Finite-parametric models in inverse problems of astrophysics Lunar occultations of stars

Details Finite-parametric models in inverse problems of astrophysics Lunar occultations of stars Finite-parametric models in inverse problems of astrophysics Lunar occultations of stars

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63.1204g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 63, Nov.-Dec. 1986, p. 1204-1214. In Russian.

Mathematics

2

Astronomical Photometry, Diameters, Lunar Occultation, Stellar Magnitude, Stellar Physics, Functions (Mathematics), Integral Equations, Light Curve, Lunar Limb, Stellar Models

Scientific paper

An efficient method for a determination of the angular diameters of
stars from the lunar occultation light curves, as well as the confidence
intervals characterizing the statistical errors of the parameters, is
described.

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