The automatic reduction of emission line spectra

Details The automatic reduction of emission line spectra The automatic reduction of emission line spectra

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..69..393t&link_type=abstract

Astrophysics and Space Science, vol. 69, no. 2, May 1980, p. 393-399.

Astronomy and Astrophysics

Astrophysics

4

Emission Spectra, Line Spectra, Nebulae, Night Sky, Radiation Counters, Curve Fitting, H Lines, Normal Density Functions, Oxygen, Photons, Statistical Distributions

Scientific paper

A method of reducing slit spectra of nebular emission lines - obtained
with a photon counting detector - is described, with particular emphasis
on the correct use of statistics. The spectral information is finally
presented as a list of wavelength, half-width and intensities of
Gaussian profiles.

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