BAO-CCD BVRI photometry.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The BAO Schmidt telescope with a Thomson CCD of 576×384 pixels was
used for BVRI photometry. 9 secondary standard stars in 3 CCD frames
were observed on October 31, 1989. The colour equations are presented
for this photometric system. Some problems relevant to the capability of
CCD photometry are discussed.

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