Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26as..122..371w&link_type=abstract
A & A Supplement series, Vol. 122, April II 1997, 371-380.
Astronomy and Astrophysics
Astronomy
Methods: Data Analysis: Numerical, Techniques: Image Processing
Scientific paper
This describes a technique for fitting baselines or continua to scans or spectra with a large proportion occupied by signal in the form of sources or emission/absorption lines. It is essentially a high-pass filtering technique; the very lowest Fourier frequencies are ``filtered out" by using them to construct a model of the continuum. The technique is interactive, and subjective in that some decision is required by the analyst; but it is very stable despite this. Errors are analyzed and some examples are given to demonstrate the versatility of the technique. The route to generating an objective (hands-off) technique is discussed.
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