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spectra obtained between 2019.10.23 and 2019.12.31, including 165,997 low resolution spectra, 1,095,21 ...
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为推动我国行星科学和行星探测领域的机构、科学家和技术专家的广泛交流,展示最新科研成果,开发科研新思路,探索未来行星科学一级学科建设道路,促进我国行星科学人才的培养,中国地球物理学会行星物理专业委员会定于2021年6月18日至21 ...
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The workshop will take place online from June 21 to 25, 2021, and consists of pre-recorded overview talks ...| The workshop will take place online from June 21 to 25, 2021, and consists of pre-recorded overview ...
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Ultra-low frequency radio astronomy (1-30 MHz), theory and proposed observations 21-cm cosmology ( ...and industry | Ultra-low frequency radio astronomy (1-30 MHz), theory and proposed observations 21 ...
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为了促进21cm实验的进展,我们正在组织一个21cm宇宙学研讨会,计划于2023年7月16日至22日在中国辽宁省沈阳市举行。该研讨会的重点是分享21cm实验的最新进展和挑战,包括EoR和post-EoR,以帮助该领域充分发挥其潜力。cylinder array Cross-correlation Sciences FRB | To promote progress in the practice of 21 ...cm experiments, we are organizing a community workshop on 21 cm cosmology, which is scheduled to be ...The workshop focuses on sharing recent progress and challenges from all the major 21 cm experiments efforts ...
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Atlas of remote sensing images of Jilin-1 of world-famous observatories comprises 21 high resolution ...
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全球著名天文台吉林一号遥感影像图集包括了21幅由吉林一号卫星对地观测所拍摄的世界著名天文台的高清遥感图片。
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共释放低分辨率光谱数共计594,239条,其中包括568,465条恒星、21,811条星系、3,963条类星体光谱。还包括409,880 颗AFGK恒星光谱参数星表。
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LAMOST第十次巡天数据发布第〇版低分辨率数据包含了2021年9月1日到2022年6月30日之间获取的低分辨率观测的390个天区中的光谱594,239条,其中包括568,465条恒星、21,811条星系 ...
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2022.06.30, including 594,239 low resolution spectra observed on 390 plates, there are 568,465 stellar、21,811 ...
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between 2022.04.01 and 2022.06.30, including 594,239 observed on 390 plates, there are 568,465 stellar、21,811 ...
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About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21 degree Mx−1, and about 66% of “Type II ...” confined events have ΨHFED/ΦAR≥1.0×10−21 degree Mx−1.
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About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21 degree Mx−1, and about 66% of “Type II ...” confined events have ΨHFED/ΦAR≥1.0×10−21 degree Mx−1.
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这个数据集包含21个文件。除了说明文档README以外的文件均以压缩包的形式上传(其中较大的文件被拆分成了多个压缩包)。用户需下载对应压缩包并进行解压以获得原始文件。
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About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21 degree Mx−1, and about 66% of “Type II ...” confined events have ΨHFED/ΦAR≥1.0×10−21 degree Mx−1.
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About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21 degree Mx−1, and about 66% of “Type II ...” confined events have ΨHFED/ΦAR≥1.0×10−21 degree Mx−1.
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This dataset contains 21 files.
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velocities, and information on astrophysical parameters and variability, for sources brighter than magnitude 21 ...