1941年至1950年张钮哲担任中央研究院天文研究所所长。
From 1941 to 1950 he was head of the astronomy research institute at National Central University.
德国海德尔堡市马普学会天文研究所的天文学家莫里西奥·西斯特纳斯说，这项新研究“很精致”。
The new study "is a nice piece of work," says Mauricio Cisternas, an astronomer at the Max Planck Institute for Astronomy in Heidelberg, Germany.
“这个发现非常令人兴奋，”德国海德堡马克斯·普朗克天文研究所的赖纳·克莱门特这样说，他在这项研究中负责选定作为观测对象的星球。
"This discovery is very exciting," said Rainer Klement of the Max Planck Institute for Astronomy in Heidelberg, Germany, who targetted the stars in the study.
2004年欧洲组织驻南半球天文研究所拍摄的这张照片，是目前已知最早的一张外部行星图。 所谓外部行星，意即太阳系外的行星。
This 2004 photograph made by the European Southern Observatory shows the first known photo of an exoplanet, or a planet beyond our solar system.
美国人每年要用1100亿塑料制品或塑料盖杯，用完丢弃的一次性容器数量被食品包装研究所（FoodPackaging Institute）形容为“天文数字”。
Americans go through 110 billion plastic or plastic-covered cups each year, using and discarding what the Food Packaging Institute describes as "astronomical numbers" of disposable containers.
“我知道这是声名大噪的时刻。”太空望远镜研究所的天文学家说。
"I knew that was the famous time," says the Space Telescope Science Institute astronomer.
说起来容易但做起来难。随着恒星的衰老，其阴暗斑点的数量也随之下降。再加上基于地球的天文学研究所遇到的困难。
That is easier said than done. The number of spots falls as a star ages. Combined with the difficulties of Earth-based astronomy.
通过日本静止气象卫星(GMS)的远距离钟同步实验正在上海天文台(SO)和日本电波研究所(rrl)之间进行。
The clock synchronization experiment via Japanese Geostationary Meteorological Satellite (GMS) is being conducted between Shanghai observatory (SO) and Radio Research Laboratories (RRL).
范登柏希与考夫曼是德国甲庆的马克士蒲朗克天文物理研究所研究员。
FRANK VAN DEN BOSCH and GUINEVERE KAUFFMANN are researchers at the Max Planck Institute for Astrophysics in Garching, Germany.
本论文中描述了两种不同的原子干涉仪方案，分别在浙江大学光学研究所量子光学实验室和巴黎天文台SYRTE实验室实施。
Two schematics of atom interferometers are depicted in this thesis, implemented by Institute of Optics at Zhejiang University and SYRTE at Paris Observatory, respectively.
本论文中描述了两种不同的原子干涉仪方案，分别在浙江大学光学研究所量子光学实验室和巴黎天文台SYRTE实验室实施。
Two schematics of atom interferometers are depicted in this thesis, implemented by Institute of Optics at Zhejiang University and SYRTE at Paris Observatory, respectively.
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