The Submillimeter Array
Top Cited Papers
- 28 October 2004
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 616 (1) , L1-L6
- https://doi.org/10.1086/423245
Abstract
The Submillimeter Array, a collaborative project of the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics, has begun operation on Mauna Kea in Hawaii. The array comprises a total of eight 6 m telescopes, which will cover the frequency range of 180-900 GHz. All eight telescopes have been deployed and are operational. First scientific results utilizing the three receiver bands at 230, 345, and 690 GHz have been obtained and are presented in the accompanying Letters.Keywords
All Related Versions
This publication has 27 references indexed in Scilit:
- Submillimeter Observations of Titan: Global Measures of Stratospheric Temperature, CO, HCN, HC 3 N, and the Isotopic Ratios 12 C/ 13 C and 14 N/ 15 NThe Astrophysical Journal, 2004
- Organic Molecules in Low-Mass Protostellar Hot Cores: Submillimeter Imaging of IRAS 16293-2422The Astrophysical Journal, 2004
- Subarcsecond Submillimeter Continuum Observations of Orion KLThe Astrophysical Journal, 2004
- Submillimeter Array Outflow/Disk Studies in the Massive Star-forming Region IRAS 18089-1732The Astrophysical Journal, 2004
- High-Density Molecular Gas in the Infrared-bright Galaxy System VV 114The Astrophysical Journal, 2004
- High-Velocity Bipolar Outflow and Disklike Envelope in the Carbon Star V HydraeThe Astrophysical Journal, 2004
- Atmospheric Phase Correction Using Total Power Radiometry at the Submillimeter ArrayThe Astrophysical Journal, 2004
- Submillimeter Array Multiline observations of the Massive Star-forming region IRAS 18089-1732The Astrophysical Journal, 2004
- Receiver control for the Submillimeter ArrayPublished by SPIE-Intl Soc Optical Eng ,2002
- The Shapes of Cross‐Correlation InterferometersThe Astrophysical Journal, 1997