Abstract

Recently a variety of array detectors have been used in the focal plane of Czerny-Turner plane-grating spectrometers. The output signals have been coupled to a variety of storage units, resulting in optical multi-channel analyzers (OMA). We present a clarification of the method for calculating the dispersion of this instrument, as well as a table of useful spectroscopic parameters for spectrometer–detector array combinations.

© 1981 Optical Society of America

Calculation of dispersion for a plane grating in a Czerny-Turner mount: a comment; errata

Leon J. Radziemski
Appl. Opt. 20(17) 2883-2883 (1981)

Aberration properties of a Czerny–Turner spectrograph using plane-holographic diffraction grating

N. C. Das
Appl. Opt. 30(25) 3589-3597 (1991)

Optical design of a crossed Czerny–Turner spectrometer with a linear array photomultiplier tube

Chen Wang, He Chen, Yinchao Zhang, Siying Chen, Pan Guo, and Lifu Wang
Appl. Opt. 58(28) 7789-7794 (2019)

A 4-m Asymmetric Czerny-Turner Grating Spectrograph

J. H. Callomon and G. G. Chandler
Appl. Opt. 8(6) 1133-1140 (1969)

Aberration-corrected Czerny-Turner imaging spectrometer with a wide spectral region

Qingsheng Xue, Shurong Wang, and Fengqin Lu
Appl. Opt. 48(1) 11-16 (2009)