Poster + Paper
18 July 2024 Upgrading the submillimeter array: wSMA and beyond
Paul K. Grimes, Garrett K. Keating, Raymond Blundell, Robert D. Christensen, Mark Gurwell, Attila Kovacs, Timothy Norton, Scott N. Paine, Ramprasad Rao, Edward C.-Y. Tong, Jonathan Weintroub, David Wilner, Robert W. Wilson, Lingzhen Zeng, Qizhou Zhang
Author Affiliations +
Conference Poster
Abstract
The Submillimeter Array (SMA) is an array of 8 antennas operating at millimeter and submillimeter wavelengths on Maunakea, Hawaii, operated by the Smithsonian Astrophysical Observatory and Academia Sinica Institute of Astronomy and Astrophysics, Taiwan. Over the past several years, we have been preparing a major upgrade to the SMA that will replace the aging original receiver cryostats and receiver cartridges with all new cryostats and new 230 and 345 GHz receiver designs. This wideband upgrade (wSMA) will also include significantly increased instantaneous bandwidth, improved sensitivity, and greater capabilities for dual frequency observations. In this paper, we will describe the wSMA receiver upgrade and status, as well as the future upgrades that will be enabled by the deployment of the wSMA receivers.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Paul K. Grimes, Garrett K. Keating, Raymond Blundell, Robert D. Christensen, Mark Gurwell, Attila Kovacs, Timothy Norton, Scott N. Paine, Ramprasad Rao, Edward C.-Y. Tong, Jonathan Weintroub, David Wilner, Robert W. Wilson, Lingzhen Zeng, and Qizhou Zhang "Upgrading the submillimeter array: wSMA and beyond", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 1309639 (18 July 2024); https://doi.org/10.1117/12.3020046
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KEYWORDS
Receivers

Shape memory alloys

Cryostats

Antennas

Calibration

Prototyping

Astrophysics

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