activity
20172020
most citedSRG/eROSITA uncovers the most X-ray luminous quasar at z>6

54 citations · 94 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE20205 cited

Modeling of 35-day superorbital cycle of and light curves of IMXB HZ Her/Her X-1

D. A. Kolesnikov, N. I. Shakura, K. A. Postnov +13

The X-ray binary Her X-1 consists of an accreting neutron star and the optical component HZ Her. The 35-day X-ray superorbital variability of this system is known since its discove…

astro-ph.HE202054 cited

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

P. Medvedev, S. Sazonov, M. Gilfanov +6

We report 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 th…

astro-ph.HE202017 cited

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

P. A. Mazzali, I. Bikmaev, R. Sunyaev +6

At the age of about 1 year, the spectra of most Type Ia supernovae are dominated by strong forbidden nebular emission lines of FeII and FeIII. Later observations (at about 2 years)…

astro-ph.SR2019

Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye

Łukasz Wyrzykowski, P. Mróz, K. A. Rybicki +182

Gaia16aye was a binary microlensing event discovered in the direction towards the northern Galactic disc and was one of the first microlensing events detected and alerted to by the…

astro-ph.HE20177 cited

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

I. F. Bikmaev, E. A. Nikolaeva, V. V. Shimansky +7

We present the results of our long-term photometric and spectroscopic observations at the Russian-Turkish RTT-150 telescope for the optical counterpart to one of the best-known sou…

astro-ph.SR201711 cited

A Jupiter-mass planet around the K0 giant HD 208897

M. Yılmaz, B. Sato, I. Bikmaev +9

For over 10 years, we have carried out a precise radial velocity (RV) survey to find substellar companions around evolved G,K-type stars to extend our knowledge of planet formation…