Location(s) | Atacama Desert |
---|---|
Coordinates | 22°58′11″S 67°42′08″W / 22.9697°S 67.7022°W |
Altitude | 4,800 m (15,700 ft) |
Wavelength | 0.34 mm (880 GHz)–2.73 mm (110 GHz) |
Telescope style |
Cassegrain reflector radio telescope |
Diameter | 4 m (13 ft 1 in) |
Website |
www |
Related media on Commons | |
The NANTEN2 Observatory is a southern sky observatory in the Atacama Desert of northern Chile. It is located at an altitude of 4,800 m (15,748 ft) on Pampa la Bola next to Cerro Chajnantor. [1] [2] The observatory is equipped with a millimeter and submillimeter wave telescope that is used for southern sky observations of atomic and molecular spectral lines in 110 GHz to 880 GHz range. [3] It is one of a number of observatories operating at Llano de Chajnantor Observatory. It is operated as a collaboration between research institutes in Japan ( Nagoya University and Osaka University), South Korea ( Seoul National University), Germany (KOSMA, Universität zu Köln, Argelander Institute for Astronomy at the University of Bonn), Australia ( University of New South Wales, University of Adelaide, Macquarie University, Swinburne University of Technology, University of Sydney, University of Western Sydney) and Chile ( Universidad de Chile).
The instrument was previously located at the Las Campanas Observatory from 1995 to 2004; it was known as the NANTEN millimeter-wavelength radio telescope back then.
Location(s) | Atacama Desert |
---|---|
Coordinates | 22°58′11″S 67°42′08″W / 22.9697°S 67.7022°W |
Altitude | 4,800 m (15,700 ft) |
Wavelength | 0.34 mm (880 GHz)–2.73 mm (110 GHz) |
Telescope style |
Cassegrain reflector radio telescope |
Diameter | 4 m (13 ft 1 in) |
Website |
www |
Related media on Commons | |
The NANTEN2 Observatory is a southern sky observatory in the Atacama Desert of northern Chile. It is located at an altitude of 4,800 m (15,748 ft) on Pampa la Bola next to Cerro Chajnantor. [1] [2] The observatory is equipped with a millimeter and submillimeter wave telescope that is used for southern sky observations of atomic and molecular spectral lines in 110 GHz to 880 GHz range. [3] It is one of a number of observatories operating at Llano de Chajnantor Observatory. It is operated as a collaboration between research institutes in Japan ( Nagoya University and Osaka University), South Korea ( Seoul National University), Germany (KOSMA, Universität zu Köln, Argelander Institute for Astronomy at the University of Bonn), Australia ( University of New South Wales, University of Adelaide, Macquarie University, Swinburne University of Technology, University of Sydney, University of Western Sydney) and Chile ( Universidad de Chile).
The instrument was previously located at the Las Campanas Observatory from 1995 to 2004; it was known as the NANTEN millimeter-wavelength radio telescope back then.