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The Hyper Suprime-Cam SSP Survey: Overview and survey design

机译：Hyper Suprime-Cam SSP调查：概述和调查设计

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Hyper Suprime-Cam (HSC) is a wide-field imaging camera on the prime focus of the 8.2-m Subaru telescope on the summit of Mauna Kea in Hawaii. A team of scientists from Japan, Taiwan, and Princeton University is using HSC to carry out a 300-night multi-band imaging survey of the high-latitude sky. The survey includes three layers: the Wide layer will cover 1400?deg2 in five broad bands (grizy), with a 5?σ point-source depth of r ≈ 26. The Deep layer covers a total of 26?deg2 in four fields, going roughly a magnitude fainter, while the UltraDeep layer goes almost a magnitude fainter still in two pointings of HSC (a total of 3.5?deg2). Here we describe the instrument, the science goals of the survey, and the survey strategy and data processing. This paper serves as an introduction to a special issue of the Publications of the Astronomical Society of Japan, which includes a large number of technical and scientific papers describing results from the early phases of this survey.
机译：Hyper Suprime-Cam（HSC）是一款宽视场成像相机，位于8.2微米斯巴鲁望远镜的主要焦点上，该望远镜位于夏威夷的莫纳克亚山顶。日本，台湾和普林斯顿大学的一组科学家正在使用HSC对高纬度天空进行300晚的多波段成像调查。该调查包括三层：宽层将在五个宽带（灰带）中覆盖1400？deg2，点源深度为5？σr≈26。深层在四个场中总共覆盖26？deg2，大约在一个微弱的幅度上移动，而UltraDeep层在两个HSC点（总计3.5？deg2）上仍几乎微弱了一个幅度。在这里，我们描述了仪器，调查的科学目标以及调查策略和数据处理。本文是日本天文学会出版物特刊的简介，其中包括大量描述该调查早期结果的技术和科学论文。

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