19 citations · 34 across the 4 of their papers we have counts for
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Phase Closure at 691 GHz using the Submillimeter Array
T. R. Hunter, A. E. T. Schinckel, A. B. Peck +6
Phase closure at 682 GHz and 691 GHz was first achieved using three antennas of the Submillimeter Array (SMA) interferometer located on Mauna Kea, Hawaii. Initially, phase closure…
Dual frequency 230/690 GHz interferometry at the Submillimeter Array
Todd R. Hunter, John W. Barrett, Raymond Blundell +13
The Submillimeter Array (SMA), a collaboration between the Smithsonian Astrophysical Observatory and the Academica Sinica Institute for Astronomy and Astrophysics of Taiwan, is an…
The Submillimeter Array Antennas and Receivers
R. Blundell
The Submillimeter Array (SMA) was conceived at the Smithsonian Astrophysical Observatory in 1984 as a six element interferometer to operate in the major atmospheric windows from ab…
Observations in the 1.3 and 1.5 THz Atmospheric Windows with the Receiver Lab Telescope
D. P. Marrone, R. Blundell, E. Tong +5
The Receiver Lab Telescope (RLT) is a ground-based terahertz telescope; it is currently the only instrument producing astronomical data between 1 and 2 THz. The capabilities of the…
Characterization and Status of a Terahertz Telescope
D. P. Marrone, R. Blundell, H. Gibson +3
The Receiver Lab Telescope (RLT) is a ground-based terahertz observatory, located at an altitude of 5525 m on Cerro Sairecabur, Chile. The RLT has been in operation since late 2002…