Titlebook: Detection and Spectrometry of Faint Light; John Meaburn Book 1976 Springer Science+Business Media B.V. 1976 spectrometry

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0067-0057 from the ultra-violet to the infra-red. Likewise many of the illustrations are drawn from astronomy. However most of the ideas that are presented invariably have applications in other branches of science and wavelength domains.978-90-277-1198-4978-94-015-6914-9Series ISSN 0067-0057 Series E-ISSN 2214-7985

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N.C.T. Van Grieken,G.A. Meijer,E.J. KuipersA critical component of any spectrometer is obviously the system employed to detect the radiation. The parameters which describe the performance of this detector then invariably determine many of those which specify the overall performance of the spectrometer itself.

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https://doi.org/10.1007/978-3-642-69511-7Until the development of all-dielectric multi-layer reflection coatings, which have low light-loss coefficients, the Fabry-Pérot interferometer had very little application to the spectrometry of faint light sources, although it was used by Fabry and Buisson as early as 1911 on the relatively bright Orion nebula, though with lossy metallic layers.

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W. R?dl,K. Hofmann-Preiss,H. WorlicekThere are a variety of interferometers whose output is the inverse Fourier transformation of the spectrum being investigated.

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