the first contemporaneous radio spectrum (alpha = -0.25). The data are all consistent with a picture in which the emission from this source is dominated by a relativistically beamed component in both the X-ray and radio bands.
Helfand David J.
Moran Edward C.
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