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First Results of the Absolute Calibration of the u, v, b, y System of Filters

Published online by Cambridge University Press:  07 February 2017

S. Tapia ,
H. L. Johnson  and
D. L. Crawford
S. Tapia
Affiliation:
Steward Observatory, University of Arizona, Tucson, Ariz., U.S.A.
H. L. Johnson
Affiliation:
Steward Observatory, University of Arizona, Tucson, Ariz., U.S.A.
D. L. Crawford
Affiliation:
Kitt Peak National Observatory*, Tucson, Ariz., U.S.A.

Abstract

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Absolute flux densities for a zero magnitude A0V star at the effective wavelengths of the u, v, b, y spectral bands are presented.

Type
Part V: Ground Based and Extraterrestrial Observations of Stellar Flux
Information
Symposium - International Astronomical Union , Volume 54: Problems of Calibration of Absolute Magnitudes and Temperature of Stars , 1973 , pp. 163 - 164
Copyright
Copyright © Reidel 1973 

References

Code, A. D.: 1960, Stars and Stellar Systems 6, 85.Google Scholar
Johnson, H. L.: 1965, Commun. Lunar Planet. Lab. 3, No. 53, 73.Google Scholar
Kharitonov, A.: 1963, Soviet Astron. 7, 258.Google Scholar
King, I.: 1952, Astron. J. 57, 253.Google Scholar
Mitchell, R. I. and Johnson, H. L.: 1969, Commun. Lunar Planetary Lab. 8, No. 132, 1.Google Scholar
Oke, J. B. and Schild, R. E.: 1970, Astrophys. J. 161, 1022.Google Scholar
Willstrop, R. V.: 1965, Mem. Roy. Astron. Soc. 69, 83.Google Scholar