後藤友嗣 - 台湾清华大学

个人简介

學經歷與榮譽 •東京大學物理博士(1999) •國立清華大學物理系助理教授 (2013 - 2017 ) •國立清華大學物理系副教授 (2017 - 迄今)

研究领域

•高红移類星體及再電離 •宇宙恆星形成歷史 •通過集成的薩克斯 - 沃爾夫效果探測暗能量 •後星爆（E+ A）星系的起源 •對星系演化的環境影響

近期论文

查看导师新发文章（温馨提示：请注意重名现象，建议点开原文通过作者单位确认）

•Cross-correlation of WISE Galaxies with the Cosmic Microwave Background, Goto et al. 2012, MNRAS, 422L,77 •Spectroscopy of the spatially extended Lyα emission around a quasar at z= 6.4, Goto et al. 2012, MNRAS, 421L,77 •A Gunn-Peterson test with a QSO at z=6.4, Goto et al. 2011, MNRAS, 415L •Evolution of Infrared Luminosity functions of Galaxies in the AKARI NEP-Deep field: Reveal- ing the cosmic star formation history hidden by dust, Goto et al. 2010, A&A AKARI special issue, 514A •A QSO host galaxy and its Lyα emission at z=6.43, Goto, T. et al. 2009, MNRAS, 400, 843 •266 E+A galaxies selected from the Sloan Digital Sky Survey Data Release 2: the origin of E+A galaxies, Goto, et al. 2005, MNRAS, 357, 937 •Discovery of a new high redshift QSO at z=5.96 with the Subaru telescope, Goto et al. 2006, MNRAS, 371, 769