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A. V. Meshcheryakov

Researcher at Russian Academy of Sciences

Publications -  43
Citations -  468

A. V. Meshcheryakov is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Luminosity & Quasar. The author has an hindex of 9, co-authored 33 publications receiving 340 citations. Previous affiliations of A. V. Meshcheryakov include Sternberg Astronomical Institute & Samara National Research University.

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Stellar Mass—Halo Mass Relation and Star Formation Efficiency in High-Mass Halos

TL;DR: In this paper, the authors derived a relation between stellar mass and halo mass for high-mass halos using a sample of galaxy clusters with accurate measurements of stellar masses from optical and ifrared data and total masses from X-ray observations.
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SRG/eROSITA uncovers the most X-ray luminous quasar at z > 6

TL;DR: In this paper, the authors reported the discovery of X-ray emission from CFHQS J142952+544717, the most distant known radio-loud quasar at z=6.18, on Dec. 10-11, 2019 with the eROSITA telescope on board the SRG satellite during its ongoing all-sky survey.
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First tidal disruption events discovered by SRG/eROSITA: X-ray/optical properties and X-ray luminosity function at z < 0.6

TL;DR: In this paper, the first sample of TDEs discovered during the SRG all-sky survey was presented, which were selected among X-ray transients detected on the 0
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Period--luminosity relation for persistent LMXBs in the near-infrared

TL;DR: In this article, a simple model of an accretion disc and a secondary star reprocessing X-ray emission of a central compact object was proposed to describe the optical and near-infrared spectral energy distribution of LMXBs.
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Period-luminosity relation for persistent low-mass X-ray binaries in the near-infrared

TL;DR: In this article, a simple model of an accretion disc and a secondary star reprocessing X-ray emission from a central compact object was proposed to describe the optical and near-infrared spectral energy distributions of LMXBs.