注册网址如下:http://119.29.84.106:8000/register | ...
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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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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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has been completed at the end of April 2021, covering a total of 2,400 square degrees 0°≤ l≤ 240°,|b| ...group, it was decided to continue the second phase of the MWISP survey and extend the survey area to |b| ...
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一期巡天历时10年,已经于2021年4月底结束,共完成0°≤ l≤ 240°,|b|≤ 5°范围共2400平方度的探测覆盖,建立了毫米波射电天文数据库。
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has been completed at the end of April 2021, covering a total of 2,400 square degrees 0°≤ l≤ 240°,|b| ...group, it was decided to continue the second phase of the MWISP survey and extend the survey area to |b| ...
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一期巡天历时10年,已经于2021年4月底结束,共完成0°≤ l≤ 240°,|b|≤ 5°范围共2400平方度的探测覆盖,建立了毫米波射电天文数据库。
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remove stellar contaminants, we obtain a reliable GPQ candidate catalog with 160,946 sources located at |b| ...
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我们应用迁移学习方法和XGBoost算法对Pan-STARRS1 (PS1) 和AllWISE测光星表进行银道面背景类星体选源,并使用Gaia自行判据排除恒星污染源,最终得到位于 |b|≤20∘内、包含 ...
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IERS Bulletin B provides current information on the Earth's orientation in the IERS Reference System.
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因为保密等原因,不能提供更多获得数据的仪器等方面的描述,数据更新时间为不定时更新,此数据为地球自转B公报主要提供了有关地球方向的最新信息,包括世界时间,地球极坐标和天极偏移等数据。
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Existing selection methods for quasars developed using high Galactic latitude (high-b) data cannot be ...applied to the Galactic plane directly because the photometric data obtained from high-b regions and ...We obtain a reliable GPQ candidate catalog with 160,946 sources located at ∣b∣ ≤ 20° in the PS1-AllWISE ...
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Existing selection methods for quasars developed using high Galactic latitude (high-b) data cannot be ...applied to the Galactic plane directly because the photometric data obtained from high-b regions and ...We obtain a reliable GPQ candidate catalog with 160,946 sources located at ∣b∣ ≤ 20° in the PS1-AllWISE ...
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area of over 6000 deg<SUP>2</SUP> for Galactic longitude 140 < l < 240 deg and latitude -60 < b ...
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area of over 6000 deg<SUP>2</SUP> for Galactic longitude 140 < l < 240 deg and latitude -60 < b ...
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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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the forbidden emission lines of [Fe II] and [O I], in which J051425.20+411310.7 is a newly discovered B[ ...