|
Time |
Presenter |
Title |
|
08:30:00 AM |
|
Breakfast |
|
09:00:00 AM |
Andrew Benson |
Welcome |
|
09:05:00 AM |
Andrew Wetzel |
Orbital Histories and Star-Formation Quenching Timescales of Dwarf Galaxies of the Local Group |
|
09:20:00 AM |
Andy Monson |
The Carnegie RR Lyrae Program and a 12-inch telescope |
|
09:35:00 AM |
Chris Burns |
Building a Better SNIa Distance Ladder |
|
09:50:00 AM |
Cristina Catalán-Torrecilla |
Panchromatic view of Star Formation Rate tracers in the Local Universe with UV, optical and IR data |
|
10:05:00 AM |
Dan Kelson |
Totally Derivative |
|
10:20:00 AM |
Shannon Patel |
The Stellar Content of X-ray Groups to z~1 with CSI |
|
10:35:00 AM |
|
Coffee |
|
10:55:00 AM |
Guillermo Blanc |
The IZI way of measuring the Mass-Metallicity Relation |
|
11:10:00 AM |
Gwen Rudie |
The CGM and ISM of High-z Galaxies |
|
11:25:00 AM |
Janet Colucci |
Chemical Abundances in Extragalactic Globular Clusters |
|
11:40:00 AM |
Jeff Rich |
Wide Field Integrated Spectroscopy with PrISM |
|
11:55:00 AM |
Tony Piro |
Tidal Interactions in White Dwarf Binaries |
|
12:10:00 PM |
Johana Teske |
Using Binary Host Star Abundances to Gauge the Influence of Planet Formation |
|
12:25:00 PM |
|
Lunch |
|
01:30:00 PM |
Juna Kollmeier |
??? |
|
01:45:00 PM |
Louis Abramson |
Understanding Diversity in Galaxy Star Formation Histories |
|
02:00:00 PM |
Andrew MacFadyen |
Binary Black Hole Accretion |
|
02:15:00 PM |
Roozbeh Davari |
The limits of measuring the structural properties of bulge and disk of local and high-z massive galaxies |
|
02:30:00 PM |
Drew Newman |
Closing the Lens Gap: The Dark Matter Profile at the Group Scale |
|
02:45:00 PM |
Soung-Chul Yang |
Properties of the Nearby Galaxies As Revealed by RR Lyrae Stars |
|
03:00:00 PM |
Stephanie Tonnesen |
??? |
|
03:15:00 PM |
|
Coffee |
|
03:35:00 PM |
Jennifer van Saders |
Stellar Rotation as a Tool: Where it Works, Where it Doesn't, and How to Tell the Difference |
|
03:50:00 PM |
Vicky Scowcroft |
Mapping the SMC with Cepheids -- What the S should really stand for… |
|
04:05:00 PM |
Yicheng Guo |
The formation and evolution of clumpy galaxies from z=3 to z=0.5 |
|
04:20:00 PM |
Yu Lu |
What governs the baryon mass budget of galaxies, inflow or outflow? |
|
04:35:00 PM |
Yue Shen |
The (non)evolution of the M-sigma relation to z~1 |
|
05:00:00 PM |
|
Friday social |