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Spectroscopic Redshift Measurements for Galaxy Clusters Detected in the Planck All-Sky Survey
Zaznobin I.A., Burenin R.A., Bikmaev I.F., Khamitov I.M., Khorunzhev G.A., Lyapin A.R., Eselevich M.V., Afanasiev V.L., Dodonov S.N., Sunyaev R.A.
observations of these galaxy clusters have been carried out with the 1.5-m Russian–Turkish telescope (RTT150
Optical Identifications of Galaxy Clusters Among Objects from the Second Planck Catalogue of Sunyaev–Zeldovich Sources
Zaznobin I., Burenin R., Bikmaev I., Khamitov I., Khorunzhev G., Konoplev V., Eselevich M., Afanasiev V., Dodonov S., Rubiño-Martín J., Aghanim N., Sunyaev R.
-Zeldovich sources. We used the data of observations with the 1.5-m Russian-Turkish telescope (RTT150), the 1.6-m
Observation of a Very Massive Galaxy Cluster at z = 0.76 in the SRG/eROSITA All-Sky Survey
Burenin R.A., Bikmaev I.F., Gilfanov M.R., Grokhovskaya A.A., Dodonov S.N., Eselevich M.V., Zaznobin I.A., Irtuganov E.N., Lyskova N.S., Medvedev P.S., Meshcheryakov A.V., Moiseev A.V., Sazonov S.Y., Starobinsky A.A., Sunyaev R.A., Uklein R.I., Khabibullin I.I., Khamitov I.M., Churazov E.M.
–Zeldovich effect. The spectroscopic redshift has been measured at the 6-m BTA telescope, z=0.7573. In addition
The First Distant X-ray Quasars (z ~ 4) among the Sources Discovered by the eROSITA Telescope of the SRG Orbital Observatory during a Deep Lockman Hole Survey
Khorunzhev G.A., Meshcheryakov A.V., Burenin R.A., Lyapin A.R., Medvedev P.S., Sazonov S.Y., Eselevich M.V., Sunyaev R.A., Gilfanov M.R.
. The spectroscopic observations of the first two candidates from this list carried out with the 1.6-m AZT-33IK
Spectroscopic Redshift Measurements for Galaxy Clusters from the Planck Survey and Observations of These Clusters in the SRG/eROSITA Survey
Zaznobin I.A., Burenin R.A., Bikmaev I.F., Khamitov I.M., Khorunzhev G.A., Lyapin A.R., Eselevich M.V., Lyskova N.S., Medvedev P.S., Gilfanov M.R., Sunyaev R.A.
out during 2019–early 2020 at the 1.6-m AZT-33IK telescope of the Sayan Observatory and the 1.5-m
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
Zaznobin I.A., Uskov G.S., Sazonov S.Y., Burenin R.A., Medvedev P.S., Khorunzhev G.A., Lyapin A.R., Krivonos R.A., Filippova E.V., Gilfanov M.R., Sunyaev R.A., Eselevich M.V., Bikmaev I.F., Irtuganov E.N., Nikolaeva E.A.
catalogue of X-ray sources detected in the 4–12 keV energy band by the Mikhail Pavlinsky ART-XC telescope
First tidal disruption events discovered by SRG/eROSITA: X-ray/optical properties and X-ray luminosity function at z < 0.6
Sazonov S., Gilfanov M., Medvedev P., Yao Y., Khorunzhev G., Semena A., Sunyaev R., Burenin R., Lyapin A., Meshcheryakov A., Uskov G., Zaznobin I., Postnov K.A., Dodin A.V., Belinski A.A., Cherepashchuk A.M., Eselevich M., Dodonov S.N., Grokhovskaya A.A., Kotov S.S., Bikmaev I.F., Zhuchkov R.Y., Gumerov R.I., Van Velzen S., Kulkarni S.
. The X-ray spectra are consistent with nearly critical accretion on to black holes of a few ×103 to 108M
Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye
Wyrzykowski, Mróz P., Rybicki K.A., Gromadzki M., Kołaczkowski Z., Zieliński M., Zieliński P., Britavskiy N., Gomboc A., Sokolovsky K., Hodgkin S.T., Abe L., Aldi G.F., Almannaei A., Altavilla G., Al Qasim A., Anupama G.C., Awiphan S., Bachelet E., Baklş V., Baker S., Bartlett S., Bendjoya P., Benson K., Bikmaev I.F., Birenbaum G., Blagorodnova N., Blanco-Cuaresma S., Boeva S., Bonanos A.Z., Bozza V., Bramich D.M., Bruni I., Burenin R.A., Burgaz U., Butterley T., Caines H.E., Caton D.B., Calchi Novati S., Carrasco J.M., Cassan A., Epas V., Cropper M., Chruślińska M., Clementini G., Clerici A., Conti D., Conti M., Cross S., Cusano F., Damljanovic G., Dapergolas A., D'Ago G., De Bruijne J.H.J., Dennefeld M., Dhillon V.S., Dominik M., Dziedzic J., Erece O., Eselevich M.V., Esenoglu H., Eyer L., Figuera Jaimes R., Fossey S.J., Galeev A.I., Grebenev S.A., Gupta A.C., Gutaev A.G., Hallakoun N., Hamanowicz A., Han C., Handzlik B., Haislip J.B., Hanlon L., Hardy L.K., Harrison D.L., Van Heerden H.J., Hoette V.L., Horne K., Hudec R., Hundertmark M., Ihanec N., Irtuganov E.N., Itoh R., Iwanek P., Jovanovic M.D., Janulis R., Jelínek M., Jensen E., Kaczmarek Z., Katz D., Khamitov I.M., Kilic Y., Klencki J., Kolb U., Kopacki G., Kouprianov V.V., Kruszyńska K., Kurowski S., Latev G.
is composed of two main-sequence stars with masses 0.57 ± 0.05 M? and 0.36 ± 0.03 M? at 780 pc
Current rabies epizootiology
Makarov V.V., Dzhupina S.I., Vedernikov V.A., Zavodskikh A.V., Afonin V.N., Baldina I.V.
Poster: Intensive learning technologies as a trend in education digitalization
Aksyanova A.V., Barabanova S.V., Kraysman N.V., Nikonova N.V., Nasonkin V.V.

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