Observations of the OH airglow emission

Details Observations of the OH airglow emission Observations of the OH airglow emission

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..940m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 691, p. 940-944.

Astronomy and Astrophysics

Astronomy

39

Airglow, Background Radiation, Hydroxyl Radicals, Spectral Bands, Spectral Emission, Infrared Astronomy, Line Spectra, Near Infrared Radiation

Scientific paper

The OH airglow emission in the J and H bands was observed for the purpose of determining the linewidths, the precise wavelengths of individual lines, and the continuum emission level between lines. The lines were not resolved with a resolving power of about 17,000. Wavelengths and intensities were measured for approximately 120 lines from 1.1 to 1.8/micron. The continuum emission intensity was also measured on a dark night and was as low as 590 photons/sq m/sq arcsec/micron at 1.665 micron. The level is about one-fiftieth the average flux of the OH airglow emission in the H band.

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