Description
We observed the young cluster NGC 2362 in X-rays with Chandra ACIS-I, and detected 387 point X-ray sources, most of which are shown to be cluster members. We report here the list of all detected X-ray sources and their basic X-ray properties, and report separately their identifications with optical stars, using data from Moitinho et al. (2001ApJ...563L..73M; UBVRI photometry) and Dahm (2005, Cat. <J/AJ/130/1805>; H{alpha} data). We include in the second table a classification of optically-identified X-ray sources, based on position in the HR diagram, which helps to separate rather clearly cluster members from field objects.
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