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SRG/eROSITA uncovers the most X-ray luminous quasar at z > 6

Monthly notices of the Royal Astronomical Society, 2020-09, Vol.497 (2), p.1842-1850

2020

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The intermediate nebular phase of SN 2014J: onset of clumping as the source of recombination

Monthly notices of the Royal Astronomical Society, 2020-05, Vol.494 (2), p.2809-2822

2020

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Modelling of 35-d superorbital cycle of B and V light curves of IMXB HZ Her/Her X-1

Monthly notices of the Royal Astronomical Society, 2020-12, Vol.499 (2), p.1747-1757

2020

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Refined Parameters of the Pre-Cataclysmic Variable with the sdB Sub-Dwarf SDSS J162256.6+473051

Astrophysical bulletin, 2022-12, Vol.77 (4), p.415-421

2022

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Investigation of the Disk of the Be Star in the High-Mass X-ray Binary IGR J21343+4738

Astronomy letters, 2023-11, Vol.49 (11), p.697-705

2023

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Detection of AGNs and Quasars with Significant Proper Motions Based on Gaia Data in the SRG/eROSITA Catalog of X-ray Sources

Astronomy letters, 2022-12, Vol.48 (12), p.724-734

2022

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Observations of Candidates for Eclipsing Cataclysmic Variables with the RTT-150 Telescope

Astronomy letters, 2021-10, Vol.47 (10), p.695-704

2021

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SRGe J214919.3+673634—a Candidate for AM Her Variables Discovered by the eROSITA Telescope onboard the Spectrum–Roentgen–Gamma Orbital Observatory

Astronomy letters, 2022-09, Vol.48 (9), p.530-541

2022

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Optical Identification of Candidates for Active Galactic Nuclei Detected by the Mikhail Pavlinsky ART-XC Telescope Onboard the SRG Observatory during an All-Sky X-ray Survey

Astronomy letters, 2021-02, Vol.47 (2), p.71-87

2021

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Accretion processes in astrophysics

Physics Uspekhi, 2019-11, Vol.62 (11), p.1126-1135

2019

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Spectroscopic Redshift Determination for a Sample of Distant Quasars Detected by the SRG Observatory Based on RTT-150 Observations. I

Astronomy letters, 2020-10, Vol.46 (10), p.645-657

2020

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Spectroscopic Redshift Determination for a Sample of Distant Quasars Detected by the SRG Observatory Based on RTT-150 Observations. II

Astronomy letters, 2021-05, Vol.47 (5), p.277-290

2021

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Observation of a Very Massive Galaxy Cluster at = 0.76 in the SRG/eROSITA All-Sky Survey

Astronomy letters, 2021, Vol.47 (7), p.443-453

2021

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Additional spectroscopic redshift measurements for galaxy clusters from the first Planck catalogue

Astronomy letters, 2016-02, Vol.42 (2), p.63-68

2016

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Spectroscopic study of the optical counterpart to the fast X-ray transient IGR J17544-2619 based on observations at the 1.5-m RTT-150 telescope

Astronomy letters, 2017-10, Vol.43 (10), p.664-676

2017

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On the nature of the 35-day cycle in the X-ray binary Her X-1/HZ Her

Proceedings of the International Astronomical Union, 2018-08, Vol.14 (S346), p.281-287

2018

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PG 1316+678: A young pre-cataclysmic binary with weak reflection effects

Astronomy reports, 2013-03, Vol.57 (3), p.212-221

2013

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Investigation of the parameters of the massive binary X-ray system IGR J17544-2619

Bulletin of the Crimean Astrophysical Observatory, 2013-06, Vol.109 (1), p.27-31

2013

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Optical identification and follow-up observations of SRGA J213151.5+491400: A new magnetic cataclysmic variable discovered with the SRG observatory

Astronomy and astrophysics (Berlin), 2024-04, Vol.684, p.A190

2024

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A Jupiter-mass planet around the K0 giant HD 208897

Astronomy and astrophysics (Berlin), 2017-12, Vol.608, p.A14

2017

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Confirmation of the Sublimation Activity of the Primitive Main-Belt Asteroids 779 Nina, 704 Interamnia, and 145 Adeona, as well as its Probable Spectral Signs on 51 Nemausa and 65 Cybele

Solar system research, 2019-07, Vol.53 (4), p.261-277

2019

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Observation of a Very Massive Galaxy Cluster at $$\boldsymbol{z}$$ = 0.76 in the SRG/eROSITA All-Sky Survey

Astronomy letters, 2021-07, Vol.47 (7), p.443-453

2021

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Low mass stellar companions around four giant stars

New astronomy, 2015-01, Vol.34, p.108-113

2015

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Accretion processes in astrophysics

Uspehi fiziceskih nauk, 2019-11, Vol.189 (11), p.1202-1212

2019

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SRG/eROSITA uncovers the most X-ray luminous quasar at z > 6

The intermediate nebular phase of SN 2014J: onset of clumping as the source of recombination

Modelling of 35-d superorbital cycle of B and V light curves of IMXB HZ Her/Her X-1

Refined Parameters of the Pre-Cataclysmic Variable with the sdB Sub-Dwarf SDSS J162256.6+473051

Investigation of the Disk of the Be Star in the High-Mass X-ray Binary IGR J21343+4738

Detection of AGNs and Quasars with Significant Proper Motions Based on Gaia Data in the SRG/eROSITA Catalog of X-ray Sources

Observations of Candidates for Eclipsing Cataclysmic Variables with the RTT-150 Telescope

SRGe J214919.3+673634—a Candidate for AM Her Variables Discovered by the eROSITA Telescope onboard the Spectrum–Roentgen–Gamma Orbital Observatory

Optical Identification and Spectroscopic Redshift Measurements of 216 Galaxy Clusters from the SRG/eROSITA All-Sky Survey

Optical Identification of Candidates for Active Galactic Nuclei Detected by the Mikhail Pavlinsky ART-XC Telescope Onboard the SRG Observatory during an All-Sky X-ray Survey

Accretion processes in astrophysics

Spectroscopic Redshift Determination for a Sample of Distant Quasars Detected by the SRG Observatory Based on RTT-150 Observations. I

Spectroscopic Redshift Determination for a Sample of Distant Quasars Detected by the SRG Observatory Based on RTT-150 Observations. II

Observation of a Very Massive Galaxy Cluster at = 0.76 in the SRG/eROSITA All-Sky Survey

Additional spectroscopic redshift measurements for galaxy clusters from the first Planck catalogue

Spectroscopic study of the optical counterpart to the fast X-ray transient IGR J17544-2619 based on observations at the 1.5-m RTT-150 telescope

On the nature of the 35-day cycle in the X-ray binary Her X-1/HZ Her

PG 1316+678: A young pre-cataclysmic binary with weak reflection effects

Investigation of the parameters of the massive binary X-ray system IGR J17544-2619

Optical identification and follow-up observations of SRGA J213151.5+491400: A new magnetic cataclysmic variable discovered with the SRG observatory

A Jupiter-mass planet around the K0 giant HD 208897

Confirmation of the Sublimation Activity of the Primitive Main-Belt Asteroids 779 Nina, 704 Interamnia, and 145 Adeona, as well as its Probable Spectral Signs on 51 Nemausa and 65 Cybele

Observation of a Very Massive Galaxy Cluster at $$\boldsymbol{z}$$ = 0.76 in the SRG/eROSITA All-Sky Survey

Low mass stellar companions around four giant stars

Accretion processes in astrophysics

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