Paper
9 August 2016 Meeting the challenges of bringing a new base facility operation model to Gemini Observatory
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Abstract
The aim of the Gemini Observatory’s Base Facilities Project is to provide the capabilities to perform routine night time operations with both telescopes and their instruments from their respective base facilities without anyone present at the summit. Tightening budget constraints prompted this project as both a means to save money and an opportunity to move toward increasing remote operations in the future.

We successfully moved Gemini North nighttime operation to our base facility in Hawaii in Nov., 2015. This is the first 8mclass telescope to completely move night time operations to base facility. We are currently working on implementing BFO to Gemini South.

Key challenges for this project include: (1) This is a schedule driven project. We have to implement the new capabilities by the end of 2015 for Gemini North and end of 2016 for Gemini South. (2) The resources are limited and shared with operations which has the higher priority than our project. (3) Managing parallel work within the project. (4) Testing, commissioning and introducing new tools to operational systems without adding significant disruptions to nightly operations. (5) Staff buying to the new operational model. (6) The staff involved in the project are spread on two locations separated by 10,000km, seven time zones away from each other. To overcome these challenges, we applied two principles: "Bare Minimum" and "Gradual Descent". As a result, we successfully completed the project ahead of schedule at Gemini North Telescope. I will discuss how we managed the cultural and human aspects of the project through these concepts. The other management aspects will be presented by Gustavo Arriagada [2], the Project Manager of this project. For technical details, please see presentations from Andrew Serio [3] and Martin Cordova [4].
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Atsuko Nitta, Gustavo Arriagada, A. J. Adamson, Martin Cordova, Arturo Nunez, Andrew Serio, and Scot Kleinman "Meeting the challenges of bringing a new base facility operation model to Gemini Observatory", Proc. SPIE 9911, Modeling, Systems Engineering, and Project Management for Astronomy VII, 99111Q (9 August 2016); https://doi.org/10.1117/12.2232084
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KEYWORDS
Gemini Observatory

Ferroelectric materials

Observatories

Phase modulation

Telescopes

Systems engineering

Lead

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