Correction of Observational Profiles of Spectral Lines

Details Correction of Observational Profiles of Spectral Lines Correction of Observational Profiles of Spectral Lines

Mar 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968ap%26ss...1..151s&link_type=abstract

Astrophysics and Space Science, Volume 1, Issue 2, pp.151-165

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

The profiles obtained from radial-velocity observations of the Rosette Nebula with a Fabry-Pérot (F.P.) interferometer ( Meaburn and Smith, 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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