RESULTS FROM THE LSST SITE MONITORING

被引:0
|
作者
Els, S. G. [1 ]
Sebag, J. [2 ]
机构
[1] TMT Observ Corp, Pasadena, CA 91125 USA
[2] Natl Opt Astron Observ, Tucson, AZ 85719 USA
基金
加拿大自然科学与工程研究理事会; 美国国家科学基金会; 加拿大创新基金会;
关键词
atmospheric effects; instrumentation; site testing; telescopes; TURBULENCE;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Large Synoptic Survey Telescope (LSST) is an 8.4 m telescope which will be dedicated to conduct an all-sky survey in several wavelength bands. In 2006, the El Perion summit on the Cerro Pachon mountain ridge was selected to become the site hosting the LSST telescope. Since 2003 meteorological data have been collected on Penon and since 2006 seeing measurements have also been obtained. Also, in late 2009 a campaign was started to compare the LSST DIMM monitor to the one used by the Thirty Meter Telescope (TMT) site testing project. Here we report on the overall results on meteorological conditions at Perion, and in particular on the optical turbulence conditions. From the LSST-TMT seeing monitor comparison it will be shown that -again- the site monitoring telescope is impacting on the measured overall seeing. The Penon results are also compared with measurements from Cerro Tololo and Cerro Pachon. It was found that high altitude turbulence does on average not greatly vary between those sites.
引用
收藏
页码:79 / +
页数:2
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