Las Campanas Observatory
The Las Campanas Observatory ( LCO ) is an astronomical observatory owned and directed by the Carnegie Institution for Science . It is located near La Serena in Chile . The location was chosen for the observatory because of its weather structure : with a height of 2,380 m, it is mostly above the clouds and offers 300 cloud-free days per year for exploring the sky.
The observatory houses a number of reflector telescopes . The largest instruments are the two Magellan telescopes with a mirror diameter of 6.5 m. There is also the "Irénée du Pont" with a mirror diameter of 2.5 m and the "Henrietta Swope" with 1.0 meters, named after Irénée du Pont or Henrietta Hill Swope . The latter is characterized by a large field of view of 2 °, which is achieved by a certain Ritchey-Chrétien arrangement with a relatively large 25 cm secondary mirror and a Gascoigne corrector .
The Giant Magellan Telescope is under construction and when completed it is expected to be the world's largest optical telescope.
The Irénée du Pont can be operated with the following instruments:
- Direct CCD Camera
- Wide field IR camera
- Wide field reimaging CCD camera
- Boller & Chivens Spectrograph (Slit Spectrograph)
- Echelle spectrograph
- ModSpec, a spectrograph that can also be used on the Henrietta Swope telescope.
The following instruments are available for the Henrietta Swope telescope:
- Direct CCD Camera
- HgCdTe - infrared camera
- ModSpec Slit Spectrograph
The 1.3 m Warsaw University Telescope and a 13-inch refractor are also located on the site.
Web links
Coordinates: 29 ° 0 ′ 36 ″ S , 70 ° 42 ′ 11 ″ W.