Paper
15 July 2016 Centralized operations and maintenance planning at the Atacama Large Millimeter/submillimeter Array (ALMA)
Bernhard Lopez, Nicholas D. Whyborn, Serge Guniat, Octavio Hernandez, Stefan Gairing
Author Affiliations +
Abstract
The Atacama Large Millimeter/submillimeter Array (ALMA) is a joint project between astronomical organizations in Europe, North America, and East Asia, in collaboration with the Republic of Chile. ALMA consists of 54 twelve-meter antennas and 12 seven-meter antennas operating as an aperture synthesis array in the (sub)millimeter wavelength range. Since the inauguration of the observatory back in March 2013 there has been a continuous effort to establish solid operations processes for effective and efficient management of technical and administrative tasks on site. Here a key aspect had been the centralized maintenance and operations planning: input is collected from science stakeholders, the computerized maintenance management system (CMMS) and from the technical teams spread around the world, then this information is analyzed and consolidated based on the established maintenance strategy, the observatory long-term plan and the short-term priorities definitions. This paper presents the high-level process that has been developed for the planning and scheduling of planned- and unplanned maintenance tasks, and for site operations like the telescope array reconfiguration campaigns. We focus on the centralized planning approach by presenting its genesis, its current implementation for the observatory operations including related planning products, and we explore the necessary next steps in order to fully achieve a comprehensive centralized planning approach for ALMA in steady-state operations.
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Bernhard Lopez, Nicholas D. Whyborn, Serge Guniat, Octavio Hernandez, and Stefan Gairing "Centralized operations and maintenance planning at the Atacama Large Millimeter/submillimeter Array (ALMA)", Proc. SPIE 9910, Observatory Operations: Strategies, Processes, and Systems VI, 99100M (15 July 2016); https://doi.org/10.1117/12.2230992
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KEYWORDS
Telescopes

Calibration

Observatories

Stars

Spectrographs

Cameras

Sensors

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