Performance of the FLAMINGOS near-IR multi-object spectrometer and imager and plans for FLAMINGOS-2: a fully cryogenic near-IR MOS for Gemini South

被引:34
作者
Elston, R [1 ]
Raines, SN [1 ]
Hanna, K [1 ]
Hon, D [1 ]
Julian, J [1 ]
Horrobin, M [1 ]
Harmer, C [1 ]
Epps, H [1 ]
机构
[1] Univ Florida, Dept Astron, Gainesville, FL 32608 USA
来源
INSTRUMENT DESIGN AND PERFORMANCE FOR OPTICAL/INFRARED GROUND-BASED TELESCOPES, PTS 1-3 | 2003年 / 4841卷
关键词
near-infrared; spectrograph; multi-object; imager; HAWAII-2; array; FLAMINGOS; FLAMING-2; Gemini telescope; MMT telescope; astronomy;
D O I
10.1117/12.459937
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We report on the performance of FLANUNGOS, the world's-first fully cryogenic near-IR multi-object spectrometer. FLANIINGOS has a fast all refractive optical system, which can be used at telescopes slower than f/7.5. This makes FLANHNGOS a very efficient wide-field imager when used on fast small aperture telescopes and a high AOmega spectrometer using laser machined aperture masks for MOS spectroscopy. FLANHNGOS uses a 2048x2048 HgCdTe HAWAII-2 array by the Rockwell Science Center. The array is read out through 32 amplifiers, which results in low overheads for observations. We describe both the operating characteristics of the HAWAII-2 array and of the array controller and data acquisition system. FLAMINGOS has been in operation for about 1.5 years and is now in routine use on four telescopes: The Kitt Peak 4-m and 2.1-m, the 6.5-m MMT and the 8-m Gemini South Telescope. We will describe the operating characteristics of FLAMINGOS on each of these telescopes that deliver fields-of-view from 21x21 arcminutes to 2.7x2.7 arcminutes and pixels from 0.6 arcseconds to 0.08 areseconds. While providing a large AOmega product for fast telescopes (i.e. f/8), FLAMINGOS becomes progressively less efficient on slower telescopes. Since nearly all large telescopes have fairly slow optical systems (f/12 or slower) the combination of large aperture and slow optical systems makes FLAMINGOS ill suited for optimal performance on cur-rent large aperture telescopes. Thus, we are beginning construction of FLAMINGOS-2, which will be optimized for performance on the f/16 Gemini South 8-m telescope. Similar to FLAMINGOS, FLAMINGOS-2 will be fully refractive using grisms, laser machined aperture masks and a 2048x2048 HgCdTe HAWAII-2 array. FLAMINGOS-2 will provide a 6.1 arcminute field-of-view with 0.18 arcsecond pixels. FLAMINGOS-2 will also be designed to accept an f/32 beam from the Gemini South MCAO system.
引用
收藏
页码:1611 / 1624
页数:14
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