Classification of Low-Resolution Stellar Spectra via Template Matching — A Simulation Study
Reference17 articles.
1. Adorf, H.-M., Röser, H.-J., 1984, Reduction of Slitless Spectra — The Detection of Faint Emission Lines, in: “Astronomy with Schmidt-type Telescopes, IAU Colloq. No. 78, Asiago 1983”, M. Capaccioli, ed., D. Reidel, Dordrecht, p. 423. 2. Banse, K., Crane, Ph., Ounnas, Ch., Ponz, D., 1983, MIDAS - ESO’s Interactive Image Processing System, in: “Proc. Digital Equipment Computer Users Society”, Zurich, p. 87. 3. Christian, C.A., 1982, Identification of Field Stars Contaminating the Color-Magnitude Diagram of the Open Cluster Be 21, Astrophys. J. Suppl. Ser., 49: 555. 4. Clowes, R.G., 1984, Automatic Processing of Objective-Prism Plates at the Royal Observatory, Edinburgh, in: “Astronomy with Schmidt-type Telescopes, IAU Colloq. No. 78, Asiago 1983”, M. Capaccioli, ed., D. Reidel, Dordrecht, p. 107. 5. Clowes, R.G., 1986, Automated quasar detection in the SGP filed: a clustering study, Mon. Not. Royal Astron. Soc., 218: 139.
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