Paper
26 June 1995 Spectrometer for astrometric interferometry
Author Affiliations +
Abstract
I present a spectrometer for a dispersed-fringe optical astrometric interferometer. The two primary requirements, that integration time and systematic error be minimized, do not interact, and both are met. The integration time at the minimum is only a weak function of the parameters, allowing adjustment for secondary criteria such as cross-dispersion resolution without significantly increasing integration time.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
James D. Phillips "Spectrometer for astrometric interferometry", Proc. SPIE 2477, Spaceborne Interferometry II, (26 June 1995); https://doi.org/10.1117/12.212990
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KEYWORDS
Sensors

Spectroscopy

Stars

Prisms

Charge-coupled devices

Visibility

Beam splitters

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