1996年12月
LEWIS: A near-infrared cross-dispersed spectrograph
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
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- 巻
- 108
- 号
- 730
- 開始ページ
- 1129
- 終了ページ
- 1134
- 記述言語
- 英語
- 掲載種別
- 研究論文(学術雑誌)
- DOI
- 10.1086/133846
- 出版者・発行元
- UNIV CHICAGO PRESS
LEWIS (L, M-band Echelle Wide coverage Intermediate-resolution Spectrometer) is an infrared spectrograph designed primarily for spectroscopy in the 2.0-5.0 mu m) region. It is capable of covering the whole L band (2.8-4.2 mu m) or M band (4.5-5.0 mu m) in one exposure with a resolving power over 1250 by using both a prism and a grating to produce a cross-dispersed echelle-type spectrogram onto a Santa Barbara Research Center (SBRC) 256x256 InSb array. The grating is characterized by a large groove spacing of 125 mu m and is utilized at very high orders (25th-37th order in the L band). The achieved throughput of the spectrograph including the quantum efficiency of the detector is about 20%.
- リンク情報
- ID情報
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- DOI : 10.1086/133846
- ISSN : 0004-6280
- Web of Science ID : WOS:A1996VY12100012