Spectrum analysis -- Tables, etc

Oscillator strength and transition probabilities for 3288 lines of Fe I [by] C.H. Corliss and J.L. Tech.

Charles H. Corliss

Atomic energy levels as derived from analyses of optical spectra.

Charlotte Emma Moore

Characteristic Roman frequencies of organic compounds [by] Francis R. Dollish, William G. Fateley [and] Freeman F. Bentley.

Francis R. Dollish

Tables of spectral lines [by] A.N. Zaidel' [and others].

Aleksandr Natanovich Zaǐdel'

Tables of spectrum lines.: Spektraltabellen. Tables des raies spectrales. [By] A.N. Zaidel' V.K. Prokof'ev [and] S.M. Raiskii.

Aleksandr Natanovich Zaǐdel'

Massachusetts Institute of Technology wavelength tables, with intensities in arc, spark, or discharge tube of more than 100,000 spectrum lines most strongly emitted by the atomic elements under normal conditions of excitation between 10,000 A. and 2000 A. arranged in order of decreasing wavelengths.: Measured and compiled under the direction of George R. Harrison by staff members of the Spectroscopy Laboratory of the Massachusetts Institute of Technology

Massachusetts Institute of Technology. Spectroscopy Laboratory

The solar spectrum 2935 A to 8770 A: second revision of Rowland's preliminary table of solar spectrum wavelengths [by] Charlotte E. Moore, M.G. Minnaert [and] J. Houtgast.

Charlotte Emma Moore

The Sadtler handbook of proton NMR spectra

editor, William W. Simons.

Tables of spectral-line intensities

[by] William F. Meggers, Charles H. Corliss, and Bourdon F. Scribner.

The Sadtler handbook of proton NMR spectra, index

editor, William W. Simons.