CCD photometry in the Vilnius system in the vicinity of the globular cluster M 56

Details CCD photometry in the Vilnius system in the vicinity of the globular cluster M 56 CCD photometry in the Vilnius system in the vicinity of the globular cluster M 56

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...388..149s&link_type=abstract

Astronomy and Astrophysics, v.388, p.149-157 (2002)

Astronomy and Astrophysics

Astrophysics

1

Stars: Fundamental Parameters, Stars: General, Galaxy: Globular Clusters: Individual: M 56

Scientific paper

CCD observations of field stars in an area north-east of the globular cluster M 56 were obtained in six bands of the Vilnius photometric system. The data sets cover a field of 9.9 m x 9.5 m. An outline of the data pathway from observations to reduction via IRAF is outlined in this text. Photometry of 366 stars brighter than 18th V magnitude has been obtained and the analysis of the observational errors is discussed.

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