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4月28日学术报告

来源： 发布时间：2014-04-25【字体：大 中 小】

　　题目："The KECK DEIMOS Spectrograph", “The TMT MOBIE Spectrograph” 

　　姓名：Sandra Faber, Matt Radovan 

　　单位：Thirty Meter Telescope (TMT) Project 

　　时间：2014年4月28日（周一）上午10：00 

　　地点：溢智厅 

　　  

　　报告人简介： 

　　Sandra Faber  

　　Sandra Faber is University Professor at the University of California, Santa Cruz, and a staff member of the UCO/Lick Observatory. She is an observational astronomer with primary research interests in cosmology and galaxy formation. Some of her major discoveries include the first structural scaling law for galaxies (called the Faber-­‐Jackson relation), large-­‐scale flow perturbations in the expansion of the Universe caused by superclusters of galaxies, and ubiquitous black holes at the centers of galaxies. She established the scientific case for the twin Keck 10 m telescopes, which inspired a subsequent wave of giant optical telescope building all over the world. From 1994-­‐2005 she was Principal Investigator of the DEIMOS spectrograph, a large optical multi-­‐object spectrograph for the Keck 2 telescope that is the most powerful instrument of its kind in the world. She and colleagues used DEIMOS to conduct the DEEP redshift survey of the distant Universe, which collected spectra of 50,000 distant galaxies and exploited the immense power of Keck to see and study galaxy formation 10 billion years back in time. She now leads the CANDELS project, the largest project in the history of the Hubble Space Telescope, to extend our view of galaxy formation back nearly to the Big Bang. She has co-­‐authored nearly 250 scientific papers, and her work has been cited over 37,000 times. 

　　Matt Radovan 

　　TMT MOBIE group leader

　　  

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