A Wide-Field Infrared Camera for the palomar 200-inch telescope

被引:154
作者
Wilson, JC [1 ]
Eikenberry, SS [1 ]
Henderson, CP [1 ]
Hayward, TL [1 ]
Carson, JC [1 ]
Pirger, B [1 ]
Barry, DJ [1 ]
Brandl, B [1 ]
Houck, JR [1 ]
Fitzgerald, GJ [1 ]
Stolberg, TM [1 ]
机构
[1] Cornell Univ, Ithaca, NY USA
来源
INSTRUMENT DESIGN AND PERFORMANCE FOR OPTICAL/INFRARED GROUND-BASED TELESCOPES, PTS 1-3 | 2003年 / 4841卷
关键词
wide-field; near-infrared;
D O I
10.1117/12.460336
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The availability of both large aperture telescopes and large format near-infrared.(NIR) detectors are making wide-field NIR imaging a reality. We describe the Wide-field Infrared Camera (WIRC), a newly commissioned instrument that provides the Palomar 200-inch telescope with such an imaging capability. WIAC features a field-of-view (FOV) of 4.33 arcminutes on a side with its currently installed 1024-square Rockwell Hawaii-I NIR detector. A 2048-square Rockwell Hawaii-II NIR detector will be installed and commissioned later this year, in collaboration with Caltech, to give WIRC an 8.7 arcminute FOV on a side. WIRC mounts at the telescope's f/3.3 prime focus. The instrument's seeing-limited optical design, optimized for the JHK atmospheric bands, includes a 4-element refractive collimator, two 7-position filter wheels that straddle a Lyot stop, and a 5-element refractive f/3 camera. Typical seeing-limited point spread functions are slightly oversampled with a 0.25 arcsec per pixel plate scale at the detector. The entire optical train is contained within a cryogenic dewar with a 2.5 day hold-time. Entrance hatches at the top of the dewar allow access to the detector without disruption of the optics and optical alignment. The optical, mechanical, cryogenic, and electronic design of the instrument are described, a commissioning science image and performance analyses are presented.
引用
收藏
页码:451 / 458
页数:8
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