Program :: Posters :: Presenter Instructions
Monday :: Tuesday :: Wednesday :: Thursday :: Friday
| Friday, September 13 | ||||
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| Plenary 17: Missions and Infrastructure Session Chair: Brian Humensky |
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| 9:00 am - 9:30 am | Michelle Hui | Future of gamma-ray science in space | ||
| 9:30 am - 9:45 am | Jeremy Perkins | BurstCube: A CubeSat for Gravitational Wave Counterparts | ||
| 9:45 am - 10:00 am | Israel Martinez-Castellanos | The Compton Spectrometer and Imager (COSI): opportunities for joint analyses with Fermi | ||
| 10:00 am - 10:15 am | Daniel Kocevski | The StarBurst Multimessenger Pioneer | ||
| 10:15 am - 10:30 am | Vidushi Sharma | General Coordinates Network (GCN): New GCN Notices and Machine Readability of Circulars | ||
| 10:30 am - 11:00 am | Coffee Break | |||
| Plenary 18: Future Missions and Instruments Session Chair: Regina Caputo |
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| 11:00 am - 11:15 am | Nicholas White | Using High Redshift GRB to Directly Measure Reionization and Early Metal Enrichment | ||
| 11:15 am - 11:30 am | Kun Hu | First Results from the 2024 Flight of the XL-Calibur Hard X-ray Polarimetry Mission | ||
| 11:30 am - 11:45 am | Zachary Metzler | The ComPair Balloon Instrument and Flight | ||
| 11:45 am - 12:00 pm | Nabin Poudyal | Enhancing Astrophysical MeV Gamma-Ray Detection with GRAMS | ||
| 12:00 pm - 12:15 pm | Yuya Nakamura | GRAINE: Balloon-borne emulsion telescope project for the sub-GeV/GeV gamma-ray observation with a high angular resolution and a polarization sensitivity | ||
| 12:15 pm - 12:30 pm | Adrien Laviron | The performance of silicon-pixel-based trackers for the polarimetry of gamma-rays converting to e+e- pairs | ||
| 12:30 pm - 12:35 pm | SOC & LOC | Closing Remarks | ||
| 12:35 pm - 2:00 pm | Lunch on your own | |||
| Gamma-ray Science Interest Group / Future in Gamma-rays Science Analysis Group Meeting (Location: Atlantic Building, Room 2400) | ||||
| 2:00 pm - 2:20 pm | Historic Overview: 1997 report on priorities for NASA's gamma-ray astronomy program - David Thompson | |||
| Directed discussion on strategic motivation for specific science priorities that will drive gamma-ray discoveries in the next several decades. | ||||
| 2:20 pm - 2:50 pm | MeV Lines | |||
| 2:50 pm - 3:20 pm | Burst-like Transients | |||
| 3:20 pm - 3:30 pm | 10-min break | |||
| 3:30 pm - 4:00 pm | Pulsars and Magnetars | |||
| 4:00 pm - 4:30 pm | Blazars and Jets | |||