Strong MgII and FeII systems at high-z and their possible associated galaxies

We can obtain accurate measurements of gas by quasar absorption systems. How to determine these gas association with related galaxies is the central question we need to solve. I will discuss strong MgII and FeII absorbers population at high-z and how do we study the gas-galaxy relation by the collaboration of big telescopes. 

Discussion Leader: 
Siwei Zou
Place: 
KIAA-PKU
Time: 
Tuesday, May 28, 2019 - 12:00pm