Answers are grounded in this paper and cite their sources.
Aims.The purpose of this paper is to introduce a robust method of data fitting convenient for dealing with astrophysical spectra contaminated by a large fraction of outliers.
No takes yet. Share an insight, caveat, or question.
Bukvić et al. (2007) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: