The Palomar Testbed Interferometer

被引:261
作者
Colavita, MM
Wallace, JK
Hines, BE
Gursel, Y
Malbet, F
Palmer, DL
Pan, XP
Shao, M
Yu, JW
Boden, AF
Dumont, PJ
Gubler, J
Koresko, CD
Kulkarni, SR
Lane, BF
Mobley, DW
van Belle, GT
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Univ Calif San Diego, San Diego, CA 92103 USA
关键词
atmospheric effects; instrumentation : detectors; instrumentation : interferometers; techniques : interferometric;
D O I
10.1086/306579
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Palomar Testbed Interferometer (PTI) is a long-baseline infrared interferometer located at Palomar Observatory, California. It was built as a testbed for interferometric techniques applicable to the Keck Interferometer. First fringes were obtained in 1995 July. PTI implements a dual-star architecture, tracking two stars simultaneously for phase referencing and narrow-angle astrometry. The three fixed 40 cm apertures can be combined pairwise to provide baselines to 110 m. The interferometer actively tracks the white-light fringe using an array detector at 2.2 mu m and active delay lines with a range of +/-38 m. Laser metrology of the delay lines allows for servo control, and laser metrology of the complete optical path enables narrow-angle astrometric measurements. The instrument is highly automated, using a multiprocessing computer system for instrument control and sequencing.
引用
收藏
页码:505 / 521
页数:17
相关论文
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