15-color BATC photometry of Landolt SA95 field (Zhou+, 2003)

Details 15-color BATC photometry of Landolt SA95 field (Zhou+, 2003) 15-color BATC photometry of Landolt SA95 field (Zhou+, 2003)

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33970361z&link_type=abstract

VizieR On-line Data Catalog: J/A+A/397/361. Originally published in: 2003A&A...397..361Z

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Methodology

Clusters: Galaxy, Galaxies: Photometry, Photometry: Ccd

Scientific paper

In this paper, we present a set of photometric observations in 15 colors of stars in the Landolt SA95 field with the BATC (Beijing-Arizona-Taipei-Connecticut) system. The wavelengths covered by the system range from 300nm to 1000nm. Visual magnitudes of the stars studied in the field are from the 10th to 20th mag. The observational methodology and the data reduction procedures are described. The relationships between the BATC intermediate-band system and the Landolt UBVRI broad band system are obtained. A catalogue of the photometry has been produced which contains the spectral energy distributions (SEDs) of 3613 stars.
(3 data files).

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