most citedObservations in the 1.3 and 1.5 THz Atmospheric Windows with the Receiver Lab Telescope

19 citations · 34 across the 4 of their papers we have counts for

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astro-ph20071 cited

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…

astro-ph20054 cited

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…

astro-ph20057 cited

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…

astro-ph200519 cited

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…

astro-ph20044 cited

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…