Search Publications

SRGz: Building an Optical Cross-Match Model for the X-ray SRG/eROSITA Sources Using the Lockman Hole Data
DOI: 10.1134/S1063773722020013 Bibcode: 2022AstL...48..109B

Gilfanov, M. R.; Medvedev, P. S.; Meshcheryakov, A. V. +1 more

We present a probabilistic model built for the optical cross-match between the SRG/eROSITA X-ray sources and photometric data from the DESI Legacy Imaging Surveys. The model relies both on positional and photometric information on optical objects nearby X-ray sources and allows performing selection with precision and recall ${≈}94%$ (for $F_{\text…

2022 Astronomy Letters
XMM-Newton 6
Optical Cross-Match of SRG/eROSITA X-ray Sources Using the Deep Lockman Hole Survey as an Example
DOI: 10.1134/S1063773722110044 Bibcode: 2022AstL...48..653B

Gilfanov, M. R.; Belvedersky, M. I.; Bykov, S. D.

We present a method for the optical cross-match of sources detected in wide-field X-ray sky surveys. For this purpose, we have constructed and trained a neural network model to characterize the photometric attributes of the populations of optical counterparts of X-ray sources and optical field objects. The photometric information processing result…

2022 Astronomy Letters
XMM-Newton 3
Study of the X-ray Pulsar IGR J21343+4738 Based on NuSTAR, Swift, and SRG Data
DOI: 10.1134/S106377372211007X Bibcode: 2022AstL...48..798G

Lutovinov, A. A.; Molkov, S. V.; Semena, A. N. +1 more

We present the results of our study of the X-ray pulsar IGR J21343+4738 based on NuSTAR, Swift, and SRG observations in the wide energy range 0.3-79 keV. The absence of absorption features in the energy spectra of the source, both averaged and phase-resolved ones, has allowed us to estimate the upper and lower limits on the magnetic field of the n…

2022 Astronomy Letters
XMM-Newton 2