Volume 397, Number 1, January I 2003
|Page(s)||361 - 369|
|Published online||11 December 2002|
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China
2 Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
3 Department of Physics and Astronomy, Box 871504, Arizona State University, Tempe, AZ 85287-1504, USA
Corresponding author: Xu ZHOU, firstname.lastname@example.org
Accepted: 18 September 2002
In this paper, we present a set of photometric observations in 15 colors of stars in the Landolt SA95 field with the BATC system. The wavelengths covered by the system range from 300 nm to 1000 nm. 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 SEDs of 3613 stars.
Key words: methods: observational / techniques: photometric / stars: general
© ESO, 2003
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