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Thursday, Sept. 13, 2012
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6-8 pm |
Welcome Reception, Calvino Cafe |
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Friday, Sept. 14
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8:45-9:00 |
Welcome - Jewell |
9:00-9:45 |
Physical Properties of the Star-forming ISM in Galaxies Near and Far: Narayanan |
9:45-10:10 |
Connections Between the Milky Way and High-z Galaxies: Evans |
10:10-10:35 |
Hydride Molecules in the ISM of the Nearby and High Redshift Universe: Monje |
10:35-11:05
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Break |
11:05-11:50 |
Observational Clues to the Epoch of Reionization: Wang |
11:50-12:15 |
Measuring the ISM in Hi-z Galaxies: Scoville |
12:15-12:40 |
Observations of Far Infrared Emission Lines at z~4: Gallerani |
12:40-1:40 |
Lunch |
1:40-2:25 |
Dust and Metallicity: Bolatto |
2:25-2:50 |
ALMA Unveils Hi-z Cosmic Microscopes Discovered by the SPT: Vieira |
2:50-3:15
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GISMO Surveys of the High-Redshift Universe: Staguhn |
3:15-3:45 |
Break |
3:45-4:10 |
ULIRG F00183 Watching the Birth of a Quasar: Norris |
4:10-4:35 |
The Highest Redshift Submm Galaxy: Wiklind |
4:35-5:20 |
The Study of Molecular and Atomic Gas in High-z Galaxies and Quasars An Historical Overview: Cox |
5:20-5:40 |
Instrumentation Development Discussion |
7-10pm |
Conference Dinner at Cavalier Inn – Roast: Vanden Bout, Brown, A. Sargent, Bash, Cox |
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Saturday, Sept. 15
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9-9:45 |
Simulations and Modeling of the ISM in Galaxies: Lagos |
9:45-10:10 |
CHILES: a Pilot for an EVLA HI Deep Field: van Gorkum |
10:10-10:35 |
A Beautiful SMG Pair in COSMOS: Sheth |
10:35-11:05 |
Break |
11:05-11:50 |
Physical Conditions in the Interstellar Medium of High-Redshift Galaxies Mass Budget and Gas Excitation: Reichers |
11:50-12:15 |
Spatial Variation of CO Excitation in High-z Galaxies: Sharon |
12:15-12:40 |
Molecular CO 1-0 in High Redshift Radio Galaxies Using the ATCA: Mao |
12:40-1:40 |
Lunch |
1:40-2:25 |
Star Formation and Molecular Gas over Cosmic Time: M. Sargent |
2:25-2:50 |
Unveiling the CO Properties of Star-forming Disk Galaxies at z~1.5 with JVLA: Aravena |
2:50-3:15 |
GBT Zpectrometer CO J=1-0 Observations of Dusty Star-forming Galaxies at z~3-3.5: Harris |
3:15-3:45 |
Break |
3:45-4:10 |
Constraints on Variations of Fundamental Constants from High Redshift Atomic and Molecular Emission and Absorption: Menten |
4:10-4:35 |
Molecular Deep Fields: Walter |
4:35-5:20 |
High-z ISM Future Perspectives: Yun |
5:20-5:35 |
Wrap-Up |
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