Abstract

The background spectra originating from an ICP excitation source using a standard set of conditions have been tabulated and classified from 2075 to 6005 Å. These data were acquired using a high-resolution, scanning echelle monochromator capability of 0.01 Å. Background features include 205 Ar transitions; atomic spectra from H, C, and Si; and molecular band emission from the OH species. Possible spectral interferences of analysis lines with this background spectra were discussed and tabulated for first through third order overlaps.

Wavelength calibration of Fourier-transform emission spectra with applications to Fe i

R. C. M. Learner and A. P. Thorne
J. Opt. Soc. Am. B 5(10) 2045-2059 (1988)

The Observation of Extraphotographic Infrared Atomic Emission Spectra

Curtis J. Humphreys and Edward Paul
Appl. Opt. 2(7) 691-698 (1963)

Isotope Shifts in the Spectra of Dy i and Er i†

John S. Ross
J. Opt. Soc. Am. 62(4) 548-554 (1972)

Spectra of Fe, Co, Ni, and Cu Isoelectronic with Na i and Mg i

U. Feldman, L. Katz, W. Behring, and L. Cohen
J. Opt. Soc. Am. 61(1) 91-95 (1971)

Transition Probabilities in the Spectra of Ne i, Ar i, and Kr i*

Peter W. Murphy
J. Opt. Soc. Am. 58(9) 1200-1208 (1968)