Empirical continuum modeling for IUE low-dispersion spectra

Details Empirical continuum modeling for IUE low-dispersion spectra Empirical continuum modeling for IUE low-dispersion spectra

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1129b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Sept. 1988, p. 1129-1133.

Statistics

Computation

7

Astronomical Spectroscopy, Computational Astrophysics, Continuous Radiation, Late Stars, Ultraviolet Spectra, Background Radiation, Broadband, Stellar Spectra

Scientific paper

The authors describe a numerical procedure for empirically determining a
"continuum" level in low-dispersion spectra from the International
Ultraviolet Explorer. They developed the technique for the automated
fitting of SWP-LO (1150 Å - 2000 Å) spectra of stars of late
spectral type, but it is more widely applicable.

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