Wine and Cheese Fall 2023: Difference between revisions
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== William Coulton () == | == William Coulton (Flatiron Institute) == | ||
'''New Views of Galaxy Groups and Clusters with Precision CMB Secondary Measurements'''<br> | '''New Views of Galaxy Groups and Clusters with Precision CMB Secondary Measurements'''<br> | ||
High resolution cosmic microwave background (CMB) experiments provide a view of the Universe both at redshift ~1100, when the primary CMB was produced, and an integrated view of the Universe between then and now, through CMB secondary anisotropies. The CMB secondary anisotropies provide direct access to the integrated mass, electron density, electron pressure and electron temperature. In this talk, I will first present recent maps of CMB secondaries from the Atacama Cosmology Telescope collaboration. I will then show how upcoming experiments will be able to measure new observable signatures of galaxy groups, and how these can be used to inform our understanding of the thermodynamics of these objects. | High resolution cosmic microwave background (CMB) experiments provide a view of the Universe both at redshift ~1100, when the primary CMB was produced, and an integrated view of the Universe between then and now, through CMB secondary anisotropies. The CMB secondary anisotropies provide direct access to the integrated mass, electron density, electron pressure and electron temperature. In this talk, I will first present recent maps of CMB secondaries from the Atacama Cosmology Telescope collaboration. I will then show how upcoming experiments will be able to measure new observable signatures of galaxy groups, and how these can be used to inform our understanding of the thermodynamics of these objects. | ||
Revision as of 17:16, 12 September 2023
This page records the schedule, titles and abstracts of the JHU/STScI CAS Astrophysics Wine & Cheese Series in Fall 2023.
Wine and Cheese sessions with one speaker will have a 50 minute talk with 10 minutes for questions. Sessions with two speakers will have two 25 minute talks, each with 5 minutes for questions. Sessions in the Graduate Student Series will have three 15 minute talks, each with 5 minutes for questions.
Back to W&C Schedule
11 September
Ferah Munshi (George Mason)
Understanding Galaxy Evolution at the Lowest Masses
Low mass galaxies challenge our picture of galaxy formation and are an intriguing laboratory for the study of star formation, feedback and dark matter physics. I will present results from high resolution, cosmological simulations that contain many (isolated) dwarf galaxies [the MARVEL dwarfs] as well as satellite dwarf galaxies [the DC Justice League]. Together, they create the largest collection of high-resolution simulated dwarf galaxies to date and the first flagship suite to resolve ultra-faint dwarf galaxies in multiple environments. This sample spans a wide range of physical (stellar and halo mass), and evolutionary properties (merger history). I will present results and predictions constraining star formation, feedback and dark matter physics soon testable by telescopes like JWST, Rubin's LSST and the Roman Space Telescope. Finally, I will present results about satellite distributions around Milky Way analogs from both zoom-in simulations and from a large sample of analogs drawn from the Romulus 25-Mpc volume simulation. I will discuss the role of environment in addition to satellite quenching times and their mechanisms with an eye toward comparing with observations.
18 September
William Coulton (Flatiron Institute)
New Views of Galaxy Groups and Clusters with Precision CMB Secondary Measurements
High resolution cosmic microwave background (CMB) experiments provide a view of the Universe both at redshift ~1100, when the primary CMB was produced, and an integrated view of the Universe between then and now, through CMB secondary anisotropies. The CMB secondary anisotropies provide direct access to the integrated mass, electron density, electron pressure and electron temperature. In this talk, I will first present recent maps of CMB secondaries from the Atacama Cosmology Telescope collaboration. I will then show how upcoming experiments will be able to measure new observable signatures of galaxy groups, and how these can be used to inform our understanding of the thermodynamics of these objects.
