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The Submillimeter Array

2007/06/01 by R. Blundell · 1 citation
Physics and Astronomy · Engineering · #Radio Astronomy Observations and Technology #Superconducting and THz Device Technology #Scientific Research and Discoveries #Radio astronomy #Cryostat #Cryocooler #Superheterodyne receiver #Physics #Antenna (radio) #Observatory #Interferometry #Radio telescope #Astronomy #Infrared astronomy #Angular resolution (graph drawing) #Heterodyne (poetry) #Submillimeter Array #Remote sensing #Optics #Microwave #Infrared #Electrical engineering #Engineering #Geology #Galaxy #Superconductivity #Acoustics

paper · doi:10.1109/mwsym.2007.380132

openalex publication_date 2007/06/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/29

Abstract

The submillimeter array, a collaboration between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics of Taiwan, is a pioneering radio-interferometer made up of eight 6-meter diameter antennas designed for high angular resolution astronomical observations of the cool universe throughout the major atmospheric windows from about 200 to 900 GHz. Each antenna houses a single cryostat, with an integrated cryocooler that can cool eight heterodyne receivers to 4 K. Four receiver bands are available: 180-250 GHz, 266-355 GHz, 320-420 GHz, and 600-700 GHz, and simultaneous observations are possible in any pair of high and low frequency receiver bands.

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