2000NewA....5..223D


Query : 2000NewA....5..223D

2000NewA....5..223D - New Astronomy, 5, 223-233 (2000/July-0)

The MARTINI adaptive optics instrument.

DOEL A.P., DUNLOP C.N., BUSCHER D.F., MYERS R.M., SHARPLES R.M. and MAJOR J.V.

Abstract (from CDS):

The Multi-Aperture Real Time Image Normalisation Instrument (MARTINI) is an adaptive optics system designed to operate at one of the Nasmyth focal stations of the 4.2 m William Herschel Telescope. Correction of atmospherically distorted images is achieved by the action of a six element segmented mirror in a real-time servo loop controlled by the signal from a CCD based Shack-Hartmann wavefront sensor. A unique aspect of the MARTINI instrument is that, from its conception, it was designed to be capable of image sharpening at visible wavelengths. An outline of the mechanical and electronic arrangement of MARTINI is given, together with a description of its modes of operation, facilities and performance. Also described are some of the first scientific results obtained with the instrument.

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Journal keyword(s):

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 4523 GiC 12 33 47.9911135872 +15 10 06.049286292   15.1       ~ 178 0
2 IC 3583 GiG 12 36 43.558 +13 15 32.93   13.31       ~ 189 1
3 M 15 GlC 21 29 58.33 +12 10 01.2           ~ 3274 0

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