UChicago-2020: Astrophysics high redshift galaxies and clusters

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Astrophysics of High-Redshift Galaxies and Clusters

Organizers Lindsey Bleem and Anthony Gonzalez
Zoom link https://fnal.zoom.us/j/97954282174?pwd=ajFUcU9yQmFaVnVFMVpRMHFBMlo4Zz09

Logistics

Overview

CMB-S4 will detect high redshift dusty galaxies out to z~9; protoclusters out to z~5 ; and massive galaxy clusters out to z~2. In this session we will discuss how CMB-S4 can shed light on the evolution from high-redshift dusty galaxies to protoclusters to galaxy clusters and highlight the insights and advances that studies of these discrete objects will bring to the field of astrophysics. The session will consist of four 10 minute talks (with 5 minutes for questions) followed by a 30 minute general discussion.


Schedule (times in PDT, UTC-7 hrs)

  • 10:00 - 10:05 Introduction, Logistics
  • 10:05 - 10:20 Claude-André Faucher-Giguère (Northwestern) "Status of simulating massive galaxies and AGN feedback in FIRE (with an eye toward how future observations can constrain the physics)" link
  • 10:20 - 10:35 Justin Spilker (UT Austin) "Dusty Galaxy Astrophysics with CMB-S4" link
  • 10:35 - 10:50 Yi-Kuan Chiang (OSU) "Cosmological Galaxy Cluster Formation" link
  • 10:50 - 11:05 Mike McDonald (MIT) "Astrophysics of High-z Galaxy Clusters in the 2030s" link
  • 11:05 - 11:30 Discussion

Notes