The equal-altitude method of quasi-absolute determination of star coordinates

Details The equal-altitude method of quasi-absolute determination of star coordinates The equal-altitude method of quasi-absolute determination of star coordinates

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pbeio..11...21l&link_type=abstract

Beijing Astronomical Observatory, Publications, Sept. 1988, p. 21-32.

Statistics

Computation

Astrolabes, Astronomical Catalogs, Astronomical Coordinates, Stars, Altitude, Computational Astrophysics, Error Analysis

Scientific paper

Absolute coordinate values are determined for 86 objects on the basis of data obtained with Mark II photoelectric astrolabe No. 2 at Beijing Astronomical Observatory during the period 1979-1984. The equal-altitude method employed in the computations is described in detail, and the results are presented in tables. The mean accuracy of the position corrections is given as + or - 1.6 msec in right ascension and + or - 0.019 arcsec in declination.

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