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20042008
most citedThe eSMA: description and first results

5 citations · 11 across the 4 of their papers we have counts for

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astro-ph20085 cited

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…

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-ph20071 cited

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…

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-ph2004

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…