“Seminar Plan”的版本间差异
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|2020.09.09 || Shen Shiyin || What determines metallicity of galaxies? [http://cluster.shao.ac.cn/~shen/myfile/metallicity.pdf] |
|2020.09.09 || Shen Shiyin || What determines metallicity of galaxies? [http://cluster.shao.ac.cn/~shen/myfile/metallicity.pdf] |
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|2020.09.16 || Liu Rongrong || Fitting the integrated spectral energy distributions of galaxies |
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|2020.01.08 || Liu Rongrong || Prospector and Prior in the non-parametric SFH |
|2020.01.08 || Liu Rongrong || Prospector and Prior in the non-parametric SFH |
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|2020.01.15 || Shen Shiyin || How to model the spectrum of a galaxy [[:File:Gal_spectrum.pdf | pdf file]] |
|2020.01.15 || Shen Shiyin || How to model the spectrum of a galaxy [[:File:Gal_spectrum.pdf | pdf file]] |
2020年9月16日 (三) 07:16的版本
腾讯会议ID: 4786244041
2nd semester
Date | Speaker | Title |
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2020.09.09 | Shen Shiyin | What determines metallicity of galaxies? [1] |
2020.09.16 | Liu Rongrong | Fitting the integrated spectral energy distributions of galaxies |
1st semester
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Date | Speaker | Title |
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2020.01.08 | Liu Rongrong | Prospector and Prior in the non-parametric SFH |
2020.01.15 | Shen Shiyin | How to model the spectrum of a galaxy pdf file |
2020.03.18 | Shen Mengting | Galaxy Morphology and Gas Content |
2020.03.25 | Lu Jiafeng | Dust Attenuation Curve |
2020.04.08 | Shen Shiyin | Compact Galaxy Systems in LAMOST |
2020.04.17 | Li Zhaozhou(SJTU) | Mass Profile of the Milky Way |
2020.04.22 | Zhang Shuhui | Star Clusters |
2020.04.29 | Zhang Xi | Open Cluster in LAMOST-MRS |
2020.05.06 | Zhao Donghai | Intro of Cosmology & Dark Matter |
2020.05.13 | Zhang Wenjing | Abundance Gradient of the Milky Way |
2020.05.20 | Zheng Yunliang | Dynamics Properties of Compact Groups |
2020.05.27 | Zhong Jing | Age of Stellars |
2020.06.03 | Zhong Wenxin | Radial Profile of Hot Gas |
2020.06.10 | Rafael S. de Souza | Catalyzing Interdisciplinarity pdf file |