注册网址如下:http://119.29.84.106:8000/register | ...
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非常欢迎天文界各位同仁的参与和支持!
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会议网址:http://gra2020.csp.escience.cn,请参会者自行在注册页面进行注册。会议注册截止日期:2021年3月30日。 2.
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本次报告以邀请报告为主,线上参会网址将近期公布。
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Radio-frequency interference environment Solar and planetary science Synergies with other disciplines (e.g ...Radio-frequency interference environment Solar and planetary science Synergies with other disciplines (e.g ...
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会议将重点介绍SKA国际进展、国内SKA已立项方向的进展情况及其它待立项方向的组织和准备情况,会议注册网址: https://docs.qq.com/form/page/DU1B4U0ZjemJOUUtG ...
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天文学是以观测为基础的一门学科,天文观测环境对于天文观测数据质量有着非常重要的影响。随着社会经济发展,天文观测台站受到所在地方城市建设影响也日益显著。
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This catalog is divided into two subsamples, i.e., the primary and secondary parts.
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contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.e.
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contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.e.
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Geostationary Operational Environmental Satellite class M1.0 and larger that occurred during 2010-2019, i.e.
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Geostationary Operational Environmental Satellite class M1.0 and larger that occurred during 2010-2019, i.e.
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investigate the origins of HiVelSCs, we perform orbit integrations and divide them into four types, i.e.
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investigate the origins of HiVelSCs, we perform orbit integrations and divide them into four types, i.e.
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contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.e.
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contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.e.
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Our method is valid for FGK stars with G ≤ 16, [Fe/H] ≥ -2.5, and E(B - V) ≤ 0.5.
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Our method is valid for FGK stars with G ≤ 16, [Fe/H] ≥ -2.5, and E(B - V) ≤ 0.5.
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forbidden emission lines of [Fe II] and [O I], in which J051425.20+411310.7 is a newly discovered B[e] ...
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forbidden emission lines of [Fe II] and [O I], in which J051425.20+411310.7 is a newly discovered B[e] ...