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The MUNI Photometric Archive

机译:Muni Photometric档案

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In the 1990s of the last century, CCD cameras became more reachable. Due to many advantages of CCD cameras, astronomers began using them as the primary detector for photometry of stellar objects. A typical observatory, which operates one telescope at a time, obtained 0.5 TB of raw data during two decades, that means one million about 500 kB-sized files. There are several observatories in the Czech Republic and Slovakia (taking into account all scientific, public as well as private ones). A rough estimate of the total amount of this photometric data is 10 TB, which could be a very interesting source of observational data. Unfortunately, these data are not available online. These data are stored in observatory archives in arbitrary format. Often it is not even possible to find requested data. We have decided to change this state by establishing a common archive of raw photometric data, which would be available online together with tools for searching, listing etc. We already defined the data format, file and directory structure of our archive. We developed sophisticated tools for archive maintenance as well. Our goal is to provide data storage with simple and straightforward access and we are ready to interconnect with the VO right after the IVOA Photometry Data Model will be released.
机译:在上个世纪的1990年代,CCD相机变得更加可达。由于CCD摄像机的许多优点,天文学家开始使用它们作为恒星物体的测光的主要检测器。一次运行一个望远镜的典型天文台,在二十年中获得了0.5 TB的原始数据,这意味着一百万个约500 kB大小的文件。捷克共和国和斯洛伐克有几个观察者(考虑到所有科学,公共和私人)。对该光度数据的总量的粗略估计为10 TB,这可能是一个非常有趣的观察数据来源。不幸的是,这些数据在线不可用。这些数据以任意格式存储在观察台档案中。通常它甚至没有找到所请求的数据。我们决定通过建立原始光度数据的常见存档来改变此状态,该数据将与搜索,清单等的工具一起使用。我们已经定义了我们存档的数据格式,文件和目录结构。我们也开发了复杂的归档维护工具。我们的目标是提供简单且简单的访问的数据存储,并且在释放IVOA测光数据模型之后,我们准备好与VO互连。

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