SRG/ART-XC all-sky X-ray survey: Catalog of sources detected during the first year
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), 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.
Table B.1 is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/661/A38- Publication:
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Astronomy and Astrophysics
- Pub Date:
- May 2022
- DOI:
- 10.1051/0004-6361/202141770
- arXiv:
- arXiv:2107.05879
- Bibcode:
- 2022A&A...661A..38P
- Keywords:
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- surveys;
- catalogs;
- X-rays: general;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- To appear on A&