A photometricity and extinction monitor at the Apache Point Observatory

被引:662
作者
Hogg, DW
Finkbeiner, DP
Schlegel, DJ
Gunn, JE
机构
[1] NYU, Dept Phys, New York, NY 10003 USA
[2] Princeton Univ, Dept Astrophys, Princeton, NJ 08544 USA
[3] Inst Adv Study, Princeton, NJ 08540 USA
[4] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
关键词
astrometry; methods : data analysis; methods : observational; surveys; techniques : image processing; techniques : photometric;
D O I
10.1086/323103
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
An unsupervised software "robot" that automatically and robustly reduces and analyzes CCD observations of photometric standard stars is described. The robot measures extinction coefficients and other photometric parameters in real time and, more carefully, on the next day. It also reduces and analyzes data from an all-sky 10 mum camera to detect clouds; photometric data taken during cloudy periods are automatically rejected. The robot reports its findings to observers and data analysts via the World Wide Web. It can be used to assess photometricity and to build data on site conditions. The robot's automated and uniform site monitoring represents a minimum standard for any observing site with queue scheduling, a public data archive, or likely participation in any future National Virtual Observatory.
引用
收藏
页码:2129 / 2138
页数:10
相关论文
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