LWIR stellar calibration: Infrared spectral curves for 30 standard stars

Details LWIR stellar calibration: Infrared spectral curves for 30 standard stars LWIR stellar calibration: Infrared spectral curves for 30 standard stars

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991stin...9128052e&link_type=abstract

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Physics

Calibrating, Curves (Geometry), Infrared Stars, Spectral Energy Distribution, Flux (Rate), Infrared Spectra, Line Spectra

Scientific paper

Best estimate spectral energy distributions are created for approximately 30 stars by fitting theoretically expected spectral curves to the available empirical flux data on the stars at a variety of wavelengths. The curves can be integrated over the band response functions for a given sensor in order to produce broadband power predictions against which to calibrate.

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