Building a Sequence of Standard Stars - Identifications and New Measurements from Photographic Plates

Details Building a Sequence of Standard Stars - Identifications and New Measurements from Photographic Plates Building a Sequence of Standard Stars - Identifications and New Measurements from Photographic Plates

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983bicds..24...13v&link_type=abstract

Bulletin d'Information du Centre de Donnees Stellaires, No.24:MAR, P. 13, 1983

Computer Science

Scientific paper

Photographic spectra of standard stars have been averaged, using an already tested procedure, to furnish reliable spectroscopic data for reference purposes. From the distribution of the continuum-normalized signals, and the hypothesis of the absence of emission lines, the authors have computed a confidence interval which can be used to discriminate weak lines from photographic noise during the identification work.

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