We report on a measurement of astrophysical tau neutrinos with 9.7 yr of IceCube data. Using convolutional neural networks trained on images derived from simulated events, seven candidate <math display="inline"><mrow><msub><mrow><mi>ν</mi></mrow><mrow><mi>τ</mi></mrow></msub></mrow></math> events were found with visible energies ranging from roughly 20 TeV to 1 PeV and a median expected parent <math display="inline"><msub><mi>ν</mi><mi>τ</mi></msub></math> energy of about 200 TeV. Considering backgrounds from astrophysical and atmospheric neutrinos, and muons from <math display="inline"><msup><mi>π</mi><mo>±</mo></msup><mo>/</mo><msup><mi>K</mi><mo>±</mo></msup></math> decays in atmospheric air showers, we obtain a total estimated background of about 0.5 events, dominated by non-<math display="inline"><msub><mi>ν</mi><mi>τ</mi></msub></math> astrophysical neutrinos. Thus, we rule out the absence of astrophysical <math display="inline"><msub><mi>ν</mi><mi>τ</mi></msub></math> at the <math display="inline"><mn>5</mn><mi>σ</mi></math> level. The measured astrophysical <math display="inline"><msub><mi>ν</mi><mi>τ</mi></msub></math> flux is consistent with expectations based on previously published IceCube astrophysical neutrino flux measurements and neutrino oscillations.
de Wasseige, G., Kruiswijk, K., Lamoureux, M., Raab, C., Vereecken, M., (IceCube Collaboration)§, IceCube, & et al. (2024). Observation of Seven Astrophysical Tau Neutrino Candidates with IceCube. Physical Review Letters, 132. https://doi.org/10.1103/PhysRevLett.132.151001 (Original work published 2024)