Paper
30 September 2004 HAWK-I: A new wide-field 1- to 2.5-μm imager for the VLT
Jean-Francois Pirard, Markus Kissler-Patig, Alan Moorwood, Peter Biereichel, Bernard Delabre, Reinhold Dorn, Gert Finger, Domingo Gojak, Gotthard Huster, Yves Jung, Franz Koch, Miska Le Louarn, Jean-Louis Lizon, Leander Mehrgan, Eszter Pozna, Armin Silber, Barbara Sokar, Joerg Stegmeier
Author Affiliations +
Abstract
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.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jean-Francois Pirard, Markus Kissler-Patig, Alan Moorwood, Peter Biereichel, Bernard Delabre, Reinhold Dorn, Gert Finger, Domingo Gojak, Gotthard Huster, Yves Jung, Franz Koch, Miska Le Louarn, Jean-Louis Lizon, Leander Mehrgan, Eszter Pozna, Armin Silber, Barbara Sokar, and Joerg Stegmeier "HAWK-I: A new wide-field 1- to 2.5-μm imager for the VLT", Proc. SPIE 5492, Ground-based Instrumentation for Astronomy, (30 September 2004); https://doi.org/10.1117/12.578293
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Cited by 41 scholarly publications.
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KEYWORDS
Sensors

Mirrors

Cryogenics

Optical filters

Telescopes

Imaging systems

Near infrared

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