Abstract

A polarization Fourier spectrometer is described that improves on the previous versions built by others and can be used from 0.3 μ to 2.5 μ. Several practical problems in the construction and data reduction are discussed, and a number of typical results are presented to show the performance of the instrument.

© 1974 Optical Society of America

Infrared Fourier spectrometer for airborne and ground-based astronomy

D. Scott Davis, Harold P. Larson, Michael Williams, Guy Michel, and Pierre Connes
Appl. Opt. 19(24) 4138-4155 (1980)

Two Asymmetric Hadamard Transform Spectrometers

Martin Harwit, Perry G. Phillips, Leon W. King, and Daniel A. Briotta
Appl. Opt. 13(11) 2669-2674 (1974)

Astronomical Fourier spectrometer

Pierre Connes and Guy Michel
Appl. Opt. 14(9) 2067-2084 (1975)

Infrared Fourier spectrometer for laboratory use and for astronomical studies from aircraft and ground-based telescopes

Harold P. Larson and Uwe Fink
Appl. Opt. 14(9) 2085-2095 (1975)

Chirped Fourier Spectroscopy. 1:Dynamic Range Improvement and Phase Correction

Thomas P. Sheahen
Appl. Opt. 13(12) 2907-2912 (1974)