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From TORTORA to MegaTORTORA—Results and Prospects of Search for Fast Optical Transients

机译:从TORTORA到MegaTORTORA —快速光学瞬态搜索的结果和前景

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摘要

To study short stochastic optical flares of different objects (GRBs, SNs, etc.) ofunknown localizations as well as NEOs it is necessary to monitor large regionsof sky with high-time resolution. We developed a system consisting of widefieldcamera with field of view of 400–600 sq.deg. which uses TV-CCD with0.13 s temporal resolution to record and classify optical transients, and a fastrobotic telescope aimed to perform their spectroscopic and photometric investigationjust after detection. Such two-telescope complex, combining wide-fieldcamera TORTORA and robotic telescope REM, operated from May 2006 atLa Silla ESO observatory. Some results of its operation, including first hightime resolution study of optical transient accompanying GRB and discoveryof its fine time structure, are presented. Also, prospects for improving theefficiency of such observations are given, and a project of a next generationwide field monitoring system, the MegaTORTORA, is described.
机译:为了研究未知位置和近地天体的不同物体(GRB,SN等)的短随机光学耀斑,有必要以高分辨率对大范围的天空进行监视。我们开发了一个由广角相机组成的系统,其视野范围为400-600平方米。它使用时间分辨率为0.13的TV-CCD记录和分类光学瞬变,并使用快速自动望远镜在检测后立即进行光谱和光度学研究。这种由两台望远镜组成的综合体,结合了TORTORA广角相机和REM机器人望远镜,于2006年5月在La Silla ESO天文台投入使用。介绍了其运行的一些结果,包括对GRB伴随的光学瞬变进行的首次高分辨研究以及发现其精细的时间结构。此外,给出了改善这种观测效率的前景,并描述了下一代现场监测系统MegaTORTORA的项目。

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