Bulk photographic photometry of stars
A new method for bulk photographic photometry of stars is proposed. This method is based on the use of a new parameterΦi proposed by the authors, which depends linearly on mv over the entire range of magnitudes.
KeywordsEntire Range Photographic Photometry
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- 1.W. A. Hiltner (ed.),Methods of Astronomy [Russian translation], Mir, Moscow (1967), p. 536.Google Scholar
- 2.R. A. Vardanian, M. O. Zakarian, M. S. Mirtsoyan, and A. N. Tomov,Soobshch. Byurakan. Observ., No. 53, 14 (1980).Google Scholar
- 3.D. L. Fried,J. Opt. Soc. Amer.,56, No. 10, 1372 (1966).Google Scholar
- 4.M. Sh. Karapetian, M. A. Mnatsakanian, and R. A. Sarkisian,Astron. Tsirk., No. 1544, 35 (1990).Google Scholar