Translator Disclaimer
Paper
12 July 2008 Overview of engineering activities at the SMA
Author Affiliations +
Abstract
The Submillmeter Array (SMA) consists of 8 6-meter telescopes on the summit of Mauna Kea. The array has been designed to operate from the summit of Mauna Kea and from 3 remote facilities: Hilo, Hawaii, Cambridge, Massachusetts and Taipei, Taiwan. The SMA provides high-resolution scientific observations in most of the major atmospheric windows from 180 to 700 GHz. Each telescope can house up to 8 receivers in a single cryostat and can operate with one or two receiver bands simultaneously. The array being a fully operational observatory, the demand for science time is extremely high. As a result specific time frames have been set-aside during both the day and night for engineering activities. This ensures that the proper amount of time can be spent on maintaining existing equipment or upgrading the system to provide high quality scientific output during nighttime observations. This paper describes the methods employed at the SMA to optimize engineering development of the telescopes and systems such that the time available for scientific observations is not compromised. It will also examine some of the tools used to monitor the SMA during engineering and science observations both at the site and remote facilities.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
R. D. Christensen, D. Y. Kubo, and Ramprasad Rao "Overview of engineering activities at the SMA", Proc. SPIE 7016, Observatory Operations: Strategies, Processes, and Systems II, 701608 (12 July 2008); https://doi.org/10.1117/12.787673
PROCEEDINGS
12 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

Japanese Large Millimeter and Submillimeter Array
Proceedings of SPIE (July 31 1998)
The Australian SKA Pathfinder
Proceedings of SPIE (September 17 2012)
Constructing the EVLA while operating the VLA
Proceedings of SPIE (July 28 2010)
The Allen Telescope Array
Proceedings of SPIE (September 28 2004)
The Atacama Large Millimeter Array (ALMA)
Proceedings of SPIE (February 04 2003)
The ALMA OT in early science: supporting multiple customers
Proceedings of SPIE (September 24 2012)

Back to Top