NASA NTRS · 19890027073
Empirical continuum modeling for IUE low-dispersion spectra
Abstract
A numerical procedure for empirically determining a 'continuum' level in low-dispersion spectra from the IUE is described. The technique was developed for the automated fitting of SWP-LO (1150 A - 2000 A) spectra of stars of late spectral type, but it is more widely applicable.
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Bennett, Jeffrey O., Ayres, Thomas R.. 1988-09-01. Empirical continuum modeling for IUE low-dispersion spectra. https://ntrs.nasa.gov/citations/19890027073
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