XMM-Newton discovery of soft X-ray absorption in the high-z superluminous Blazar RBS 315

Details XMM-Newton discovery of soft X-ray absorption in the high-z superluminous Blazar RBS 315 XMM-Newton discovery of soft X-ray absorption in the high-z superluminous Blazar RBS 315

2005-09-16

arxiv.org/abs/astro-ph/0509488v1

Astronomy and Astrophysics

Astrophysics

Accepted by A&A Letters

Scientific paper

10.1051/0004-6361:200500189

We present the analysis and the results of a 20 ks XMM-Newton observation of the extremely X-ray loud (L_X ~ 5 x 10^{47} erg/s) flat-spectrum radio quasar RBS 315 at a redshift of 2.69. This EPIC observation has allowed us to strongly constrain the slope of the continuum (Gamma = 1.23+/-0.01) as well as to discover the presence of a sharp drop below ~ 2 keV in its spectrum. Such a flat photon index and the huge luminosity suggest that the X-ray emission is due to the low energy tail of the Comptonized spectrum, produced from plasma in a relativistic jet oriented close to our line of sight. Even though the hypothesis of a break in the continuum cannot be completely discarded as an explanation of the soft X-ray cutoff, the presence of intrinsic absorption appears more plausible. Spectral fits with cold (Nh(z) = 1.62+/-0.09 x 10^{22} cm^{-2}) and lukewarm (Nh(z) = 2.2^{+0.9}_{-0.3} x 10^{22} cm^{-2}; xi = 15^{+38}_{-12} erg/cm^{2}/s) absorbers are statistically indistinguishable. Remarkably, our results are very similar to those reported so far for other absorbed high-z Blazars observed by XMM-Newton. The existence of this ``homogeneous'' class of jet-dominated superluminous obscured QSOs at high z therefore could be important in the context of the formation and cosmological evolution of radio-loud objects

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