most citedThe outburst of the X-ray nova GRS 1739-278 in September, 2016

8 citations · 9 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2024

Deep Hard X-ray Survey of the M81 Field Based on INTEGRAL Data

R. Krivonos, I. Mereminskiy, S. Sazonov

We have carried out a deep survey of the M81 field in the 25-60 keV energy band based on long-term (2003-2023) INTEGRAL observations. A record sensitivity of 0.16 mCrab at a detect…

astro-ph.HE2024

Flickering pulsations in bright X-ray pulsars: the evidence of gravitationally lensed and eclipsed accretion column

Alexander A. Mushtukov, Albert Weng, Sergey S. Tsygankov +1

It is expected that extreme mass accretion rate onto strongly magnetised neutron star results in appearance of accretion columns above stellar surface. For a distant observer, rota…

astro-ph.HE2024

SRG/ART-XC Galactic Bulge deep survey. I. Maximum likelihood source detection algorithm for X-ray surveys

A. Semena, A. Vikhlinin, I. Mereminskiy +4

We describe an X-ray source detection method entirely based on the maximum likelihood analysis, in application to observations with the ART-XC telescope onboard the Spectrum Roentg…

astro-ph.GA2024

Nature of the diffuse emission sources in the H I supershell in the galaxy IC 1613

Anastasiya D. Yarovova, Alexei V. Moiseev, Ivan S. Gerasimov +6

We present a study of the nearby low-metallicity dwarf galaxy IC 1613, focusing on the search for massive stars and related feedback processes, as well as for faint supernova remna…

astro-ph.HE20231 cited

Hard X-rays and QPO in Swift J1727.8-1613: the rise and plateau of the 2023 outburst

I. Mereminskiy, A. Lutovinov, S. Molkov +5

We report on the detection of type-C quasi-periodic oscillations during the initial stages of the outburst of Swift J1727.8-1613 in 2023. Using data of the INTEGRAL observatory alo…

astro-ph.HE2023

Probing the nature of the X-ray source IGR J16327-4940 with Chandra

L. Sidoli, V. Sguera, K. Postnov +3

We report on the results of a Chandra observation of the source IGRJ16327-4940, suggested to be a high mass X-ray binary hosting a luminous blue variable star (LBV). The source fie…