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Proceedings Paper

The Faint Object Spectrograph For The 2.5M Isaac Newton Telescope
Author(s): J. M. Breare; R. S. Ellis; J. R. Powell
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Paper Abstract

The faint object spectrograph (FOS) is a highly efficient, fixed format spectrograph using a CCD detector and aimed at low resolution (15-20Å fwhm) spectrophotometry over the range 4000 to 10500K. The overall efficiency including atmosphere and telescope absorption is 12% at 7000K and a zenith distance of 27.5. It has a fixed spectrum format and is provided with an extensive set of on-line data reduction and analysis operations.

Paper Details

Date Published: 13 October 1986
PDF: 5 pages
Proc. SPIE 0627, Instrumentation in Astronomy VI, (13 October 1986); doi: 10.1117/12.968100
Show Author Affiliations
J. M. Breare, Durham University (United Kingdom)
R. S. Ellis, Durham University (United Kingdom)
J. R. Powell, Herstmonceux Castle (United Kingdom)

Published in SPIE Proceedings Vol. 0627:
Instrumentation in Astronomy VI
David L. Crawford, Editor(s)

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