NASA NTRS · 19830032235
Infrared spectroscopy in astronomy
Abstract
The use of infrared spectroscopy in astronomy has increased dramatically in the past ten years. The broad design considerations are discussed in terms of wavelength coverage and resolution. Three rough resolution ranges, lambda/Delta lambda of approximately 100, 1000 and 10,000, are identified in which various types of astronomical problems can be studied. Numerous existing systems are briefly discussed and references are given to more complete descriptions.
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Houck, J. R.. 1981-01-01. Infrared spectroscopy in astronomy. https://ntrs.nasa.gov/citations/19830032235
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