In August-September 2019, the ART-XC telescope scanned a large field (about 40 sq. deg) around the Galactic Center for nearly 3 weeks as part of the SRG Cal-PV phase. This resulted in a unique survey of the Galactic Bulge in the hard X-ray band of 4-30 keV. The main results of this survey will be presented, with a focus on the statistical properties of cataclysmic variables and low-luminosity X-ray binaries.
|Presenter status||ART-XC consortium member|