HAWK-I:: a new 'Wide field' 1-2.5 μm imager for the VLT

被引：82

作者：

Pirard, JF ^{[1
]}

Kissler-Patig, M ^{[1
]}

Moorwood, A ^{[1
]}

Biereichel, P ^{[1
]}

Delabre, B ^{[1
]}

Dorn, R ^{[1
]}

Finger, G ^{[1
]}

Gojak, D ^{[1
]}

Huster, G ^{[1
]}

Jung, Y ^{[1
]}

Koch, F ^{[1
]}

Le Louarn, M ^{[1
]}

Lizon, JL ^{[1
]}

Mehrgan, L ^{[1
]}

Pozna, E ^{[1
]}

Silber, A ^{[1
]}

Sokar, B ^{[1
]}

Stegmeier, J ^{[1
]}

机构：

[1] ESO, D-85748 Garching, Germany

来源：

GROUND-BASED INSTRUMENTATION FOR ASTRONOMY, PTS 1-3 | 2004年 / 5492卷

关键词：

infrared; imaging; ground-based; astronomy;

D O I：

10.1117/12.578293

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

HAWK-1 (High Acuity, Wide field K-band Imaging) is a 0.9 mum - 2.5 mum 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.

引用

页码：1763 / 1772

页数：10

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