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ChiVOLabs: Cloud service that offers interactive environment for reprocessing astronomical data

机译:ChiVOLabs:云服务,提供用于重新处理天文数据的交互式环境

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The advancement of technology in telescopes and observation instruments has allowed more and more data to be available with higher resolution and quality, but the way to obtain this data is the same, astronomers are conditioned to obtain observation time. Once the data is public in most cases fall into disuse and except with initiatives such as the virtual observatory that seeks to offer this data over standards and protocols for storage and access, the data will not used again. Our proposal seeks to recover these large volumes of observations already made and offer them as a cloud service from a High Performance Computing (HPC) environment to be reprocessed by the scientific community with the aim of generating new science from them. This is why the Chilean Virtual Observatory (ChiVO) have created ChiVOLabs. a system with a microservice architecture on Docker that allow us. based on searches in our virtual observatory, to offer the possibility of reprocessing ALMA data through a Jupyter Notebook interface. The process starts using the IVOA protocol: Simple Cone Search (SCS) to find the astronomical data and then to select the option to reprocess them. The architecture creates a Docker environment with the entire analysis stack of ChiVO and Python in our datacenter. Furthermore, it transforms the reduction script used to generate the original product in a jupyter notebook automatically connected to our CASA (Common Astronomy Software Applications) cluster (Pipeline of reduction of ALMA). Finally, we search in our datalake raw ALMA data, known as ASDM. from which is generated the selected product and are created a link to these raw in the container. With this we offer to the scientific community the possibility of reprocessing these data according to their scientific interests and generating new data products that can finally be downloaded or continue to be working with our libraries using the full computing power of our datacenter.
机译:望远镜和观测仪器技术的进步使得越来越多的数据能够以更高的分辨率和更高的质量获得,但是获取这些数据的方式是相同的,天文学家需要获得观测时间。一旦数据在大多数情况下是公开的,并且除了诸如虚拟天文台之类的举措之外,这些举措都试图通过用于存储和访问的标准和协议来提供此数据,则这些数据将不再被使用。我们的建议旨在恢复已经做出的大量观测结果,并从高性能计算(HPC)环境中将其作为云服务提供,由科学界对其进行重新处理,以期从中产生新的科学。这就是智利虚拟天文台(ChiVO)创建ChiVOLabs的原因。一个在Docker上具有微服务架构的系统,使我们可以使用。根据我们虚拟天文台中的搜索结果,可以通过Jupyter Notebook界面重新处理ALMA数据。该过程开始使用IVOA协议:简单锥体搜索(SCS)查找天文数据,然后选择对它们进行重新处理的选项。该架构使用数据中心中的ChiVO和Python的整个分析堆栈创建了一个Docker环境。此外,它会在自动连接到我们的CASA(通用天文软件应用程序)集群(ALMA简化流程)的jupyter笔记本中转换用于生成原始产品的简化脚本。最后,我们在数据湖中搜索原始的ALMA数据,称为ASDM。从中生成选定的产品,并在容器中创建指向这些原始物料的链接。借此,我们为科学界提供了根据其科学兴趣重新处理这些数据并生成新的数据产品的可能性,这些产品最终可以下载或继续使用我们的数据中心的全部计算功能与我们的图书馆合作。

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