SRG/ART-XC all-sky X-ray survey: Catalog of sources detected during the first year
astro-ph.HE
/ Authors
M. Pavlinsky, S. Sazonov, R. Burenin, E. Filippova, R. Krivonos, V. Arefiev, M. Buntov, C. -T. Chen, S. Ehlert, I. Lapshov
and 13 more authors
V. Levin, A. Lutovinov, A. Lyapin, I. Mereminskiy, S. Molkov, B. D. Ramsey, A. Semena, N. Semena, A. Shtykovsky, R. Sunyaev, A. Tkachenko, D. A. Swartz, A. Vikhlinin
/ Abstract
We present a first catalog of sources detected by the Mikhail Pavlinsky ART-XC telescope on board the SRG observatory in the 4-12 keV energy band during its ongoing all-sky survey. The catalog comprises 867 sources detected on the combined map of the first two 6-month scans of the sky (December 2019 - December 2020). The achieved sensitivity to point sources varies between ~4x10^-12 erg/s/cm2 near the ecliptic plane and ~8x10^-13 erg/s/cm2 (4-12 keV) near the ecliptic poles, and the typical localization accuracy is ~15 arcsec. Of the 750 sources of known or suspected origin in the catalog, 56% are extragalactic (mostly active galactic nuclei, AGN; and clusters of galaxies) and the rest are Galactic (mostly cataclysmic variables, CVs; and low- and high-mass X-ray binaries). For 114 sources, ART-XC has detected X-rays for the first time. Although the majority of these (~80) are expected to be spurious (given the adopted detection threshold), there can be a significant number of newly discovered astrophysical objects. We have started a program of optical follow-up observations of the new and previously unidentified X-ray sources, which has already led to the identification of several AGN and CVs. With the SRG all-sky survey planned to continue for a total of four years, we can expect the ART-XC survey in the 4-12 keV band to significantly surpass previous surveys that were carried out in similar (medium X-ray) energy bands in terms of the combination of angular resolution, sensitivity, and sky coverage.