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Automatic detection of objective prism stellar spectra
1998
Astronomy and Astrophysics Supplement Series
Object detection is a common problem in image processing and particularly in astronomy and astrophysics, when a huge number of objects are to be processed. Such is the case of objective prism plates, where thousands of spectra are recorded. We present a new method for automatic detection of stellar spectra on digitally-scanned objective prism plates. Our method is based on signal processing techniques with emphasis on obtaining the maximum signal-to-noise ratio from the data, as well as on
doi:10.1051/aas:1998322
fatcat:5ljzmnd26jhfnnsjxfjzjjknwm