| Time (PDT) | Title | Speaker |
| 8:30 am | Welcome and Opening Comments | |
| 9:00 am | Introduction to Roman | |
| 9:30 am | Introduction to Microlensing and Its Historical Perspectives | |
| 10:15 am | Break | |
| 10:45 am | Planet Populations, or Why Do We Need Roman | |
| 11:30 am | Introduction to Other Microlensing Sources | |
| 12:00 pm | Poster Pops I | |
| 12:30 pm | Lunch | |
| 1:30 pm | Poster Session I | |
| 2:15 pm | Theory of Planet Formation and Planetary System Architectures | |
| 3:00 pm | Introduction to the Galactic Bulge Time Domain Survey | |
| 3:30 pm | Break | |
| 4:00 pm | Introduction to Hands-On Session I | |
| 4:20 pm | Introduction to Hands-On Session II | |
| 4:40 pm | Adjourn |
| Time (PDT) | Title | Speaker |
| 8:30 am | Fundamentals of Microlensing | |
| 9:00 am | Higher-Order Effects in Microlensing | |
| 9:30 am | Microlensing Planet Host Star Characterization | |
| 10:00 am | Break | |
| 10:30 am | Challenges in Roman Microlensing | |
| 11:00 am | Roman Microlensing Planet Yields | |
| 11:30 am | Dealing with Dust in the Galactic Plane | |
| 12:00 pm | Poster Pops II | |
| 12:30 pm | Lunch | |
| 1:30 pm | Hands-On Session I | |
| 5:00 pm | Adjourn | |
| 5:30 pm | Optional Dinner |
| Time (PDT) | Title | Speaker |
| 8:30 am | Fundamentals of Transiting Planets | |
| 9:00 am | Challenges with Roman Transits | |
| 9:30 am | Roman Transiting Planet Yields | |
| 10:00 am | Break | |
| 10:30 am | Galactic Context | |
| 11:00 am | Introduction to Microlensing Occurrence Rate Methods | |
| 11:30 am | Introduction to Transit Occurrence Rate Methods | |
| 12:00 pm | Completing the Galactic Census of Planets: Combining Microlensing and Transit Demographics | |
| 12:30 pm | Lunch | |
| 1:30 pm | Poster Session II | |
| 2:15 pm | Hands-On Session II | |
| 5:00 pm | Adjourn |
| Time (PDT) | Title | Speaker |
| 8:30 am | Microlensing Pipelines: From Pixels to Lightcurves (AKA the Challenges of Crowded Field Photometry and Astrometry) | |
| 9:00 am | Microlensing Pipelines: From Lightcurves to Characterization (AKA the Pros and Cons of Different Microlensing Event Modeling Techniques) | |
| 9:30 am | Transit Pipelines | |
| 10:00 am | Characterizing Transit Host Stars | |
| 10:30 am | Break | |
| 11:00 am | Non-Exoplanet Science with the GBTDS (Astrophysics) | |
| 11:45 am | Non-Exoplanet Science with the GBTDS (Solar System) | |
| 12:15 pm | Group Photo | |
| 12:30 pm | Lunch | |
| 1:30 pm | Hands-on Session: Group Projects | |
| 5:00 pm | Adjourn |
| Time (PDT) | Title | Speaker |
| 8:30 am | Precursor Observations (Euclid, HST) | |
| 9:00 am | Individual Microlensing Event Follow-Up with Big Telescopes | |
| 9:30 am | Contemporaneous Microlensing Surveys | |
| 10:00 am | Contemporaneous Time Domain Surveys | |
| 10:30 am | Break | |
| 11:00 am | The Roman GPS and How It Can Be Used to Expand on Microlensing and Transit Surveys | |
| 11:30 am | Panel: Exoplanet Demographics Opportunities with Roman GO Time | |
| 12:15 pm | Lunch | |
| 1:15 pm | How Roman Science Leads to HWO | |
| 1:45 pm | How Roman Coronagraph Technology Leads to HWO | |
| 2:15 pm | Break | |
| 2:45 pm | Group Project Presentations | |
| 4:45 pm | Closing Comments | |
| 5:00 pm | Adjourn |
Questions? Sagan_Workshop@ipac.caltech.edu
(last updated December 17th, 2025 22:19:03)
The NASA Exoplanet Science Institute is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program.
