Submillimeter Atmospheric Transparency at Maunakea, at the South Pole, and at Chajnantor
نویسندگان
چکیده
For a systematic assessment of submillimeter observing conditions at different sites, we constructed tipping radiometers to measure the broad band atmospheric transparency in the window around 350μm wavelength. The tippers were deployed on Maunakea, Hawaii, at the South Pole, and in the vicinity of Cerro Chajnantor in northern Chile. Identical instruments permit direct comparison of these sites. Observing conditions at the South Pole and in the Chajnantor area are better than on Maunakea. Simultaneous measurements with two tippers demonstrate conditions at the summit of Cerro Chajnantor are significantly better than on the Chajnantor plateau. Subject headings: Atmospheric effects — Instrumentation: tipping radiometers — Site testing — Astronomical instruments — Radio telescopes and equipment — Earth: atmosphere
منابع مشابه
Observing Conditions for Submillimeter Astronomy
Consistently superb observing conditions are crucial for achieving the scientific objectives of a telescope. Submillimeter astronomy is possible only at a few exceptionally dry sites, notably Mauna Kea, the Antarctic plateau, and the Chajnantor region in the high Andes east of San Pedro de Atacama in northern Chile. Long term measurements of 225 GHz and 350μm atmospheric transparency demonstrat...
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