Communication Dans Un Congrès Année : 2023

H.E.S.S. realtime follow-ups of IceCube high-energy neutrino alerts

Résumé

The evidence for multi-messenger photon and neutrino emission from the blazar TXS 0506+056 has demonstrated the importance of realtime follow-up of neutrino events by various ground- and space-based facilities. The effort of H.E.S.S. and other experiments in coordinating observations to obtain quasi-simultaneous multiwavelength flux and spectrum measurements has been critical in measuring the chance coincidence with the high-energy neutrino event IC-170922A and constraining theoretical models. For about a decade, the H.E.S.S. transient program has included a search for gamma-ray emission associated with high-energy neutrino alerts, looking for gamma-ray activity from known sources and newly detected emitters consistent with the neutrino location. In this contribution, we present an overview of follow-up activities for realtime neutrino alerts with H.E.S.S. in 2021 and 2022. Our analysis includes both public IceCube neutrino alerts and alerts exchanged as part of a joint H.E.S.S.--IceCube program. We focus on interesting coincidences observed with gamma-ray sources, particularly highlighting the significant detection of PKS 0625-35, an AGN previously detected by H.E.S.S., and three IceCube neutrinos.

Dates et versions

hal-04197438 , version 1 (06-09-2023)

Identifiants

Citer

Federica Bradascio, Halim Ashkar, Jowita Borowska, Jean Damascene Mbarubucyeye, Enzo Oukacha, et al.. H.E.S.S. realtime follow-ups of IceCube high-energy neutrino alerts. 38th International Cosmic Ray Conference, Jul 2023, Nagoya, Japan. pp.1546, ⟨10.22323/1.444.1546⟩. ⟨hal-04197438⟩
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