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The Medium Dispersion Prism of the UK Schmidt Telescope

Published online by Cambridge University Press:  25 April 2016

R. D. Cannon ,
J. A. Dawe ,
D. H. Morgan ,
Ann Savage  and
M. G. Smith
R. D. Cannon
Affiliation:
The Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ
J. A. Dawe
Affiliation:
The Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ
D. H. Morgan
Affiliation:
The Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ
Ann Savage
Affiliation:
The Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ
M. G. Smith
Affiliation:
The Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ
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Extract

The U.K. 1.2 metre Schmidt Telescope acquired its first full aperture objective prism in 1975. This was a very low dispersion prism (2400 Å/mm at 4300 Å) which has been found to be particularly useful in searching for faint QSO’s.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 4 , 1982 , pp. 468 - 474
Copyright
Copyright © Astronomical Society of Australia 1982

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References

(1) Houk, N., and Cowley, A. P., Univ. Mich. Catalogue of Two-dimensional Spectral Types for the HD Stars, (1975).Google Scholar
(2) Westerlund, B. E., and Smith, L. F., Mon. Not. R. Astron. Soc., 127, 449 (1964).Google Scholar
(3) Boksenberg, A., Shortridge, K., Fosbury, R. A. E., Penston, M. V., and Savage, Ann, Mon. Not. R. Astron. Soc., 172, 289 (1975).Google Scholar
(4) Lynds, C. R., and Wills, D., Astrophys. J., 172, 531 (1972).Google Scholar
(5) Wills, D., and Lynds, C. R., Astrophys. J. Suppl. Ser., 36, 317 (1978).Google Scholar
(6) Lynds, C. R., and Wills, D., Nature, 226, 532 (1970).Google Scholar
(7) Wampler, E. J., Robinson, L. B., Baldwin, J. A., and Burbidge, E. M., Nature, 243, 336 (1973).Google Scholar
Cheney, Janet E., and Rowan-Robinson, M., Mon. Not. R. Astron. Soc., 195, 497 (1981).Google Scholar
Feast, M. W., Mon. Not. R. Astron. Soc., 140, 345 (1968).Google Scholar
Fehrenbach, Ch., Duflot, M. A., and Acker, A., Astron. Astrophys. Suppl. Ser., 33, 115 (1978).Google Scholar
MacAlpine, G. M., and Williams, G. A., Astrophys. J. Suppl. Ser., 45, 113 (1981).Google Scholar
Nandy, K., Reddish, V. C., Tritton, K. P., Cooke, J. A., and Emerson, D., Mon. Not. R. Astron. Soc., 178, 63 p. (1977).Google Scholar
Peterson, B. A., Wright, A. E., Jauncey, D. L., and Condon, J. J., Astrophys. J., 232, 400 (1979).Google Scholar
Savage, Ann, and Bolton, J. G., Mon. Not. R. Astron. Soc., 188, 599 (1979).Google Scholar