以亚微分分辨率进行全天空毫米波探测的理由

F. D'esert, M. Calvo, Andrea Catalano, S. Leclercq, J. Macı́as-Pérez, F. Mayet, A. Monfardini, L. Perotto, N. Ponthieu
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引用次数: 0

摘要

有几个用毫米波望远镜观测天空的新项目,其中最大的是南半球的西蒙斯天文台和 CMB-S4。NIKA2 合作项目已经掌握了足够的知识,可以为 15 米天线建造大型焦平面 KID 摄像机。这样就能在五年内以亚arcminute 分辨率和毫扬斯基点源灵敏度覆盖整个北半球。我们描述了这样一个项目的主要科学驱动力:SZ 天空、高红移毫米波宇宙以及银河系和附近星系的星际介质。我们还简要说明了主要的困难(科学、组织、技术和资金)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The case for an all-sky millimetre survey at subarcminute resolution
There are several new projects to survey the sky with millimetre eyes, the biggest being Simons Observatory and CMB-S4, in the Southern Hemisphere. The NIKA2 collaboration has acquired sufficient knowledge to build a large focal plane KID camera for a 15 m antenna. This would allow covering the whole Northern Hemisphere in five years at subarcminute resolution and with milliJansky point-source sensitivity. We describe the main scientific drivers for such a project: the SZ sky, the high-redshift millimetre Universe and the interstellar medium in our Galaxy and the nearby galaxies. We also show briefly the main difficulties (scientific, organisational, technical and financial).
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