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Paper: A CO Survey of the Southern Galaxy
Volume: 217, Imaging at Radio Through Submillimeter Wavelengths
Page: 66
Authors: Bronfman, L.; May, J.; Luna, A.
Abstract: On December 12th 1982 the 1.2 mSouthern Millimeter Wave Telescope, an instrument specifically designed for CO surveys of molecular clouds in the Southern Galaxy, arrived Cerro Tololo after being constructed and tested atop the roof of the Goddard Institute for Space Studies by Columbia University staff and students, and by Universidad de Chile and NASA personnel. The telescope saw first light on December 22nd 1982, and has been operational ever since. During these years we have completed deep CO surveys of the Carina arm (Grabelsky et al. 1987), the IV galactic quadrant (Bronfman et al. 1988), the III galactic quadrant (May et al. 1993), and the galactic center (Bitran et al. 1997), contributing with a major fraction of the presently available galactic CO data. When combined with CO surveys of the I and II galactic quadrants obtained with its twin instrument, the Northern 1.2m Millimeter Wave Telescope now at the Center for Astrophysics, these data provided for the first time a complete, well sampled, and homogeneous picture of the molecular gas content of the Milky Way.
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