13 citations · 59 across the 11 of their papers we have counts for
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658 GHz Vibrationally-Excited Water Masers with the Submillimeter Array
T. R. Hunter, K. H. Young, R. D. Christensen +1
Discovered in 1995 at the Caltech Submillimeter Observatory (CSO), the vibrationally-excited water maser line at 658 GHz (455 micron) is seen in oxygen-rich giant and supergiant st…
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…