Results of photometric (B,V,R) measurements on the meridian axial circle.

Details Results of photometric (B,V,R) measurements on the meridian axial circle. Results of photometric (B,V,R) measurements on the meridian axial circle.

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kfnt...13f..14l&link_type=abstract

Kinematika Fiz. Nebesn. Tel, Tom 13, No. 6, p. 14 - 17

Astronomy and Astrophysics

Astronomy

Stars: Astrometry, Stars: Photometry

Scientific paper

Since March 1996, coordinate measurements on the meridian axial circle are accompanied by determinations of star brightness in B, V, R bands. To find preliminary estimate of the photometry accuracy, the authors have processed about 800 observations of FK5 stars. Comparison with the photometric reference catalogue has shown that the root-mean-square errors of one measurement are: σV = 0.09m, σB-V = 0.14m, σV-R = 0.05m. The internal uncertainty is: σV = 0.08m, σB-V = 0.09m, σV-R = 0.05m.

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