论文标题

Murchison广场阵列的校准数据库全天虚拟天文台

Calibration database for the Murchison Widefield Array All-Sky Virtual Observatory

论文作者

Sokolowski, M., Jordan, C. H., Sleap, G., Williams, A., Wayth, R. B., Walker, M., Pallot, D., Offringa, A., Hurley-Walker, N., Franzen, T. M. O., Johnston-Hollitt, M., Kaplan, D. L., Kenney, D., Tingay, S. J.

论文摘要

我们使用新开发的校准解决方案的新开发的PostgreSQL数据库,为Murchison广场全天文台(MWA ASVO)提供了一个校准组件。自2013年就职典礼以来,MWA记录了Pawsey SuperComputing Center存档的34 pb pb。根据MWA数据访问政策,收集十八个月后,数据将公开获得。因此,大多数档案数据现在可向公众使用。 2017年通过MWA ASVO接口提供了对公共数据的访问,该界面允许全球研究人员以标准射电天文学数据格式(CASA测量集或UV FITS FILES)下载MWA未校准的数据。 MWA ASVO校准功能的添加为研究人员开辟了一条新的,强大的途径,而没有详细了解MWA望远镜和数据处理,以下载校准的可见性数据并使用标准的射电媒体软件包创建图像。为了用校准解决方案填充数据库,我们开发了完全自动化的管道。一条近实时的管道一旦收集到新的校准观测,并将校准解决方案上传到数据库,从而可以监视望远镜的干涉性能。基于此数据库,我们对长期间隔内MWA校准解决方案的稳定性进行了分析。

We present a calibration component for the Murchison Widefield Array All-Sky Virtual Observatory (MWA ASVO) utilising a newly developed PostgreSQL database of calibration solutions. Since its inauguration in 2013, the MWA has recorded over thirty-four petabytes of data archived at the Pawsey Supercomputing Centre. According to the MWA Data Access policy, data become publicly available eighteen months after collection. Therefore, most of the archival data are now available to the public. Access to public data was provided in 2017 via the MWA ASVO interface, which allowed researchers worldwide to download MWA uncalibrated data in standard radio astronomy data formats (CASA measurement sets or UV FITS files). The addition of the MWA ASVO calibration feature opens a new, powerful avenue for researchers without a detailed knowledge of the MWA telescope and data processing to download calibrated visibility data and create images using standard radio-astronomy software packages. In order to populate the database with calibration solutions from the last six years we developed fully automated pipelines. A near-real-time pipeline has been used to process new calibration observations as soon as they are collected and upload calibration solutions to the database, which enables monitoring of the interferometric performance of the telescope. Based on this database we present an analysis of the stability of the MWA calibration solutions over long time intervals.

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