Difference between revisions of "UChicago-2020: CGM"
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Agenda | Agenda | ||
− | * 10:00am - 10:20am PDT - Hsiao-Wen Chen | + | * 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 | + | * 10:20am - 10:40am PDT - Drummond Fielding ''Simulations and models for the CGM and their relation to galaxy formation'' |
− | * 10:40am - 11:00am PDT - Stefania Amodeo | + | * 10:40am - 11:00am PDT - Stefania Amodeo ''SZ measurements with existing data sets'' |
* 11:00am - 11:30am PDT - Discussion | * 11:00am - 11:30am PDT - Discussion |
Revision as of 14:21, 7 August 2020
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.
Agenda
- 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
- 10:40am - 11:00am PDT - Stefania Amodeo SZ measurements with existing data sets
- 11:00am - 11:30am PDT - Discussion