SMA OBSERVER CENTER
 
IMAGE: Panoramic View of the SMA in the fog. credit: N. Patel.
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The Submillimeter Array (SMA) is an 8-element radio interferometer located atop Maunakea in Hawaii. Operating at frequencies from 180 GHz to 418 GHz, the 6m dishes may be arranged into configurations with baselines as long as 509m, producing a synthesized beam of sub-arcsecond width. Each element can observe with two receivers simultaneously, with 12 GHz bandwidth each per sideband, for a total of 48 GHz processed bandwidth. The digital correlator backend provides a uniform resolution of 140 kHz, across the entired processed bandwdith. The Submillimeter Array is a joint venture of the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics.


NEWS

2026 Apr 17: Pause in Observing

A series of storms starting in March is significantly impacting SMA operations. The SMA is pausing observing until a full assessment of the array health is possible.

2026 Apr 17: 2026A proposal deadline has passed

TAC process is on hold, pending further assessment of the SMA recovery timeline.

Current configuration: The SMA is in COM configuration

Please see the Array Configuration Schedule for more details