5 citations · 11 across the 4 of their papers we have counts for
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The eSMA: description and first results
Sandrine Bottinelli, Ken H. Young, Richard Chamberlin +15
The eSMA ("extended SMA") combines the SMA, JCMT and CSO into a single facility, providing enhanced sensitivity and spatial resolution owing to the increased collecting area at the…
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…
Characterization of Instrumental Phase Stability
D. Y. Kubo, T. R. Hunter, R. D. Christensen +1
Atmospheric water vapor causes significant undesired phase fluctuations for the Submillimeter Array (SMA) interferometer, particularly in its highest frequency observing band of 69…
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…
Submillimeter Array Observations of CS J=14--13 Emission from the Evolved Star IRC+10216
K. H. Young, T. R. Hunter, D. J. Wilner +1
We present imaging observations of the evolved star IRC+10216 in the CS J=14--13 line at 685.4 GHz and associated submillimeter continuum at about 2'' resolution made with the part…