PoS - Proceedings of Science
Volume 444 - 38th International Cosmic Ray Conference (ICRC2023) - Neutrino Astronomy & Physics (NU)
VAE-based latent-space classification of RNO-G data
T. Glüsenkamp*,  Rno-g, J.A.A. Aguilar, P. Allison, D.Z. Besson, A. Bishop, O. Botner, S. Bouma, S. Buitink, W. Castiglioni, M. Cataldo, B.A. Clark, A. Coleman, K. Couberly, P. Dasgupta, S. De Kockere, K.D. de Vries, C. Deaconu, M.A. DuVernois, A. Eimer, C. Glaser, A. Hallgren, S. Hallmann, J.C. Hanson, B. Hendricks, J. Henrichs, N. Heyer, C. Hornhuber, K. Hughes, T. Karg, A. Karle, J.L. Kelley, M. Korntheuer, M. Kowalski, I. Kravchenko, R. Krebs, R. Lahmann, P. Lehmann, U.A. Latif, P. Laub, H. Liu, J. Mammo, M.J. Marsee, Z.S. Meyers, M. Mikhailova, K. Michaels, K. Mulrey, M. Muzio, A. Nelles, A. Novikov, A. Nozdrina, E. Oberla, B. Oeyen, I. Plaisier, N. Punsuebsay, L. Pyras, D. Ryckbosch, F. Schlüter, O. Scholten, D. Seckel, M.F.H. Seikh, D.J.B. Smith, J. Stoffels, D. Southall, K. Terveer, S. Toscano, D. Tosi, D.J. Van Den Broeck, N. van Eijndhoven, A.G. Vieregg, J.Z. Vischer, C. Welling, D.R. Williams, S.A. Wissel, R. Young and A. Zinket al. (click to show)
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Pre-published on: July 25, 2023
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Abstract
The Radio Neutrino Observatory in Greenland (RNO-G) is a radio-based ultra-high energy neutrino detector located at Summit Station, Greenland. It is still being constructed, with 7 stations currently operational. Neutrino detection works by measuring Askaryan radiation produced by neutrino-nucleon interactions. A neutrino candidate must be found amidst other backgrounds which are recorded at much higher rates---including cosmic-rays and anthropogenic noise---the origins of which are sometimes unknown. Here we describe a method to classify different noise classes using the latent space of a variational autoencoder. The latent space forms a compact representation that makes classification tractable. We analyze data from a noisy and a silent station. The method automatically detects and allows us to qualitatively separate multiple event classes, including physical wind-induced signals, for both the noisy and the quiet station.
DOI: https://doi.org/10.22323/1.444.1056
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