Running a distributed virtual observatory: US Virtual Astronomical Observatory operations

被引:0
|
作者
McGlynn, Thomas A. [1 ]
Hanisch, Robert J. [2 ,3 ]
Berriman, G. Bruce [4 ]
Thakar, Aniruddha R. [5 ]
机构
[1] NASA, Goddard Space Flight Ctr, High Energy Astrophys Sci Arch Res Ctr, Code 660 1, Greenbelt, MD 20771 USA
[2] US Virtual Astronom Observat, Washington, DC 20036 USA
[3] space Telescope Sci Inst, Baltimore, MD 21227 USA
[4] CALTECH, Infrared Proc & Anly Ctr, Pasadena, CA 91125 USA
[5] Johns Hopkins Univ, Ctr Astrophys Sci, Baltimore, MD 21218 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
Virtual observatory; observatory operations; validation; monitoring; distributed computing;
D O I
10.1117/12.926083
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
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页数:7
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