Abstract
An FTS system has been constructed and operated in the range 700–10 000 cm−1. It has been used primarily for the observation of astronomical objects. Detector-noise-limited performance has been realized through the entire spectral range, and thermal background compensation has been achieved satisfactorily. Two features are emphasized: (1) the flexibility of the spectrometer in both spectral range and choice of resolution, and (2) the photometric quality.
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