NUK - logo
E-viri
Recenzirano Odprti dostop
  • SRG/ART-XC all-sky X-ray su...
    Pavlinsky, M.; Sazonov, S.; Burenin, R.; Filippova, E.; Krivonos, R.; Arefiev, V.; Buntov, M.; Chen, C.-T.; Ehlert, S.; Lapshov, I.; Levin, V.; Lutovinov, A.; Lyapin, A.; Mereminskiy, I.; Molkov, S.; Ramsey, B. D.; Semena, A.; Semena, N.; Shtykovsky, A.; Sunyaev, R.; Tkachenko, A.; Swartz, D. A.; Vikhlinin, A.

    Astronomy and astrophysics (Berlin), 05/2022, Letnik: 661
    Journal Article

    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), ART-XC sky surveys 1 and 2, or ARTSS12. The achieved sensitivity to point sources varies between ~4 x 10 -12 erg s -1 cm -2 near the ecliptic plane and ~8 x 10 -13 erg s -1 cm -2 (4–12keV) near the ecliptic poles, and the typical localization accuracy is ~15”. 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.