SRG/ART-XC all-sky X-ray survey: Catalog of sources detected during the first year

被引:20
|
作者
Pavlinsky, M. [1 ]
Sazonov, S. [1 ]
Burenin, R. [1 ]
Filippova, E. [1 ]
Krivonos, R. [1 ]
Arefiev, V [1 ]
Buntov, M. [1 ]
Chen, C-T [2 ]
Ehlert, S. [3 ]
Lapshov, I [1 ]
Levin, V [1 ]
Lutovinov, A. [1 ]
Lyapin, A. [1 ]
Mereminskiy, I [1 ]
Molkov, S. [1 ]
Ramsey, B. D. [3 ]
Semena, A. [1 ]
Semena, N. [1 ]
Shtykovsky, A. [1 ]
Sunyaev, R. [1 ]
Tkachenko, A. [1 ]
Swartz, D. A. [2 ]
Vikhlinin, A. [1 ,4 ]
机构
[1] Space Res Inst, 84-32 Profsouznaya Str, Moscow 117997, Russia
[2] Univ Space Res Assoc, Huntsville, AL 35805 USA
[3] NASA, Marshall Space Flight Ctr, Huntsville, AL 35812 USA
[4] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
基金
俄罗斯科学基金会;
关键词
surveys; catalogs; X-rays: general; NEWTON SLEW SURVEY; ART-XC; NUSTAR OBSERVATIONS; BLAZAR CANDIDATES; OPTICAL-IDENTIFICATION; CATACLYSMIC BINARIES; INTEGRAL SOURCES; SPECTRUM; RADIO; TELESCOPE;
D O I
10.1051/0004-6361/202141770
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 similar to 4 x 10(-12) erg s(-1) cm(-2) near the ecliptic plane and -8 x 10(-13) erg s(-1) cm(-2) (4-12 keV) near the ecliptic poles, and the typical localization accuracy is similar to 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 (similar to 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.
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页数:18
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