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Las Campanas Observatory (LCO) is an astronomical observatory owned and operated by the Carnegie Institution for Science (CIS). It is located in the southern Atacama Desert of Chile in the Atacama Region approximately 100 kilometres (62 mi) northeast of the city of La Serena. The LCO telescopes and other facilities are located near the northern end of a 7 km (4.3 mi) long mountain ridge. Cerro Las Campanas, near the southern end and over 2,500 m (8,200 ft) high, is the future home of the Giant Magellan Telescope.
LCO was established in 1969 and is the primary observing facility of CIS. It supplanted Mount Wilson Observatory in that role due to increasing light pollution in the Los Angeles area. The headquarters of Carnegie Observatories is located in Pasadena, California, while the main office in Chile is in La Serena next to the University of La Serena and a short distance from the Association of Universities for Research in Astronomy facility.
On February 24, 1987 at LCO, Ian Shelton and Oscar Duhalde became the first official observers of Supernova 1987A (SN 1987A).
The 6.5 m (260 in) Magellan Telescopes are two identical single-mirror reflecting telescopes. The Walter Baade Telescope saw first light in 2000, and the Landon Clay Telescope in 2002. They are managed by LCO for an international consortium of institutions which includes LCO.
The 2.5 m (98 in) du Pont Telescope is named after industrialist Irénée du Pont and has been in operation since 1977. It is a Ritchey-Chrétien telescope with a Gascoigne corrector lens, and was built by Boller & Chivens and L&F Industries.
The 1.0 m (39 in) Swope Telescope was the first telescope installed at LCO, and began operating in 1971. It is named after CIS astronomer Henrietta Swope. It is a Ritchey-Chrétien telescope built by Boller & Chivens with a Gascoigne corrector lens.
The 1.3 m (51 in) Warsaw Telescope is the main instrument of the Optical Gravitational Lensing Experiment operated by the University of Warsaw Observatory. Installed in 1996, it is a Ritchey-Chrétien design built by DFM Engineering.
The All Sky Automated Survey (ASAS) is a project to monitor the southern sky for variable stars. It consists of two wide-field telescopes, one narrow field telescope, and one ultra-wide field telescope. A prototype system was installed in 1996 and a second in 1997, both in the same enclosure as the 10-inch astrograph. The three larger telescopes were installed in 2000. The ultra-wide device was added in 2002 when the existing telescopes were moved to a new, smaller enclosure.
The Hungarian Automated Telescope South (HAT-South) facility is part of the HATNet Project to detect exoplanets using the transit method. It consists of a pair of four 0.18 m (7.1 in) Takahasi reflecting astrographs on a common mount. It was installed in 2009.
The Birmingham Solar Oscillations Network (BiSON) operates at station at LCO.
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