Running a distributed virtual observatory: U.S. Virtual Astronomical Observatory operations
Abstract
Operation of the US Virtual Astronomical Observatory shares some issues with modern physical observatories, e.g., intimidating data volumes and rapid technological change, and must also address unique concerns like the lack of direct control of the underlying and scattered data resources, and the distributed nature of the observatory itself. In this paper we discuss how the VAO has addressed these challenges to provide the astronomical community with a coherent set of science-enabling tools and services. The distributed nature of our virtual observatory-with data and personnel spanning geographic, institutional and regime boundaries-is simultaneously a major operational headache and the primary science motivation for the VAO. Most astronomy today uses data from many resources. Facilitation of matching heterogeneous datasets is a fundamental reason for the virtual observatory. Key aspects of our approach include continuous monitoring and validation of VAO and VO services and the datasets provided by the community, monitoring of user requests to optimize access, caching for large datasets, and providing distributed storage services that allow user to collect results near large data repositories. Some elements are now fully implemented, while others are planned for subsequent years. The distributed nature of the VAO requires careful attention to what can be a straightforward operation at a conventional observatory, e.g., the organization of the web site or the collection and combined analysis of logs. Many of these strategies use and extend protocols developed by the international virtual observatory community. Our long-term challenge is working with the underlying data providers to ensure high quality implementation of VO data access protocols (new and better 'telescopes'), assisting astronomical developers to build robust integrating tools (new 'instruments'), and coordinating with the research community to maximize the science enabled.
Additional Information
© 2012 Society of Photo-Optical Instrumentation Engineers (SPIE). This paper describes work done with the support of the US Virtual Astronomical Observatory. The VAO is jointly funded by the National Science Foundation (under Cooperative Agreement AST-0834235) and by the National Aeronautics and Space Administration. The VAO is managed by the VAO, LLC, a non-profit 501(c)(3) organization registered in the District of Columbia and a collaborative effort of the Association of Universities for Research in Astronomy (AURA) and the Associated Universities, Inc. (AUI).Attached Files
Published - 84480E.pdf
Submitted - 1206.4493.pdf
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Additional details
- Eprint ID
- 71522
- Resolver ID
- CaltechAUTHORS:20161027-064953346
- NSF
- AST-0834235
- NASA
- Created
-
2016-10-27Created from EPrint's datestamp field
- Updated
-
2021-11-11Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 8448