“Seminar Plan”的版本间差异
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无编辑摘要 |
无编辑摘要 |
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! Date !! Speaker !! Title |
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|2019.01.23 || Shen Shiyin || 宇宙学101[[:File:Cosmology101.pdf | pdf]] |
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|2020.01.15 || Shen Shiyin || How to model the spectrum of a galaxy [[:File:Gal_spectrum.pdf | pdf file]] |
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|2020.03.18 || Shen Mengting || Galaxy Morphology and XXXX |
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|2019.04.10 || Fu Jian || L-Galaxies2019 |
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|2020.03.25 || Lu Jiafeng || Dust Attenuation Curve |
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|2019.04.24 || Yuan Zhen || Gaia MW science [http://online.kitp.ucsb.edu/online/gaia19/ Link A] [https://distill.pub/2019/visual-exploration-gaussian-processes/#Multivariate Link B] |
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|2019.05.29 || Li Lu || Algorithms for substructure searching I [[:File:Substructure.pdf | pdf]] [https://pan.cstcloud.cn/s/dgvwMlOiSSs Link] |
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|2019.06.12 || Liu Rongrong || Spectral indices in sps[[:File:spectral indices in sps.pdf | pdf]] |
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|2019.10.23 || Chen Li || Thick Disk vs Thin Disk in Milky Way |
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|2019.10.31 || Hu Guozhen || Metallicity and Kinematics of Galactic Disks with APOGEE and the GAIA |
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|2019.11.06 || Wang Chun (PKU) || The Chemical Evolution of the MW Discs |
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|2019.11.13 || Shan Xingmei || Star Clusters in MW |
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|2019.11.13 || Ju MT & Shen MT || FAST Observation |
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|2019.12.04 || Fu Jian || Dust Modelling in the Galaxy Evolution Model and Chemical Evolution Model |
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|2019.12.11 || Li Lu || Initial Mass Function |
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|2019.12.25 || Pan Cuiyun || Variable Star Sample in GAIA DR2 |
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|2020.01.15 || Shen Shiyin || How to model the spectrum of a galaxy [[:File:Gal_spectrum.pdf | pdf file]] |
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2020年3月25日 (三) 06:51的版本
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 XXXX |
2020.03.25 | Lu Jiafeng | Dust Attenuation Curve |