斯巴鲁Hyper Suprime-Cam战略计划的首次数据发布
First Data Release of the Hyper Suprime-Cam Subaru Strategic Program
摘要:
Hyper Suprime-Cam Subaru战略计划(HSC-SSP)是一项三层成像调查,旨在解决当今天文学中一些最突出的问题,包括暗物质和暗能量的性质。该调查已获得斯巴鲁望远镜300个夜晚的观测时间,并于2014年3月开始。本文介绍了HSC-SSP的首次公开数据发布。此版本包括前1.7年观测(61.5夜)的数据,宽,深和超深层分别覆盖约108,26和4平方度,深度分别为i~26.4,~26.5和~27.0等(点源为5 sigma)。所有的层都在五个宽带(灰色)中观察到,并且深层和超深层也在窄带中观察到。我们在Wide层的i波段实现了令人印象深刻的0.6 arcsec图像质量。我们表明,我们实现了1- 2%的PSF测光(rms)内部和外部(对泛星1),和~10质量和40质量的内部和外部天体测量精度,分别。通过专门的用户界面和数据库服务器向社区提供校准图像和目录。除了管道产品,我们还提供增值产品,如光度红移和一系列公共光谱红移。所有数据的详细描述都可以在网上找到。数据发布网站为https://hsc-release.mtk.nao.ac.jp/。
英文摘要:
The Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) is a three-layered imaging survey aimed at addressing some of the most outstanding questions in astronomy today, including the nature of dark matter and dark energy. The survey has been awarded 300 nights of observing time at the Subaru Telescope and it started in March 2014. This paper presents the first public data release of HSC-SSP. This release includes data taken in the first 1.7 years of observations (61.5 nights) and each of the Wide, Deep, and UltraDeep layers covers about 108, 26, and 4 square degrees down to depths of i~26.4, ~26.5, and ~27.0 mag, respectively (5sigma for point sources). All the layers are observed in five broad bands (grizy), and the Deep and UltraDeep layers are observed in narrow bands as well. We achieve an impressive image quality of 0.6 arcsec in the i-band in the Wide layer. We show that we achieve 1-2 per cent PSF photometry (rms) both internally and externally (against Pan-STARRS1), and ~10 mas and 40 mas internal and external astrometric accuracy, respectively. Both the calibrated images and catalogs are made available to the community through dedicated user interfaces and database servers. In addition to the pipeline products, we also provide value-added products such as photometric redshifts and a collection of public spectroscopic redshifts. Detailed descriptions of all the data can be found online. The data release website is https://hsc-release.mtk.nao.ac.jp/.
机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。