Adaptive optics at the WHT

The WHT is unusually well-placed for exploitation of adaptive-optics (AO) t echnology. The site seeing is excellent (median 0.7 arcsec), dome seeing is negligible, and preliminary studies indicate that most of the atmospheric seeing originates in a well-defined layer at low altitude, which bodes well for future laser-guide-star AO. The Durham group have built up extensive e xperience with natural-guide-star adaptive-optics experiments at the GHRIL Nasmyth focus, and the NAOMI common-user AO facility is due to be commissio ned at this focus early in 2000. NAOMI will provide near-diffraction-limite d imaging in the IR (Strehl similar to0.6, FWHM similar to0.15 arcsec in K) and is expected to give significant correction in the optical (poorer Stre hl, but similar FWHM). NAOMI will perform better at short wavelengths than AO systems on other telescopes, and observers will require instrumentation that can exploit this crucial advantage. (C) 2001 Elsevier Science B.V. All rights reserved.