Chandra ACIS survey of M33 (ChaSeM33) (Plucinsky+, 2008)

Computer Science

Scientific paper

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Cross Identifications, Supernova Remnants, X-Ray Sources

Scientific paper

Our program was designed to comprise two long (~100ks each) uninterrupted observations of seven overlapping ACIS-I fields, separated by 6 months or more. ChASeM33 observations began in 2005 September; in this paper we present the observations performed in the first year of observations (i.e., through 2006 August).
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