Abstract

Many spectra, particularly infrared spectra, are recorded on charts which are linear in transmittance as the ordinate vs wavelength or wave number as the abscissa. When these records are used for quantitative analysis, the data must be converted to absorbance.

Absorptivity Recorder

D. D. Tunnicliff and Roland C. Hawes
J. Opt. Soc. Am. 50(11) 1039-1042 (1960)

Correction of interferogram data acquired using a focal plane FT-IR spectrometer system

Cong Gao, Jianhua Mao, and Ren Chen
Appl. Opt. 57(10) 2434-2440 (2018)

Measuring Spectral Transmittances of Photographic Objectives with the Cary Model 11 MS Recording Spectrophotometer*

F. Grum and F. C. Williams
J. Opt. Soc. Am. 50(7) 675-677 (1960)

A Gamma-Nomograph*

Edwin S. Hodge
J. Opt. Soc. Am. 41(10) 731_1-732 (1951)

Hole burning, Stark effect, and data storage: 2: holographic recording and detection of spectral holes

Cosimo De Caro, Alois Renn, and Urs P. Wild
Appl. Opt. 30(20) 2890-2898 (1991)