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Catalina Real-Time Transient Survey : ウィキペディア英語版
Catalina Real-time Transient Survey
The Catalina Real-Time Transient Survey is a collaboration using three telescopes looking for optical transients. The same telescopes are used as in the Catalina Sky Survey. They are Mt. Lemmon Survey, Catalina Sky Survey, and Siding Spring Survey. When transients are detected they are alerted on a short time scale so that others can observe the event as well using VOEventNet and SkyAlert. It has detected supernovae, cataclysmic variables, blazars, active galactic nuclei and flares.〔(【引用サイトリンク】title=The CRTS Survey )
==References==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Catalina Real-time Transient Survey」の詳細全文を読む



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