Speaker: Xiaohui Fan (U. of Arizona)
Contact Information: xiaohuidominicfan@gmail.com
Title: An Early JWST View of Quasars at Cosmic Dawn
Abstract: Quasars at cosmic dawn are powerful probes to the formation and growth of early supermassive black holes in the universe, their connections to high-redshift galaxy and structure formation, and the evolution of the intergalactic medium at the epoch of reionization. I will first review the progress in surveys of the most distant quasars, which have discovered hundreds of luminous quasars within the first billion years of cosmic history, with the highest redshift at z~7.6. They are powered by billion solar mass black holes, possible only by a combination of massive early black hole seeds with highly efficient and sustained accretion. I will then present the latest results of studies of early quasars and their environments using JWST. While rapid early black hole growth is accompanied by intense star formation and feedback in their host galaxies, the diverse quasar environment unveiled by these observations suggests a complex interplay between black hole accretion, galaxy assembly, the physics of reionization and the emergence of early large scale structure. I will conclude with a look into the future, as the era of the first supermassive black holes is finally within the horizon of our research efforts.
Visitor's room: Peyton 27C
Wednesday (November 27)
9:30 a.m.:
10:00 a.m:
10:30 a.m.:
11:00 a.m.:
11:30 a.m.:
12:00 p.m.: [suggestion] no meeting - unscheduled buffer time block
12:30 p.m.: Lunch / Wunch
1:00 p.m.: Lunch / Wunch
1:30 p.m.: Jenny's group meeting
2:00 p.m.: Jenny's group meeting
2:30 p.m.: [suggestion] no meeting - unscheduled buffer time block -- Maybe meeting with Jenny right after?
3:00 p.m.:
3:30 p.m.: Minghao Guo
4:00 p.m.: Jiayi Sun (110A)
4:30 pm.:
5:00 pm.:
Wednesday (27 November 2024)
Faculty Host: Michael Strauss
Postdoc Host: Jiayi Sun
Nick Loudas
Hanpu Liu
Miguel Montalvo
Jiaxuan Li
Minghao Guo
Speaker
STUDENTS HAVE PRIORITY.
PLEASE NO MORE THAN 8 PEOPLE (it is more difficult to properly interact with the speaker in larger groups).