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An Upper Limit on Nickel Overabundance in the Supercritical Accretion Disk Wind of SS 433 from X-ray Spectroscopy
DOI: 10.1134/S1063773718060038 Bibcode: 2018AstL...44..390M

Medvedev, P. S.; Tsygankov, S. S.; Sazonov, S. Yu. +2 more

We analyze a long (with a total exposure time of 120 ks) X-ray observation of the unique Galactic microquasar SS 433 carried out by the XMM-Newton space observatory with the goal of searching for the fluorescent line of neutral (or weakly ionized) nickel at energy 7.5 keV. We consider two models for the formation of fluorescent lines in the spectr…

2018 Astronomy Letters
XMM-Newton 12
Optical Identification of X-ray Sources from the 14-Year INTEGRAL All-Sky Survey
DOI: 10.1134/S1063773718090037 Bibcode: 2018AstL...44..522K

Medvedev, P. S.; Lutovinov, A. A.; Eselevich, M. V. +6 more

We present the results of our optical identifications of several hard X-ray sources from the INTEGRAL all-sky survey obtained over 14 years of observations. Having improved the positions of these objects in the sky with the X-ray telescope (XRT) of the Swift observatory and the XMMNewton observatory, we have identified their counterparts using opt…

2018 Astronomy Letters
INTEGRAL XMM-Newton 8
X-ray Luminosity Function of Quasars at 3 < z < 5 from XMM-Newton Serendipitous Survey Data
DOI: 10.1134/S1063773718090049 Bibcode: 2018AstL...44..500K

Sazonov, S. Yu.; Khorunzhev, G. A.; Burenin, R. A.

The X-ray luminosity function of distant (3 < z < 5.1) type 1 quasars has been measured. A sample of distant high-luminosity (1045 erg s-1 ≤ L X,2-10 < 7.5×1045 erg s-1 in the 2-10 keV energy band) quasars from the catalog by Khorunzhev et al. (2016) compiled from the data of the 3XMM…

2018 Astronomy Letters
XMM-Newton 7