The weighting-function method in the computation of solar and stellar spectra

Details The weighting-function method in the computation of solar and stellar spectra The weighting-function method in the computation of solar and stellar spectra

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jqsrt..37..407g&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 37, April 1987, p. 407-409.

Statistics

Computation

Absorption Spectra, Solar Spectra, Stellar Spectra, Weighting Functions

Scientific paper

Accurate expressions for the computation of absorption lines, both in solar and stellar spectra, can only be obtained with the help of differential weighting functions. For arbitrary absorption in the stellar flux, the integrated weighting function is only approximately applicable. Approximate formulae for the weighting functions are not required.

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