30 Doradus OB Associations (Parker 1992)

Details 30 Doradus OB Associations (Parker 1992) 30 Doradus OB Associations (Parker 1992)

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat.2187....0p&link_type=abstract

VizieR On-line Data Catalog: II/187A. Originally published in: 1992PASP..104.1107P; 1993AJ....106..560P; 1993AJ....106.1471P

Physics

Magellanic Clouds, Clusters: Open, Photometry: Ubv

Scientific paper

These data have been reduced from 39 CCD frames (with short, medium, and long exposure times ranging from 3 to 1000 seconds) using the photometry program DAOPHOT (Peter Stetson, 1987PASP...99..191S). The photometric errors listed in these tables are the errors derived by DAOPHOT using the relative magnitude of the star on the CCD and the goodness of the fit of the point spread function. Most stars appear on more than one CCD frame per filter, and their resulting tabulated magnitudes are the averages of the individual measurements inversely weighted by the squares of their errors.
The stars in these tables are from two regions: the central region and a non-overlapping northern region. The latter are designated by four digit numbers starting with 9. The X,Y coordinates are the positions relative to the northwestern-most corner of each region.
(3 data files).

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