Difference between revisions of "2013/12/4"
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* 沈世银[[EG sources in LAMOST DR1]] | * 沈世银 [[EG sources in LAMOST DR1]] | ||
* 钟靖 [[LAMOST光谱的IDL可视化程序]] | * 钟靖 [[LAMOST光谱的IDL可视化程序]] | ||
* 甘建铃LAMOST的球状星团的金属丰度的测量问题 | |||
:*可以利用[http://people.ucsc.edu/~conroy/FSPS.html FSPS]的code | |||
* 李静 M巨星在WISE里面的颜色 | |||
:*WISE的W1-W4能很好的区分巨星和矮星 | |||
* 常瑞香: [http://202.127.29.128/data/group_discussion/star_counts_du.ppt 银河系结构模型, Du et al. 2006] | * 常瑞香: [http://202.127.29.128/data/group_discussion/star_counts_du.ppt 银河系结构模型, Du et al. 2006] | ||
Latest revision as of 06:15, 13 December 2013
- 沈世银 EG sources in LAMOST DR1
- 钟靖 LAMOST光谱的IDL可视化程序
- 甘建铃LAMOST的球状星团的金属丰度的测量问题
- 可以利用FSPS的code
- 李静 M巨星在WISE里面的颜色
- WISE的W1-W4能很好的区分巨星和矮星