Optimal star selection for observational programs using the equal altitude method

Details Optimal star selection for observational programs using the equal altitude method Optimal star selection for observational programs using the equal altitude method

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...28k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Sept.-Oct. 1989, p. 28-31. In Russian.

Statistics

Computation

Computational Astrophysics, Star Distribution, Stellar Models, Stellar Systems, Altitude, Optimization, Stellar Structure, Three Dimensional Models

Scientific paper

The optimum geometrical and temporal structure of groups of stars for observation by the equal altitude method is estimated using the D-optimality criterion. It is found that compound two-hour groups of four stars, which are observed in two reciprocal perpendicular verticals, are optimal for determining longitude and latitude and for gaining information on the stability of almucantar parameters during group observations.

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