Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..393m&link_type=abstract
(Astronomicheskii Zhurnal, vol. 62, Mar.-Apr. 1985, p. 393-403) Soviet Astronomy (ISSN 0038-5301), vol. 29, Mar.-Apr. 1985, p. 2
Astronomy and Astrophysics
Astronomy
15
Atmospheric Attenuation, Atmospheric Correction, Iteration, Stellar Spectrophotometry, Transmittance, Data Reduction, Spectral Energy Distribution, Transparence
Scientific paper
A method is proposed for determining the spectral transmission coefficient p(lambda) and allowing for atmospheric extinction in wide-band, multicolor stellar photometry. The method is based on the representation (modeling) of p(lambda) in the form of a function of a small number of parameters determined from the multicolor measurements themselves. It permits the elimination of systematic errors exceeding 0.005 m in the atmospheric reduction of wide-band and integral measurements. From prolonged WBVR observations (130 nights in the course of seven years) pronounced variations of selectivity in atmospheric transparency were found which are taken into account in the proposed method of reduction of measurement results.
Khaliullin Kh. F.
Moshkalev V. G.
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