Talks

	A	B	C	E	F	G	H
1	Presenter	Institution	Title
2	Tuesday (2/21)
3	Tuesday Morning (9:00 AM - 12:30 PM) Session chair: Hsiao-Wen Chen
4	Session 1- What is the multiphase structure of the CGM, and how can we best constrain it observationally?
5	Peng Oh	UC Santa Barbara	A Theoretical Framework for the Multiphase Structure of the CGM
6	Todd Tripp	University of Massachusetts	Turbulent Literature Mixings (TLMs): Steps Toward Observationally Testing a Theoretical Framework for the Multiphase Circumgalactic Medium
7	Zach Hafen	The University of California Irvine	Results from the Halo21 CGM Absorption-System Modeling Challenge
8	Sameer	University of Notre Dame	Observing Multiphase CGM through the lens of a Forward Modeling Bayesian Approach
9
10	Jane Charlton	Penn State	Observational Evidence for the Circumgalactic Mist
11	Ryan Farber	Max Planck Institute for Astrophysics	Shattering, Splattering, or Splintering? Towards a Universal Formation Mechanism for a Foggy Molecular CGM
12	Zhijie Qu	The University of Chicago	On the thermodynamic properties of the cool CGM at z <~ 1
13	Deborah Lokhorst	NRC Herzberg Astronomy & Astrophysics Research Centre	Extensive ionized gas in the M81 group of galaxies revealed by the pathfinder Dragonfly Spectral Line Mapper
14	Benjamin Darwin Oppenheimer	University of Colorado, Boulder	Simulations of the multi-wavelength CGM
15	Fakhri Zahedy	Carnegie Observatories	Spatially Resolving the CGM of Massive Galaxies: the Role of Galaxy Environment
16
17	Tuesday Afternoon (2:00 PM - 5:25 PM) Session chair: Brian O'Shea
18	Lighting Talks Round 1
19	Ahmed Shaban	North Carolina State University	Spatially Resolved Galactic Outflow at z ~ 2 Using Gravitational Lensing
20	Jake Bennett	CfA, Harvard University	The impact of the first supermassive black holes on the early CGM
21	Jeremy Meinke	ASU	Analyzing the CGM of z~1 Quiescent Galaxies via the Thermal Sunyaev-Zel'dovich Effect
22	Skylar Grayson	ASU	Characterizing AGN Feedback Processes Using SIMBA
23	Discussion
24	Session 2 - How turbulent is the CGM, how is this connected to the kinematics of CGM cold-clouds, and how does this depend on galaxy mass and environment?
25	Gwen Rudie	Carnegie	Observational constraints on CGM turbulence and the kinematics of cold-clouds
26	Benjamin Wibking	Michigan State University	Accelerating Cold Clouds with Both Hot Winds and Radiation
27	Ann-Christine Vossberg	UC Santa Barbara	Using AMR to resolve the cooling length
28	Lighting Talks Round 2
29	Antonia Fernández-Figueroa	Swinburne University of Technology	The Circumgalactic medium of galaxy pairs
30	Kelly Sanderson	New Mexico State University	Mapping the Morphology and Kinematics of a Lya-selected Nebula at z=3.15 with MUSE
31	Bart Wakker	University of Wisconsin-Madison	The structure and physical properties of the Local Cosmic Web
32	Mandy Chen	The University of Chicago	Spatially-resolved CGM dynamics in both non-active and active halos
33
34	Rajsekhar Mohapatra	Princeton University	Cooling vs buoyancy vs turbulence: when do galaxy halos become thermally unstable?
35	Nicole Melso	The University of Arizona	A New Tentacle for the Squid Galaxy: Very Extended Ionized Gas around NGC 1068
36	Christopher Churchill	New Mexico State University	Will Deep Learning of Cosmological Simulations Applied to Absorption Lines Unlock the Kinematic Multiphase Structure of the CGM?
37	Rajeshwari Dutta	University of Milano-Bicocca	Probing gas flows around galaxies using large IFU surveys
38	Discussion
39
40	Wednesday (2/22)
41	Wednesday Morning (9:00 AM - 12:30 PM) Session chair: Molly Peeples
42	Session 3 - What can we learn from the CGM of the Milky Way and nearby galaxies, and how do these differ from populations at higher redshifts?
43	Andy Fox	STScI	Observations of the Fermi bubble, MW HVCs & MS
44	Yong Zheng	Rensselaer Polytechnic Institute	The CGM of the Milky Way and other very nearby galaxies
45	David M. French	STScI	The Local CGM: A Deep Survey of Galactic HI
46	Varsha Kulkarni	University of South Carolina	The Galaxy-CGM Connection at Low Redshifts
47	Brian O'Shea	Michigan State University	Examining self-regulation of star formation with idealized simulations of Milky Way-like galaxies
48
49	Rongmon Bordoloi	North Carolina State University	Spatially resolving circumgalactic gas using gravitational lensing
50	Kirill Tchernyshyov	University of Washington	The CGM2 Survey: Quenching and the Transformation of the Circumgalactic Medium
51	Lighting Talks Round 3
52	Benjamin Weiner	MMT/Steward	Satellites of Milky Way analog galaxies and their properties, from the SAGA survey
53	Pengfei Li	University of Utah	Understanding the Circumgalactic Medium by Emulating Extended Lyman Alpha Halos
54	Ramona Augustin	STScI	The small-scale structure of the circumgalactic medium: combining state-of-the-art IFU observations with high resolution simulations
55	Zhihui Li	Caltech	Understanding the CGM of High-z Galaxies with Spatially-Resolved Lyα Radiative Transfer Modeling
56	Discussion
57
58	Session 4 - How does the CGM deviate from equilibrium assumptions- hydrostatic (for hot gas), ionization (for UV species), thermal (for cool gas), pressure (hot/cool)?
59	Cassi Lochhaas	STScI	How well do hydrostatic, ionization, thermal, and pressure equilibrium characterize the CGM?	Theory	F	Postdoc	Postdoc
60	Yakov Faerman	University of Washington	Modeling the Cool Circumgalactic Medium
61
62	Wednesday Afternoon (2:00 PM - 5:10 PM) Session chair: Joop Schaye
63	Tim Heckman	JHU	Assessment of the Mass-Dependent Importance of Feedback on the CGM from AGN vs. Stars
64	Yuval Birnboim	Hebrew University of Jerusalem	Global structures and internal processes of galactic halos
65	Chris Carr	Columbia University	Regulating Star Formation with a Hot Circumgalactic Medium
66	Mansi Padave	ASU	Connecting the CGM to Stellar Disk Growth in Nearby Galaxies
67	Joel N Bregman	University of Michigan	Hot Halo Gas is Revealed by Sunyaev-Zeldovich Observations
68	Lighting Talks Round 4
69	Anjali Ramesh	ASU	Investigating the Ionization State of Low-z QSO Absorption Line Systems
70	Benjamin Rosenwasser	University of Toledo	Classification of the Lyman α forest and the origin of OVI
71	Clayton Strawn	UC Santa Cruz	The PI-CI threshold, and what it can tell us about the CGM
72	Itai Bromberg	Hebrew University in Jerusalem Israel	Metal absorption surrounding galaxies: Disentangling the CGM from the IGM
73	Discussion
74
75	Session 5 - How are gas and angular momentum accreted from the CGM onto galaxies? How important is rotational support in the CGM relative to turbulent support?
76	Crystal Martin	UC Santa Barbara	Observations and Simulations of MgII co-rotation signal
77	Stephanie Ho	New Mexico State University	Kinematics of the Multiphase Circumgalactic Gas Flow
78	Jonathan Stern	Tel Aviv University	The structure of hot, rotating CGM and how they feed disk galaxies
79	Daniel DeFelippis	CEA Paris-Saclay	CGM Angular Momentum Evolution on Short Timescales in an IllustrisTNG Subbox
80
81	Thursday (2/23)
82	Thursday Morning (9:00 AM - 12:25 PM) Session chair: Benjamin Oppenheimer
83	Sanchayeeta Borthakur / Evan Scannapieco	ASU	Logistics
84	Hasti Nateghi	Swinburne University of Technology	Tracking gas accretion in the CGM and IGM of galaxies
85	Claude-Andre Faucher-Giguere	Northwestern University	The interplay between the physics of the circumgalactic medium and galaxy evolution in FIRE
86	Lighting Talks Round 5
87	Alejandro Jorge Olvera	ASU	Indirect Evidence of Low Metallicity Gas Accretion from the CGM of NGC 99
88	Claude-Andre Faucher-Giguere	University of Minnesota	The Imprint of Galactic Inflows on Spectral Lines
89	Patrick Kamieneski	ASU	Using gravitational lensing to resolve massive rotating molecular disks around dusty starbursts at Cosmic Noon
90	Discussion
91	Session 6 - How do metals cycle in and out of galaxies, and how are they distributed in the CGM? How well mixed are metals in the CGM?
92	Dylan Nelson	Heidelberg University	Metal accretion, recycling, and mixing in the CGM
93	Erin Boettcher	University of Maryland, College Park and NASA Goddard Space Flight Center	Illuminating the Disk-Halo Connection Using UV Reflection Nebulae
94	Coffee Break
95	Chris Howk	University of Notre Dame	Observational constraints on metals cycling through the CGM
96	Harley Katz	Oxford University	How density and temperature inhomogeneities and non-equilibrium effects impact inferences of outflow rates
97	Hsiao-Wen Chen	The University of Chicago	Resolving the density and elemental abundances of the CGM
98	Farhan Hasan	New Mexico State University	The connection between galaxy quenching and cosmic web structures across cosmic time
99	Ayan Acharyya	Johns Hopkins University	Metallicity gradient evolution in FOGGIE galaxies as a diagnostic for metal transport
100	Lunch