Brightness variations in comet P/Halley determined by the least scatter algorithm

Details Brightness variations in comet P/Halley determined by the least scatter algorithm Brightness variations in comet P/Halley determined by the least scatter algorithm

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985aexpr...1..133m&link_type=abstract

Astronomy Express (ISSN 0265-5365), vol. 1, June 1985, p. 133-136.

Astronomy and Astrophysics

Astronomy

5

Astronomical Photometry, Brightness Distribution, Comet Nuclei, Halley'S Comet, Algorithms, Eureca (Esa), Fourier Analysis

Scientific paper

The theoretical basis of the least-scatter-method period-finding algorithm EUREKA is explained, and the algorithm is applied to analyze the combined recent photometric observations of comet P/Halley (West and Pedersen, 1984; Le Fevre et al., 1984: Jewitt and Danielson, 1984). Periods of 0.684 d with scatter 0.24 mag and 2.005 d with scatter 0.22 mag are determined.

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