Wine and Cheese Fall 2024

From caswiki
Revision as of 13:52, 6 September 2024 by Kdkuntz (talk | contribs) (Created page with "{| align="right" | __TOC__ |} This page records the schedule, titles and abstracts of the JHU/STScI CAS Astrophysics Wine & Cheese Series in Fall 2024. 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. <h2>Back to W&C Schedule </h2> =9 September= == John Sol...")
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to navigationJump to search

This page records the schedule, titles and abstracts of the JHU/STScI CAS Astrophysics Wine & Cheese Series in Fall 2024.

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.

Back to W&C Schedule

9 September

John Soltis (JHU)

Direct Estimation of Galaxy Cluster Mass Accretion Rate using Machine Learning
Galaxy cluster mass abundances provide an important cosmological constraint. Mass estimates, however, are biased by galaxy cluster dynamical state. The dynamical state, the intensity of physical disturbance in the galaxy cluster, is a direct result of its mass accretion rate. I will present a machine learning model for directly constraining the mass accretion rate of galaxy clusters from only X-ray and thermal Sunyaev-Zeldovich observations. Furthermore, I will discuss the different machine learning interpretability methods we employ to better understand the model, and the conclusions we draw from them.

Farhad Yusef-Zadeh (Northwestern)

Highlights of the MeerKAT Radio Survey of the Galactic Center
It has been 40 years since the magnetized radio filaments were first reported toward the Galactic center (GC), the first hint of an energetic activity in this region. Since then, a large number of synchrotron emitting filaments has been discovered in this high cosmic-ray pressure environment. In particular, the recent MeerKAT survey, which has been a gold mine in the study of the extreme environment of the GC, has increased the number of filaments by an order of magnitude. In this talk, I will discuss the statistical properties of the GC filaments, the comparison of the intracluster medium (ICM) and GC filaments, models of these enigmatic objects and the association of a milli-second pulsar powering a nonthermal radio filament near the magnetized Snake filament.

16 September