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Tuesday, April 24, 2018

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4:00 pm - 5:00 pm
East Bridge 201
Moore-Tachikawa 2d TQFTs whose values are holomorphic symplectic varieties
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4:00 pm - 5:00 pm
Cahill, Hameetman Auditorium
Measuring the Cosmic Microwave Background Polarization with the South Pole Telescope and Future Instruments
  • Abby Crites, Caltech,
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