Correction of the Atmospheric Transmission in Infrared Spectroscopy

Details Correction of the Atmospheric Transmission in Infrared Spectroscopy Correction of the Atmospheric Transmission in Infrared Spectroscopy

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aj....111..537m&link_type=abstract

Astronomical Journal v.111, p.537

Astronomy and Astrophysics

Astronomy

62

Atmospheric Effects, Infrared: General

Scientific paper

High-resolution and sensitive near-infrared spectroscopy is often limited by the ability to correct the atmospheric transmission. The simple division of the object spectrum by the spectrum of a nearby star turns out to be unsatisfactory because of the stellar features in the latter. We show how to measure the atmospheric transmission with a nearby early GV or late FV star, and to correct for the stellar features by means of the (atmospheric-transmission-corrected) solar spectrum.

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