TXS 0506+056 is a blazar studied through a gamma-ray flare associated in direction and time with the high-energy neutrino alert IceCube-170922A. The event motivated coordinated observations across the electromagnetic spectrum, connecting a variable relativistic source with a possible source of energetic neutrinos.[ref]
Multi-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A by IceCube Collaboration and others. Abstract: alert, directional/temporal association and follow-up observations
An association is a statistical inference involving localization, timing and backgrounds. It does not directly image the neutrino-production site or uniquely determine the jet's particle composition. The physical interpretation must account for the measured photons and neutrino evidence together.
TXS 0506+056 is a notable blazar, which is a specific type of active galactic nucleus (AGN) characterized by its relativistic jets pointing close to the Earth. This particular blazar is located in the constellation Canes Venatici. It gained significant attention due to its association with high-energy gamma-ray emissions and was identified as a source of high-energy cosmic neutrinos.
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