2011-1-21Purple Mountain Observatory Chinese Academy of Sciences紫金山天文台中国科学院学术报告题 目：报告人：XSHD-2011-006Mapping the Milky Ways Dark Matter and Stellar Halo薛香香 博士摘 要：(国家天文台)Through spectroscopy of

DE = keV bins(2-6) keV: 清晰的年调制(6–20) keV: 拟合结果Sm=0 ?2 dof==2??=1 yr and t0= day年调制幅度的能量分布相位t与 2nd June的轻微的不同可以用非热暗物质的贡献(比如 SagDEG stream)来解释E (keV)Sm (cpdkgkeV)Zm (cpdkgkeV)Ym (cpdkgkeV)t

Proportional Light in aDual Phase Xenon ChamberElena Aprilefor the XENON CollaborationPhysics Department and Columbia Astrophysics Laboratory Columbia University New YorkThe XENON CollaborationColum