Eric Charles Two recent developments with Gamma Ray Burst Classification And their implications...

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GLAST Performance I: LAT Angular Resolution (per  ) thinthick Effective Area all layers At 30 (100) MeV single photon Angular resolution ~ 10° (3°) PSF occupies 0.09 sr ( sr) For typical observation angle F = 40°: A eff (40°) ~ 0.75 A eff (0°)

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Population III Gamma-Ray Burst - hp.phys.titech.ac.jp · Gamma-Ray Burst Kunihito Ioka (KEK)! Suwa & KI arXiv:1009.6001! Nagakura+ arXiv:1104.5691! de Souza, Yoshida & KI arXiv:1105.2395!

Population III Gamma-Ray Burst - hp.phys.titech.ac.jp · Gamma-Ray Burst Kunihito Ioka (KEK)! Suwa & KI arXiv:1009.6001! Nagakura+ arXiv:1104.5691! de Souza, Yoshida & KI arXiv:1105.2395!

CALET Gamma-ray Burst Monitor observationsCALET CALET Gamma-ray Burst Monitor observations CALET S.B. Ricciarini for the CALET collaboration COSPAR 2018 Pasadena, 17 July 2018

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