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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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计划中的x射线望远镜hub(热宇宙重子测量器)的任务是测量热气体的性质。为了讨论中心的科学目标，我们组织了一系列研讨会。第一届是2018年在上海举行的。涉及的主要主题: circumgalactic介质 星系际介质 AGN和恒星反馈 热星际介质 AGN 星系团 漫射x射线背景 超新星残骸 任务 | Aims and Scope ...Measuring the properties of hot gas is the task of the planned X-ray telescope HUBS (Hot Universe Baryons ...intergalactic medium AGN and stellar feedback Hot interstellar medium AGN Galaxy clusters The diffuse X-ray ...
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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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对这些热气体的观测是HUBS（http://hubs.phys.tsinghua.edu.cn/en/index.html） X射线空间天文望远镜的主要任务。银河系科学，包括X射线背景、超新星遗迹、恒星与致密天体 5. 高分辨率光谱学 欢迎大家注册参会，尤其鼓励研究生与博士后参会并提交报告。
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主镜面型为抛物面，有效口径1000 mm，设计有效视场1.5°X 1.5°。配备了光学天文测光常用的Johnson、SDSS 和Stromgren滤光片系统，可进行恒星类型、参数、金属丰度等观测。
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type star spectra obtained by LAMOST low resolution survey during October 24th 2011 and June 8th 2019x.
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stellar spectra obtained by LAMOST low resolution survey during October 24th 2011 and June 8th 2019x.
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stellar spectra obtained by LAMOST low resolution survey during October 24th 2011 and June 8th 2019x.
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IERS Bulletin A contains Earth orientation parameters x/y pole, UT1-UTC and their errors at daily intervals ...
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clocks correspond to different types of clocks, among which 35- represents cesium atomic clocks and 4x- ...
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其中，钟的序号不同数字对应了不同的钟的类型，其中35-表示铯原子钟、4x-表示氢原子钟，这两种占据了钟类型的绝大多数，此外还有其他的钟类型。NTSC通过数据字典匹配提取NTSC原子钟速率数据。
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其中，钟的序号不同数字对应了不同的钟的类型，其中35-表示铯原子钟、4x-表示氢原子钟，这两种占据了钟类型的绝大多数，此外还有其他的钟类型。
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Among them, 35- represents cesium atomic clock and 4x- represents hydrogen atomic clock, which occupy ...
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The ESA's X-ray Multi-mirror Mission (XMM-Newton) created a new high-quality version of the XMM-Newton ...the Sloan Digital Sky Survey (SDSS) DR12 photometric data base and the AllWISE data base; we then get X-ray ...sources with information from the X-ray, optical, and/or infrared bands and obtain the XMM-WISE, XMM-SDSS ...For the sample from the X-ray band, a rotation-forest classifier performs the best.Their membership of and membership probabilities for individual X-ray sources are assigned.
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The ESA's X-ray Multi-mirror Mission (XMM-Newton) created a new high-quality version of the XMM-Newton ...the Sloan Digital Sky Survey (SDSS) DR12 photometric data base and the AllWISE data base; we then get X-ray ...sources with information from the X-ray, optical, and/or infrared bands and obtain the XMM-WISE, XMM-SDSS ...For the sample from the X-ray band, a rotation-forest classifier performs the best.Their membership of and membership probabilities for individual X-ray sources are assigned.
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temperature (Teff[K]), surface gravity (Logg), 15 elemental abundances (XH), 1σ uncertainty of parameters (X_err ...
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The ESA's X-ray Multi-mirror Mission (XMM-Newton) created a new high-quality version of the XMM-Newton ...the Sloan Digital Sky Survey (SDSS) DR12 photometric data base and the AllWISE data base; we then get X-ray ...sources with information from the X-ray, optical, and/or infrared bands and obtain the XMM-WISE, XMM-SDSS ...For the sample from the X-ray band, a rotation-forest classifier performs the best.Their membership of and membership probabilities for individual X-ray sources are assigned.