Illuminating the Circumgalactic Medium Colin Hill, Nick Battaglia, and Matt McQuinn
The next decade of mm-wave observations will transform our understanding of galaxy formation, driven by precisely measuring the thermodynamic properties of ionized gas, using the cosmic microwave background as a "backlight". In this session we will discuss how these observations will probe the CGM gas well into the outskirts of hitherto-unexplored high-redshift, low-mass systems and the synergies with other observables.
Chair/Moderator: Nick Battaglia
Note Taker: Colin Hill
- 10:00am - 10:20am PDT - Hsiao-Wen Chen Absorption line measurements and their implications for the CGM and galaxy formation
- 10:20am - 10:40am PDT - Drummond Fielding Simulations and models for the CGM and their relation to galaxy formation File:CGM CMBS4 LR.pdf
- 10:40am - 11:00am PDT - Stefania Amodeo SZ measurements with existing data sets
- 11:00am - 11:30am PDT - Discussion File:S4 UChic 2020 SZ Questions.pdf