Wide-Field Astronomical Surveys in the Next Decade

Strauss, Michael A. ; /Princeton U. ; Tyson, J.Anthony ; /UC, Davis ; Anderson, Scott F. ; /Washington U., Seattle, Astron. Dept. ; Axelrod, T.S. ; /LSST Corp. ; Becker, Andrew C. ; /Washington U., Seattle, Astron. Dept. ; Bickerton, Steven J. ; /Princeton U. ; Blant

关键词: ASTRONOMY;    ASTROPHYSICS;    DISTRIBUTION;    ENGINES;    PLANNING Astrophysics;   

DOI  :  10.2172/952656
RP-ID  :  FERMILAB-FN-0832-CD
PID  :  OSTI ID: 952656
Others  :  Other: arXiv eprint number arXiv:0903.3149
Others  :  TRN: US200915%%108

学科分类：物理（综合）

美国|英语

来源: SciTech Connect

【 摘 要 】

Wide-angle surveys have been an engine for new discoveries throughout the modern history of astronomy, and have been among the most highly cited and scientifically productive observing facilities in recent years. This trend is likely to continue over the next decade, as many of the most important questions in astrophysics are best tackled with massive surveys, often in synergy with each other and in tandem with the more traditional observatories. We argue that these surveys are most productive and have the greatest impact when the data from the surveys are made public in a timely manner. The rise of the 'survey astronomer' is a substantial change in the demographics of our field; one of the most important challenges of the next decade is to find ways to recognize the intellectual contributions of those who work on the infrastructure of surveys (hardware, software, survey planning and operations, and databases/data distribution), and to make career paths to allow them to thrive.