A photometric study of the BAO-CCD BVRI system.

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 photometric standard stars in 3
CCD frames were observed on Oct. 31, 1989, to establish the color
equations. Some problems relevant to the capability of CCD photometry
are discussed.

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