NAOMI: adaptive optics at the WHT

Chris R. Benn; Maarten Blanken; Craige Bevil; Sebastian Els; Stephen Goodsell; Tom Gregory; Paul Jolley; Andy J. Longmore; Olivier Martin; Richard M. Myers; Roy Ostensen; Simon Rees; Rene G. M. Rutten; Ilona Soechting; Gordon Talbot; Simon M. Tulloch

doi:10.1117/12.552216

25 October 2004 NAOMI: adaptive optics at the WHT

Chris R. Benn, Maarten Blanken, Craige Bevil, Sebastian Els, Stephen Goodsell, Tom Gregory, Paul Jolley, Andy J. Longmore, Olivier Martin, Richard M. Myers, Roy Ostensen, Simon Rees, Rene G. M. Rutten, Ilona Soechting, Gordon Talbot, Simon M. Tulloch

Author Affiliations +

Proceedings Volume 5490, Advancements in Adaptive Optics; (2004) https://doi.org/10.1117/12.552216
Event: SPIE Astronomical Telescopes + Instrumentation, 2004, Glasgow, United Kingdom

Abstract

NAOMI is the AO system of the 4.2-m William Herschel Telescope on La Palma. It delivers near-diffraction-limited images in the IR, and a significantly improved PSF at optical wavelengths. The science cameras currently comprise an IR imager (INGRID), an optical integral-field spectrograph (OASIS) and a coronagraph which may be placed in the light path to either instrument. 19 science programmes were observed during 2002-3. Observing overheads are small, with as much as 60% of the night spent integrating on science targets. In late 2004 this year, the WFS will be equipped with a low-noise L3 CCD, giving a gain of a factor of 2 in S:N for faint guide stars. A Rayleigh laser guide star is under development, with first light expected summer 2006, providing a unique facility: AO-corrected optical integral-field spectroscopy anywhere on the northern sky.

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Chris R. Benn, Maarten Blanken, Craige Bevil, Sebastian Els, Stephen Goodsell, Tom Gregory, Paul Jolley, Andy J. Longmore, Olivier Martin, Richard M. Myers, Roy Ostensen, Simon Rees, Rene G. M. Rutten, Ilona Soechting, Gordon Talbot, and Simon M. Tulloch "NAOMI: adaptive optics at the WHT", Proc. SPIE 5490, Advancements in Adaptive Optics, (25 October 2004); https://doi.org/10.1117/12.552216

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