时间：2020年11月26日下午3:00

地点：行健楼437会议室

题目： 从z=2开始的大质量星系演化（Massive galaxy Evolution since z=2）

报告人：黄家声 研究员（中国科学院南美天文中心首席科学家兼执行主任）

报告摘要：

The most important epoch in galaxy evolution was at z=2~3 where both star formation rate density and AGN activities were in their peak stage.  The star formation happened in most massive galaxies with very intensive burst known as Ultraluminous Infrared Galaxies (ULIRGs). Current galaxy formation theories fail to predict numbers of ULIRGs at this redshifts and also have a hard time to propose a mechanism to quench this burst. In this talk I will discuss the ULIRG population at z~2 and their descendent counterparts, massive red galaxies at z~1. We try to establish their evolution connection using the large samples in wide field, yet deep, surveys in both optical and IR bands.

报告人简介：1981-1988，南京大学, 本科/研究生;
                           1988-1991，中科院北京天文台理论天体物理组；
                           1991-1997，夏威夷大学天文中心，博士; 
                           1997-1999，德国海德堡马普天文研究所，博士后；
                           1999-2015，美国哈佛史密松天体物理中心，研究员; 
                           2012至今，国家天文台研究员，中科院南美天文中心首席科学家/执行主任。