Statistics – Computation
Scientific paper
Nov 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...334..465e&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 334, Nov. 1, 1988, p. 465-469.
Statistics
Computation
20
Astrometry, Computational Astrophysics, Stellar Motions, Stellar Parallax, Mathematical Models, Matrices (Mathematics)
Scientific paper
The matrix of the normal equations of a central overlapping-plate solution with general models for frame parameters and the star parameters (providing, e.g., for an estimate of the parallax of each star) is inverted explicitly in terms of the inverses of the matrices in the isolated systems for the frame parameters and the star parameters. This allows one, without actually inverting the matrix of the system numerically, to calculate from explicit formulae those numerical estimates of the star parameters and the frame parameters which would follow from a rigorous overlapping-plate solution as well as to calculate rigorously the covariance matrix of the adjustment parameters.
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