M48 (NGC 2548) BATC photometry and membership (Wu+, 2006)

Details M48 (NGC 2548) BATC photometry and membership (Wu+, 2006) M48 (NGC 2548) BATC photometry and membership (Wu+, 2006)

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..71181104w&link_type=abstract

VizieR On-line Data Catalog: J/PASP/118/1104. Originally published in: 2006PASP..118.1104W

Computer Science

Scientific paper

Beijing-Arizona-Taiwan-Connecticut (BATC) multiband photometric data in the field of open cluster M48 are used to determine its membership. By comparing observed spectral energy distributions of M48 stars with theoretical ones, membership probabilities of 750 stars with limiting magnitudes of 15.0 in the BATC c band ({lambda}eff=4194{AA}) are determined. We find 323 stars with membership probabilities higher than 30% that are considered to be candidate members of M48. Comparing membership probabilities of 229 stars obtained in common between the present method and proper-motion-based methods, an 80% agreement among these methods is obtained
(3 data files).

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