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19992021
most citedThe eROSITA X-ray telescope on SRG

884 citations · 2k across the 35 of their papers we have counts for

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astro-ph2008★ 14 cited

Optical identification of hard X-ray source IGRJ18257-0707

R. A. Burenin, I. F. Bikmaev, M. G. Revnivtsev +4

We present the results of the optical identification of hard X-ray source IGRJ18257-0707 trough the spectroscopic observations of its optical counterpart with RTT150 telescope. Acc…

astro-ph2008★ 34 cited

Optical Identifications of Five INTEGRAL Hard X-ray Sources in the Galactic Plane Region

I. F. Bikmaev, R. A. Burenin, M. G. Revnivtsev +4

The results of optical identifications of five hard X-ray sources in the Galactic plane region from the INTEGRAL all-sky survey are presented. The X-ray data on one source (IGRJ202…

astro-ph2008★ 52 cited

Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z=3.2 gamma-ray burst

C. C. Thöne, D. A. Kann, G. Jóhannesson +58

Aims: With this paper we want to investigate the highly variable afterglow light curve and environment of gamma-ray burst (GRB) 060526 at . Methods: We present one of the…

astro-ph2008★ 17 cited

Several New Active Galactic Nuclei Among X-ray Sources Detected by INTEGRAL and SWIFT Observatories

R. A. Burenin, A. V. Mescheryakov, M. G. Revnivtsev +4

We present the results of the optical identifications of a set of X-ray sources from the all-sky surveys of INTEGRAL and SWIFT observatories. Optical data were obtained with Russia…

astro-ph2008★ 3 cited

Observations of GRB 060526 Optical Afterglow with Russian-Turkish 1.5-m Telescope

I. M. Khamitov, R. A. Burenin, I. F. Bikmaev +4

We present the results of the photometric multicolor observations of GRB 060526 optical afterglow obtained with Russian-Turkish 1.5-m Telescope (RTT150, Mt. Bakirlitepe, Turkey). T…

astro-ph2005★ 23 cited

Broad band variability of SS433: Accretion disk at work?

M. Revnivtsev, S. Fabrika, P. Abolmasov +6

We present broad band power spectra of variations of SS433 in radio, optical and X-ray spectral bands. We show that at frequencies lower than 1e-5 Hz the source demonstrates the sa…