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Near-infrared spectrophotometry of Titan

Icarus, 1975
Several unusual features in the near-IR spectrum of Titan are examined. Observations during four apparitions establish the reality of the S(1) absorption at 8150.7 A, but the existence of the S(O) absorption at 8272.7 A will require further sightings to become definitively established. These two features are particularly important, as they bear on the
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Near Infrared Absorption Spectrophotometry

Applied Spectroscopy, 1952
Interest in several regions of the electromagnetic spectrum has increased greatly since the War under the stimulation of new apparatus for the generation and detection of radiation. Just as the perfection of the magnetron and the klystron has given the spectroscopist relatively powerful sources of ...
James L. Lauer, E. J. Rosenbaum
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Quantitative Analysis by Infrared Spectrophotometry

Applied Spectroscopy Reviews, 1970
Abstract To complement some current references [1,2] on quantitative infrared analysis, the following goals have been set for this paper: To assess the recent history of quantitative infrared analysis. To describe and illustrate instrumentation and techniques for measuring infrared absorbance simply but precisely.
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Typing of Klebsiella by Infrared Spectrophotometry

Journal of Infectious Diseases, 1955
S, LEVINE   +3 more
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Infrared Spectrophotometry

2020
Thomas J. Bruno, Paris D.N. Svoronos
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Spectrophotometry of Stars in the Near Infrared

1987
The aim of this exercise is to become acquainted with some aspects of spectro-photometrical observations in the near infrared with modern detectors and mainly with the calibration problem. Any spectrophotometrical work i.e. any attempt to derive the spectral energy distribution of a star includes the determination of the response curve of the system, S(
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Infrared Spectrophotometry

1973
R.D.B. Fraser, T.P. MacRae
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