A photometric study of the BAO-CCD BVRI system

Details A photometric study of the BAO-CCD BVRI system A photometric study of the BAO-CCD BVRI system

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acaps..12...47j&link_type=abstract

(Acta Astrophysica Sinica, vol. 12, no. 1, 1992, p. 47-53) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 16, no. 2,

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Charge Coupled Devices, Schmidt Telescopes, Spectrophotometry, Goodness Of Fit, Interstellar Extinction, Reference Stars, Stellar Color

Scientific paper

The BAO Schmidt telescope with a Thomson CCD of 576 x 384 pixels was
utilized for BVRI photometry. Nine secondary photometric standard stars
in three CCD frames were observed on 31 October 1989, to establish the
color equations. Various problems relative to the capability of CCD
photometry are discussed.

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