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Low resolution stellar spectrophotometric observations in the region 1500 Å–3000 Å

Published online by Cambridge University Press:  14 August 2015

G.C. Sudbury
G.C. Sudbury*
Affiliation:
Royal Observatory, Edinburgh, Great Britain

Extract

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The success of Stecher and Milligan (1962) in obtaining UV photoelectric objective dispersion spectra of stars in 1962 inspired similar work at the Royal Observatory, Edinburgh. For a number of reasons we preferred to build a system using grating dispersion in the convergent beam from a 21-cm diameter paraboloidal mirror (Sudbury, 1969). The same principle of random sky scan from a spinning rocket was employed.

Type
Part I: Stellar Fluxes
Information
Symposium - International Astronomical Union , Volume 36: Ultraviolet Stellar Spectra and Related Ground-Based Observations , 1970 , pp. 134
Copyright
Copyright © Reidel 1970 

References

Stecher, T. P. and Milligan, J. E.: 1962, Astrophys. J. 136, 1.Google Scholar
Sudbury, G. C.: 1969, Appl. Opt. 8, 2013.Google Scholar