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Correction of observational profiles of spectral lines
Authors:M G Smith  A N Walker
Institution:(1) Dept. of Astronomy, University of Manchester, England;(2) Present address: Kitt Peak National Observatory, Tucson, Ariz., USA
Abstract:The profiles obtained from radial-velocity observations of the Rosette Nebula with a Fabry-Pérot (F.P.) interferometer (Meaburn andSmith, 1968) had to be corrected, for the spreading action of the instrumental function, and for motion of the observer. Two current methods are compared and a method devised for fitting a sum of Gaussians to a noisy output profile.
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