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Tanaka, Satoru; Kodaira, Keiichi; Tsuji, Takashi
Symposium on the cosmic observations for the fiscal year 19771977
Symposium on the cosmic observations for the fiscal year 19771977
AbstractAbstract
[en] The photometric data of infrared four colors (1 - 2.5μ) obtained with a 15 cm balloon telescope BAT-1, flown on May 29, 1976, were analyzed. On the basis of an αBoo model, the atmospheric physical parameters of five red giant stars, αSco, αHer, delta Vir, delta Oph and σ Lib were determined. These results are described. Since atmospheric absorption was negligible in the sky, sensitivity variation of the photometer was derived by repeated observation of bright stars, α Boo, α Sco and α Her, and those corrected for it were used as basic data. (Mori, K.)
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Tokyo Univ. (Japan). Inst. of Space and Aeronautical Science; p. 425-430; 1977; p. 425-430; Tokyo Univ. Inst. of Space and Aeronautical Science; Tokyo, Japan; Symposium on the cosmic observations; Tokyo, Japan; 22 - 24 Jun 1977
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Book
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Conference
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