CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation
We propose to survey the complete Galactic sample of confirmed massive binaryBe+sdO stars. We aim to probe the models which predicts that a significantfraction of Be-type stars have hot companions w
CSC uses combined (i.e. overlapping) Chandra observations for detecting X-ray sources. This allows the catalog to include significantly fainter sources than CSC 1.1. The set of overlapping observation
