SRG/ART-XC Galactic Bulge deep survey. II. Catalogue of point sources

Author:

Semena A1ORCID,Mereminskiy I1ORCID,Lutovinov A1,Sazonov S1,Arefiev V1,Borisov K2,Burenin R1,Buntov M1,Garanin S3,Garin M3,Grigorovich S3,Karasev D1,Krivonos R1ORCID,Levin V1,Lapshov I1,Molkov S1,Pavlinsky M1,Shtykovsky A1,Semena N1,Sunyaev R1,Tkachenko A1,Vikhlinin A14,Voron V2

Affiliation:

1. Space Research Institute of RAS , 84/32 Profsoyuznaya str, Moscow 117997 , Russia

2. State Space Corporation Roscosmos , 42 Schepkina str, Moscow 107996 , Russia

3. VNIIIEF , Nizhny Novgorod region 607188 , Russia

4. Harvard-Smithsonian Center for Astrophysics , 60 Garden Street, Cambridge, MA 02138 , USA

Abstract

ABSTRACT We present a catalogue of point sources detected with the Mikhail Pavlinsky ART-XC telescope onboard the SRG observatory during a wide-field survey of the Galactic Bulge that was conducted as part of the mission’s calibration and performance verification phase in 2019. The survey consisted of nearly 18 d of consecutive scanning observations of the sky region |l| < 6 deg, |b| < 2.5 deg with the median sensitivity of 4 × 10−13 erg s−1 cm−2 in the 4–12 keV energy band, which allows the detection of sources down to a luminosity of 3 × 1033 erg s−1 near the Galactic Centre. Using a maximum-likelihood-based algorithm, 172 sources were detected. Of these, 153 are registered on the average 4–12 keV map and 18 sources are either extremely hard (detected only at energies above 7 keV) or highly variable (detected only in individual scans shorter than a day). For 121 sources, there are plausible counterparts in other X-ray source catalogues, including 43 with known classification. The remaining 51 sources are previously unknown objects, discovered by ART-XC during the Galactic Bulge survey.

Funder

Russian Academy of Sciences

NASA

ADS

CDS

Publisher

Oxford University Press (OUP)

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