Cassegrain Echelle Spectrograph
The Cassegrain Echelle Spectrograph (CASPEC) instrument was the first major ESO-built instrument at the Cassegrain focus of the ESO 3.6-metre telescope at La Silla Observatory, in Chile. The decision to build such an instrument was taken in 1974, but due to ESO’s move from Geneva, Switzerland to Garching, Germany and the difficulties in procuring a suitable 2D detector, tests at the ESO 3.6-metre telescope only started in June 1983. Visiting astronomers could observe with CASPEC beginning on 1 April 1984.
CASPEC was able to obtain high-resolution spectroscopic observations of stars, nuclei of galaxies and quasi-stellar objects (QSOs) as faint as magnitude 16 with its signal-to-noise ratio, that were only then possible to obtain with large coudé instruments. This gave ESO astronomers the possibility to carry out detailed observations of the physical conditions and abundances of faint stars and extragalactic observations at this spectral resolution for the first time.
Over time, CASPEC was upgraded to optical cameras and several CCDs of increasing sensitivity and resolution. During its 15-year lifetime, CASPEC was used for a large variety of scientific programs and contributed to many important discoveries. In 1987, for example, CASPEC helped in the discovery of the most distant known object in the Universe at that time. About ten years later CASPEC helped studying a major transition period in the early Universe, providing a high-resolution spectrum of a bright southern quasar.
CASPEC was decommissioned in 1999.
This table lists the global capabilities of the instrument. The authoritative technical specifications as offered for astronomical observations are available from the Science Operations page.