The DETSP procedure tests have been run in the Astronomical Institute under MIDAS-96NOV environment
on a Hewlett-Packard HP-C160 workstation with 64-bit CPU, 64MB RAM, and operating system
HP-UX 10.20. We used two frames from digitized high-quality copies of spectral
plates taken with the 1.2 UK Schmidt Telescope in Australia. The one is a pixels
frame lpr31r from an image scanned by the Super-COSMOS facility at the Royal Observatory of Edinburgh.
The other is the a53em frame of
pixels from an image
digitized by a PDS 1010A microdensitometer at the Trieste Observatory.
Experts detected spectra in these frames using standard methods of detection
on direct and spectral plates.
Applying the DETSP procedure, we had 553 detections (Fig. 2)
and 13 undetected spectra (error ) for the frame lpr31r. For the
frame a53em, we had 427 detections (Fig. 3) and 17
undetected spectra (error
). A careful analysis showed that the missed
spectra are in majority too faint, so they are unusable for further
processing (e.g. automated classification). Applying the described method,
a very significant number of spectra were automatically detected
(True-Positive detections
). It is worth to point out that despite
the presence of M-type and Carbon star spectra on the frames, there were no
false detections. In both cases, the processing took about 20 min without
displaying supporting plots and images and about twice more with them.
Implementation of this MIDAS procedure in a C language program will
significantly reduce this processing time. The results are very encouraging
for this procedure as well as for the next steps, extraction and classification, of the OBJPR context for automated processing of objective prism spectra.
This research has been supported by a grant from the General Secretariat of Research and Technology of Greece, PENED programme. The authors are grateful to the UK Schmidt Telescope Plate Library (ROE) for the loan of the observational material.
Copyright The European Southern Observatory (ESO)