Lake Baikal, home of the Baikal neutrino telescope

Blazar and neutrino source · 22 September 2017 · announced July 2018

TXS 0506+056

The high-energy neutrino IceCube-170922A arrived from the direction of a flaring gamma-ray blazar, the first evidence for a source of cosmic neutrinos.

Our part

The alert met the criteria of the H.E.S.S. neutrino follow-up programme Fabian had set up, and H.E.S.S. took part in the worldwide observing campaign.

Follow-up, step by step

  1. 20:54:30 UTC
    IceCube

    Real-time analysis detects a neutrino of about 290 TeV.

  2. T0 + 43 s
    IceCube

    Alert distributed to observers worldwide.

  3. T0 + ~4 h
    H.E.S.S.

    The direction becomes visible from Namibia and follow-up observations are possible.

  4. Following weeks
    Fermi-LAT and partners

    The blazar is found in a flaring state; a campaign from radio to very-high-energy gamma rays follows.

  5. 12 July 2018
    Publications

    Joint results published in Science.

Illustration of the observatories that took part in the multi-messenger campaign on the neutrino IceCube-170922A and the blazar TXS 0506+056

Papers