Analysis of lunar occultations of close binaries and radio sources by the regularization method

Details Analysis of lunar occultations of close binaries and radio sources by the regularization method Analysis of lunar occultations of close binaries and radio sources by the regularization method

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980azh....57..762b&link_type=abstract

(Astronomicheskii Zhurnal, vol. 57, July-Aug. 1980, p. 762-766.) Soviet Astronomy, vol. 24, July-Aug. 1980, p. 439-441. Transla

Computer Science

Numerical Analysis

Binary Stars, Light Curve, Lunar Occultation, Numerical Analysis, Radio Sources (Astronomy), Angular Distribution, Signal To Noise Ratios

Scientific paper

Tikhonov's regularization method can be applied to solve numerically the integral equation relating an observed occultation curve to the brightness distribution across the occulted source. The method can allow for instrumental effects, is stable against stochastic noise, and should be valuable for analyzing lunar occultations of both optical and radio objects with complex angular structure. As an illustration, a photoelectric occultation curve of the close binary star 16 Tau is analyzed.

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