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- W2017556406 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 SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only." @default.
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- W2017556406 date "1995-06-26" @default.
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- W2017556406 title "<title>Spectrometer for astrometric interferometry</title>" @default.
- W2017556406 doi "https://doi.org/10.1117/12.212990" @default.
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