Proceedings Paper
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Paper Abstract
This paper presents some results of work carried out with the Cambridge, England, CCD System that demonstrate its abilities to work at the faintest levels yet achieved at a telescope. Future applications of this method are also discussed in relation to Next Generation Telescopes and larger CCDs. Recent results of our programme to extend our wavelength coverage into the near IR (1 - 5 microns) are also described.
Paper Details
Date Published: 9 January 1984
PDF: 3 pages
Proc. SPIE 0445, Instrumentation in Astronomy V, (9 January 1984); doi: 10.1117/12.966139
Published in SPIE Proceedings Vol. 0445:
Instrumentation in Astronomy V
Alec Boksenberg; David L. Crawford, Editor(s)
PDF: 3 pages
Proc. SPIE 0445, Instrumentation in Astronomy V, (9 January 1984); doi: 10.1117/12.966139
Show Author Affiliations
Craig D. Mackay, Institute of Astronomy (England)
Douglas M Astill, Institute of Astronomy (England)
Published in SPIE Proceedings Vol. 0445:
Instrumentation in Astronomy V
Alec Boksenberg; David L. Crawford, Editor(s)
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