AN IMAGING FABRY–PÉROT SYSTEM FOR THE ROBERT STOBIE SPECTROGRAPH ON THE SOUTHERN AFRICAN LARGE TELESCOPE
AN IMAGING FABRY–PÉROT SYSTEM FOR THE ROBERT STOBIE SPECTROGRAPH ON THE SOUTHERN AFRICAN LARGE TELESCOPE
复制标题
南非大型望远镜罗伯特·斯托比摄谱仪的法布里-珀罗成像系统
DOI:
10.1088/0004-6256/135/5/1825
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发表时间:
2007
期刊:
影响因子:
--
通讯作者:
IC Optical Systems Ltd.
中科院分区:
文献类型:
--
作者:
N. Rangwala;T. Williams;C. Pietraszewski;Charles L. Joseph Rutgers University;IC Optical Systems Ltd.
We present the design of the Fabry–Pérot system of the Robert Stobie Spectrograph on the 10 m class Southern African Large Telescope and its characterization as measured in the laboratory. This system provides spectroscopic imaging at any desired wavelength spanning a bandpass 430–860 nm, at four different spectral resolving powers (λ/Δλ) ranging from 300 to 9000. Our laboratory tests revealed a wavelength dependence of the etalon gap and parallelism with a maximum variation between 600–720 nm that arises because of the complex structure of the broadband multi-layer dielectric coatings. We also report an unanticipated optical effect of this multi-layer coating structure that produces a significant, and wavelength-dependent, change in the apparent shape of the etalon plates. This change is caused by two effects: the physical non-uniformities or thickness variations in the coating layers, and the wavelength dependence of the phase change upon reflection that can amplify these non-uniformities. We discuss the impact of these coating effects on the resolving power, finesse, and throughput of the system. This Fabry–Pérot system will provide a powerful tool for imaging spectroscopy on one of the world's largest telescopes.