Difference between revisions of "Star cluster group"
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== bookmarks == | == bookmarks == | ||
Local Group Astrostatistics Conference http://dept.astro.lsa.umich.edu/lgastrostatistics/ | Local Group Astrostatistics Conference http://dept.astro.lsa.umich.edu/lgastrostatistics/ | ||
[[Category:Internal]] | [[Category:Internal]] | ||
Revision as of 08:32, 24 June 2015
Discussions
2015
2015.06.23
Li: 星團 IMF
PADOVA isochrone test
Zhong: M35 Proper Motion
PM+Spatial --> high prob. mem. comp. with LAMOST RV. (need phot info. to support the results)
2015.06.18
Lin: 跟中央大學談的合作事項。
1. PTF 在星團中的變星 -- 饒兆聰，楊庭彰 (造父變星、RR Ly)
2. NGC752 科學文章 -- 陳文屏 (蒸發、潮汐的成員，動力自行成員、金屬豐度)
3. 星團中的 Brown Dwarfs -- 陳文屏
2015.06.08
Lin: 說明用密度找PS1星團，分析距離年齡的方法。
整理出star cluster catalog以及Be star catalog。
Zhong: LAMOST在星團中的觀測還不足。
Li: 學習Chi-square fitting方法。
Star Clusters
in LAMOST
in APGOEE
in Pan-STARRS
in 2MASS
in Kepler
Catalogs
open clusters
globular clusters
variable stars
Star cluster sample from (186) Dias et al. 2002[1] and (320) Kharchenko et al. 2013. [2] with age > 10^9 years and 0 < Dec < 80 deg.
be stars
brown dwarfs
bookmarks
Local Group Astrostatistics Conference http://dept.astro.lsa.umich.edu/lgastrostatistics/