HIPPARCOS great-circle reduction - Theory, results and intercomparisons

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Accuracy, Data Reduction, Great Circles, Hipparcos Satellite, Satellite Observation, Satellite Orientation, Data Smoothing, Least Squares Method, Root-Mean-Square Errors

Scientific paper

In this paper some of the results of the great-circle reduction in the two data reduction consortia (NDAC and FAST) are presented. It is shown that the root-mean-square (rms) error of the great-circle abscissa of stars brighter than 10 mag is between 3-5 milli-arcsec. This is as was expected before launch, even in spite of the fact that the data-sets are shorter in the revised mission. There is a large positive correlation between the abscissa of stars separated by a multiple of the basic angle. Moreover, the great-circle results are affected by systematic errors at the beginning of the reductions. This is confirmed by intercomparisons between the two consortia. Finally, it is shown that the along-scan attitude of the Hipparcos satellite can be described with a few hundred parameters with milli-arcsec accuracy.

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