Abstract
Multi-object slit spectroscopy with a wide-field telescope is potentially a very effective way of collecting large quantities of data for statistical analysis on a wide variety of astronomical object-c1asses. A pilot-model system with 40 channels has been developed for the 1.2-metre UK Schmidt telescope, and has been extensively tested with photographic detection of the spectra. The commissioning of a dedicated cooled CCD camera in the immediate future is expected to lead to the rapid implementation of a user service with the system.
| Original language | English |
|---|---|
| Pages (from-to) | 787-796 |
| Number of pages | 10 |
| Journal | Proceedings of SPIE - The International Society for Optical Engineering |
| Volume | 627 |
| DOIs | |
| Publication status | Published - 13 Oct 1986 |
| Externally published | Yes |
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