Purpose
CCAT is a groundbreaking submillimeter telescope that will be located at 5600 m altitude on Cerro Chajnantor in the Andes mountains of northern Chile. CCAT will combine high sensitivity, a wide field of view, and a broad wavelength range to provide an unprecedented capability for deep, large area multicolor submillimeter surveys. Science objectives include galaxy formation and evolution throughout the history of the Universe; the hot gas pervading clusters of galaxies; star formation, protoplanetary disks, and debris disks in the Milky Way galaxy; and Kuiper belt objects in the outer reaches of the Solar system. Instrumentation will include bolometer cameras, direct detection spectrometers, and heterodyne receiver arrays.
News & Events
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NEWS
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CCAT Special Session at the 221st AAS Meeting
At the 221st American Astronomical Society Meeting, held in Long Beach, California, …
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CCAT workshop in Paris, June 2012
The proposed CCAT, submillimeter telescope will be the main telescope in the next …
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EVENTS
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