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Tunable etalons and other applications of multi-application low-voltage piezoelectric instrument control electronics (MALICE)
EMS have developed low voltage piezoelectric (LVPZT) tunable filters for the James Webb Space Telescope (JWST), and a wide field tunable Michelson for the Canadian Space Agency"s (CSA) Stratosphe...
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Optical design for a Fabry-Perot image interferometer for solar observations
We outline here a preliminary optical design study for a telecentric tunable Fabry-Perot etalon system. The first result of the optical optimization into a design, which delivers performance image qua...

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HAWK-I: A new wide-field 1- to 2.5-µm imager for the VLT

Proc. SPIE, Vol. 5492, 1763 (2004); doi:10.1117/12.578293

Online Publication Date: 5 October 2004

Conference Date: Monday 21 June 2004
Conference Location: Glasgow, Scotland, United Kingdom
Conference Title: Ground-based Instrumentation for Astronomy
Conference Chairs: Alan F. M. Moorwood, Masanori Iye
HAWK-I (High Acuity, Wide field K-band Imaging) is a 0.9 µm - 2.5 µm wide field near infrared imager designed to sample the best images delivered over a large field of 7.5 arcmin x 7.5 arcmin. HAWK-I is a cryogenic instrument to be installed on one of the Very Large Telescope Nasmyth foci. It employs a catadioptric design and the focal plane is equipped with a mosaic of four HAWAII 2 RG arrays. Two filter wheels allow to insert broad band and narrow band filters. The instrument is designed to remain compatible with an adaptive secondary system under study for the VLT.

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