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Atmospheric extinction in B and V photometry at the South Pole

Published online by Cambridge University Press:  30 March 2016

Kwan-Yu Chen  and
Frank Bradshaw Wood
Kwan-Yu Chen
Affiliation:
University of Florida
Frank Bradshaw Wood
Affiliation:
University of Florida

Extract

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Scientific work at the South Pole during austral winter began in 1957, the International Geophysical Year. Interest in a polar observatory was already expressed in the survey of polar research conducted by the Committee of Polar Research (Gould, 1970). But not until 1986, was photoelectric photometry of variable stars made at the South Pole (Chen et al 1988); and in 1988, stellar observations for atmospheric extinction were made. The optical telescope used for stellar observations at the South Pole is a twin-mirror siderostat with an 8 cm lens (Chen et al 1986; Taylor 1988). The computer-controlled automated telescope made the polar observations possible.

Type
Joint Commission Meetings
Information
Highlights of Astronomy , Volume 9: Highlights of Astronomy. As presented at the XXIst General Assembly of the IAU, 1991 , 1992 , pp. 581
Copyright
Copyright © Kluwer 1992

References

Chen, K-Y., Esper, J., McNeill, J. D., Oliver, J. P., Schneider, G. and Wood, F.B., 1986. ‘Proceedings of the 118th Symposium of the International Astronomical Union’, eds. Hearnshaw, J. B and Cottrell, P. L. pp. 83–84.Google Scholar
Chen, K-Y., Oliver, J. P. and Wood, F. B. 1988. ‘Antarctic J. of the United States’, 1987 Review, Vol. XXII, No. 5, 283–284.Google Scholar
Gould, L. M. 1970. ‘Polar Research’ (National Academy of Sciences, Washington, D.C.), p.170.Google Scholar
Taylor, M. J. 1988. ‘Sky and Telescope’ 76 Google Scholar