Abstract

A method for using a computer in conjunction with photon counting is described. The computer system (University of Michigan Amdahl 470V/6) is not dedicated but the programming gives a fast, efficient, versatile, and accurate calibration of high resolution visible-uv spectra. In addition, the system greatly enhances and facilitates the production of plots of the spectrum, integration of spectral intensities, and signal averaging of weak spectra.

Line shapes in high-resolution optoacoustic spectroscopy

P. Minguzzi, S. Profeti, M. Tonelli, and A. Di Lieto
J. Opt. Soc. Am. B 3(8) 1075-1081 (1986)

Interpolation errors in UV–visible spectroscopy for stratospheric sensing: implications for sensitivity, spectral resolution, and spectral range

H. K. Roscoe, D. J. Fish, and R. L. Jones
Appl. Opt. 35(3) 427-432 (1996)

High Resolution Luminescence Spectrometer. 2:Data Treatment and Corrected Spectra

Vo Dinh Tuan and Urs P. Wild
Appl. Opt. 13(12) 2899-2906 (1974)

Line-shape studies in high-resolution stimulated resonance Raman spectroscopy and application to accurate determinations of hyperfine splittings in I₂

Ch. J. Bordé, G. Camy, N. Courtier, F. du Burck, A. N. Goncharov, and M. Gorlicki
J. Opt. Soc. Am. B 13(9) 1837-1848 (1996)

Rocket-borne instrument with a high-resolution microchannel plate detector for planetary UV spectroscopy

William E. McClintock, Charles A. Barth, Robert E. Steele, George M. Lawrence, and J. Gethyn Timothy
Appl. Opt. 21(17) 3071-3079 (1982)