Active compensation of flexure on the WHT ISIS spectrograph

P. D'Arrigo, F. Diego, D. D. Walker

Research output: Contribution to journalArticle

4 Citations (Scopus)

Abstract

ISIS Spectrograph Automatic Active Collimator (ISAAC) was developed at the Optical Science Lab, University College London, as an experimental system to improve the image stability on the detectors of the Intermediate-dispersion Spectroscopic and Imaging System (ISIS) at the William Herschel Telescope (WHT). It is based on the concept of active compensation, where spectrum drifts, owing to the spectrograph flexing under the effect of gravity, are compensated by the movement of an active optical element. ISAAC is a fine-steering tip-tilt collimator mirror; it was tested on the spectrograph in 1995 July. Here we report the details of the design and the laboratory tests together with the results of the experiment on ISIS at the WHT. The experiment shows that active compensation can reduce flexure down to less than 3 μm over 4 h of telescope motions, dramatically improving the spectrograph performance. A way of implementing ISAAC as a common user facility is briefly discussed, together with a study of the characteristics of flexure in ISIS.

LanguageEnglish
Pages679-686
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume281
Issue number2
DOIs
Publication statusPublished - 11 Jul 1996
Externally publishedYes

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flexing
flexure
spectrographs
telescopes
collimators
tilt
experiment
gravity
mirrors
gravitation
detectors

Cite this

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abstract = "ISIS Spectrograph Automatic Active Collimator (ISAAC) was developed at the Optical Science Lab, University College London, as an experimental system to improve the image stability on the detectors of the Intermediate-dispersion Spectroscopic and Imaging System (ISIS) at the William Herschel Telescope (WHT). It is based on the concept of active compensation, where spectrum drifts, owing to the spectrograph flexing under the effect of gravity, are compensated by the movement of an active optical element. ISAAC is a fine-steering tip-tilt collimator mirror; it was tested on the spectrograph in 1995 July. Here we report the details of the design and the laboratory tests together with the results of the experiment on ISIS at the WHT. The experiment shows that active compensation can reduce flexure down to less than 3 μm over 4 h of telescope motions, dramatically improving the spectrograph performance. A way of implementing ISAAC as a common user facility is briefly discussed, together with a study of the characteristics of flexure in ISIS.",
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Active compensation of flexure on the WHT ISIS spectrograph. / D'Arrigo, P.; Diego, F.; Walker, D. D.

In: Monthly Notices of the Royal Astronomical Society, Vol. 281, No. 2, 11.07.1996, p. 679-686.

Research output: Contribution to journalArticle

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AU - Diego, F.

AU - Walker, D. D.

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