XMM observations of {eta} Cha cluster (Lopez-Santiago+, 2011)

Details XMM observations of {eta} Cha cluster (Lopez-Santiago+, 2011) XMM observations of {eta} Cha cluster (Lopez-Santiago+, 2011)

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35249097l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/524/A97. Originally published in: 2011A&A...524A..97L

Computer Science

Clusters: Open, X-Ray Sources

Scientific paper

We used proprietary data from a deep XMM-Newton EPIC observation targeting the core of the {eta} Chamaleontis cluster. Specific software for the reduction of XMM-Newton data was used to analyze our observation. To detect sources in the composed EPIC pn+mos image, we used the wavelet-based code PWDetect. General coronal properties were derived from plasma model fitting. X-ray light curves in the 0.3-8.0keV energy range were generated for each star.
(1 data file).

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