Astronomy with a visible-band imaging fourier transform spectrometer

被引：0
|
作者：
Wurtz, R [1 ]
Wishnow, E [1 ]
Blais-Ouellette, S [1 ]
Cook, K [1 ]
Carr, D [1 ]
Lewis, I [1 ]
Grandmont, F [1 ]
Stubbs, C [1 ]
机构：
[1] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA
来源：
NEXT GENERATION WIDE-FIELD MULTI-OBJECT SPECTROSCOPY | 2002年 / 280卷
关键词：
D O I：
暂无
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Imaging through a Fourier transform spectrograph produces a high-throughput spectrum for every pixel in a field of typical CCD imaging sizes, a few arcminutes. We describe the design of the Livermore Imaging Fourier Transform Spectrograph for visible-band astronomy. We present astronomical observations with this instrument at the 3.5-meter Apache Point Observatory.
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页码：139 / 143
页数：5
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