An Imaging Fabry-Perot System for the Robert Stobie Spectrograph on the Southern African Large Telescope

Details An Imaging Fabry-Perot System for the Robert Stobie Spectrograph on the Southern African Large Telescope An Imaging Fabry-Perot System for the Robert Stobie Spectrograph on the Southern African Large Telescope

2007-10-19

arxiv.org/abs/0710.3750v2

Astronomy and Astrophysics

Astrophysics

17 pages, 14 figures, accepted for publication in The Astronomical Journal

Scientific paper

10.1088/0004-6256/135/5/1825

We present the design of the Fabry-Perot system of the Robert Stobie Spectrograph on the 10-meter 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 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 refection 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-Perot system will provide a powerful tool for imaging spectroscopy on one of the world's largest telescopes.

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