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Massimiliano Lincetto (CPPM)12/10/2026 14:00
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Angela Zegarelli (Ruhr Universität Bochum (RUB), Germany)12/10/2026 14:20
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Claire Guépin (LUPM)12/10/2026 14:40
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Srijan Sehgal (Bergische Universität Wuppertal)12/10/2026 15:00
The Pierre Auger Observatory, the world’s largest extensive air-shower detector array, is optimized for the measurement of ultra-high-energy cosmic rays (UHECRs) and also provides sensitivity to ultra-high-energy neutrinos via detection of neutrino-induced air showers. Since the start of full operations in 2004, the Observatory has delivered key results in UHECR physics, including constraints...
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Barbara Patricelli (University of Pisa and INFN - Pisa)12/10/2026 15:20
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Min ZHA12/10/2026 16:00
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Tiffany Collins (Universität Potsdam)12/10/2026 16:20
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Antonio Stamerra (INAF-OAR and SNS-Pisa)12/10/2026 16:40
Transient sources such as gamma-ray bursts (GRBs), gravitational-wave (GW) events and their electromagnetic counterparts, high-energy neutrino counterparts, and Galactic transients such as recurrent novae, have attracted increasing attention in gamma-ray astronomy. The detection of these events at energies around and above 1 TeV has provided new insights into hadronic and leptonic emission...
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Jason Hessels12/10/2026 17:20
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Lauren Rhodes12/10/2026 17:40
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13/10/2026 15:00
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Paula Sanchez Saez (ESO)13/10/2026 15:20
Unlocking the Dynamic Universe: The Case for WST as a Spectroscopic Time-Domain Machine
The dynamic universe is one of the defining scientific frontiers of the coming decades, yet our ability to fully explore it is fundamentally constrained by a spectroscopic bottleneck that will only deepen in the 2040s. Photometric surveys such as LSST and Gaia, and multi-messenger observatories including...
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13/10/2026 15:40
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