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Variability of X-ray pulsars in a hard energy band observed with INTEGRAL

Optical identifications of five INTEGRAL hard X-ray sources in the Galactic plane for the first time. The optical observations were performed with the 1.5-m RTT-150 telescope (Turkish National

Optical identification of the hard X-ray source IGR J18257-0707 associatedwith a faint optical object (m R ≈ 20.4) whose optical spectrumexhibits a broad H α emission line

Preliminary results of the alignment and Hartmann tests of the AZT-22 telescope

Variability of X-ray pulsars in a hard energy band observed with INTEGRAL

Optical identifications of five INTEGRAL hard X-ray sources in the Galactic plane for the first time. The optical observations were performed with the 1.5-m RTT-150 telescope (Turkish National

Optical identification of the hard X-ray source IGR J18257-0707 associatedwith a faint optical object (m R ≈ 20.4) whose optical spectrumexhibits a broad H α emission line

First simultanous X-ray and optical observations of rapid variability of supercritical accretor SS433

Observations of the optical afterglow from GRB 060526 with the RTT-150 telescope-Turkish 1.5-m RTT-150 telescope (Mount Bakyrlytepe, Turkey) are presented. The afterglow light curve

Preliminary results of the alignment and Hartmann tests of the AZT-22 telescope

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