activity
20032026
most citedINTEGRAL observations of SS433: Results of coordinated campaign

91 citations · 615 across the 31 of their papers we have counts for

collaborators

33 papers

astro-ph.HE2026

X-ray spectral scaling of black hole mass in quasi-periodic eruptive source RX J1301.9+2747

Lev Titarchuk, Elena Seifina, Vadim Arefiev +2

We present a spectral and timing analysis of X-ray emission from the actively accreting supermassive black hole (SMBH) in RX~J1301.9+2747 with prominent quasi-periodic eruptions (Q…

astro-ph.HE2026

Energy-independent X-Ray Polarization in 4U 1630-47 in the Intermediate State from Spectroscopy and Polarimetry

Elena Seifina, Lev Titarchuk, Paolo Soffitta +4

The IXPE mission enabled measurements of X-ray polarization in accreting binaries. The dependence of the X-ray polarization degree on the binary inclination and the optical depth o…

astro-ph.HE2025

Linear Polarization in a Black Hole, 4U~1957+115 and its X-ray Spectral Analysis

Lev Titarchuk, Elena Seifina, Paolo Soffiitta +1

We present a new spectro-polarimetric method for estimation of the inclination of X-ray binaries using the linear polarization (LP) value in black hole (BH) sources, based on the e…

astro-ph.HE2025★ 2 cited

X-ray linear polarization prediction in Black-Hole binaries and Active Galactic Nuclei and its measurements by IXPE

Lev Titarchuk, Paolo Soffitta, Elena Seifina +3

We present a theoretical framework for the formation of X-ray linear polarization in black hole (BH) source. The X-ray linear polarization originates from up-scatterings of initial…

astro-ph.GA2024

Changing Look AGN: An X-ray Look

Lev Titarchuk, Elena Seifina, Yegor Mishin

To date, a number of changing-look (CL) active galactic nuclei (AGNs) are known. We studied, in detail what happens to the X-ray spectrum during the CL events using the example of…

astro-ph.HE2024

SDSS~J075217.84+193542.2: X-ray weighing of a secondary BH

Lev Titarchuk, Elena Seifina

Precise measurements of black hole (BHs) masses are necessary to understand the coevolution of these sources and their host galaxies. Sometimes in the center of a galaxy there is n…