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author Stein, R.
Velzen, S.V.
Kowalski, M.
Franckowiak, A.
Gezari, S.
Miller-Jones, James
Frederick, S.
Sfaradi, I.
Bietenholz, M.F.
Horesh, A.
Fender, R.
Garrappa, S.
Ahumada, T.
Andreoni, I.
Belicki, J.
Bellm, E.C.
Böttcher, M.
Brinnel, V.
Burruss, R.
Cenko, S.B.
Coughlin, M.W.
Cunningham, V.
Drake, A.
Farrar, G.R.
Feeney, M.
Foley, R.J.
Gal-Yam, A.
Golkhou, V.Z.
Goobar, A.
Graham, M.J.
Hammerstein, E.
Helou, G.
Hung, T.
Kasliwal, M.M.
Kilpatrick, C.D.
Kong, A.K.H.
Kupfer, T.
Laher, R.R.
Mahabal, A.A.
Masci, F.J.
Necker, J.
Nordin, J.
Perley, D.A.
Rigault, M.
Reusch, S.
Rodriguez, H.
Rojas-Bravo, C.
Rusholme, B.
Shupe, D.L.
Singer, L.P.
Sollerman, J.
Soumagnac, M.T.
Stern, D.
Taggart, K.
van Santen, J.
Ward, C.
Woudt, P.
Yao, Y.
author_facet Stein, R.
Velzen, S.V.
Kowalski, M.
Franckowiak, A.
Gezari, S.
Miller-Jones, James
Frederick, S.
Sfaradi, I.
Bietenholz, M.F.
Horesh, A.
Fender, R.
Garrappa, S.
Ahumada, T.
Andreoni, I.
Belicki, J.
Bellm, E.C.
Böttcher, M.
Brinnel, V.
Burruss, R.
Cenko, S.B.
Coughlin, M.W.
Cunningham, V.
Drake, A.
Farrar, G.R.
Feeney, M.
Foley, R.J.
Gal-Yam, A.
Golkhou, V.Z.
Goobar, A.
Graham, M.J.
Hammerstein, E.
Helou, G.
Hung, T.
Kasliwal, M.M.
Kilpatrick, C.D.
Kong, A.K.H.
Kupfer, T.
Laher, R.R.
Mahabal, A.A.
Masci, F.J.
Necker, J.
Nordin, J.
Perley, D.A.
Rigault, M.
Reusch, S.
Rodriguez, H.
Rojas-Bravo, C.
Rusholme, B.
Shupe, D.L.
Singer, L.P.
Sollerman, J.
Soumagnac, M.T.
Stern, D.
Taggart, K.
van Santen, J.
Ward, C.
Woudt, P.
Yao, Y.
author_sort Stein, R.
building Curtin Institutional Repository
collection Online Access
description Cosmic neutrinos provide a unique window into the otherwise hidden mechanism of particle acceleration in astrophysical objects. The IceCube Collaboration recently reported the likely association of one high-energy neutrino with a flare from the relativistic jet of an active galaxy pointed towards the Earth. However a combined analysis of many similar active galaxies revealed no excess from the broader population, leaving the vast majority of the cosmic neutrino flux unexplained. Here we present the likely association of a radio-emitting tidal disruption event, AT2019dsg, with a second high-energy neutrino. AT2019dsg was identified as part of our systematic search for optical counterparts to high-energy neutrinos with the Zwicky Transient Facility. The probability of finding any coincident radio-emitting tidal disruption event by chance is 0.5%, while the probability of finding one as bright in bolometric energy flux as AT2019dsg is 0.2%. Our electromagnetic observations can be explained through a multizone model, with radio analysis revealing a central engine, embedded in a UV photosphere, that powers an extended synchrotron-emitting outflow. This provides an ideal site for petaelectronvolt neutrino production. Assuming that the association is genuine, our observations suggest that tidal disruption events with mildly relativistic outflows contribute to the cosmic neutrino flux.
first_indexed 2025-11-14T11:36:50Z
format Journal Article
id curtin-20.500.11937-91523
institution Curtin University Malaysia
institution_category Local University
language English
last_indexed 2025-11-14T11:36:50Z
publishDate 2021
publisher NATURE RESEARCH
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-915232023-05-18T02:03:12Z A tidal disruption event coincident with a high-energy neutrino Stein, R. Velzen, S.V. Kowalski, M. Franckowiak, A. Gezari, S. Miller-Jones, James Frederick, S. Sfaradi, I. Bietenholz, M.F. Horesh, A. Fender, R. Garrappa, S. Ahumada, T. Andreoni, I. Belicki, J. Bellm, E.C. Böttcher, M. Brinnel, V. Burruss, R. Cenko, S.B. Coughlin, M.W. Cunningham, V. Drake, A. Farrar, G.R. Feeney, M. Foley, R.J. Gal-Yam, A. Golkhou, V.Z. Goobar, A. Graham, M.J. Hammerstein, E. Helou, G. Hung, T. Kasliwal, M.M. Kilpatrick, C.D. Kong, A.K.H. Kupfer, T. Laher, R.R. Mahabal, A.A. Masci, F.J. Necker, J. Nordin, J. Perley, D.A. Rigault, M. Reusch, S. Rodriguez, H. Rojas-Bravo, C. Rusholme, B. Shupe, D.L. Singer, L.P. Sollerman, J. Soumagnac, M.T. Stern, D. Taggart, K. van Santen, J. Ward, C. Woudt, P. Yao, Y. Science & Technology Physical Sciences Astronomy & Astrophysics Cosmic neutrinos provide a unique window into the otherwise hidden mechanism of particle acceleration in astrophysical objects. The IceCube Collaboration recently reported the likely association of one high-energy neutrino with a flare from the relativistic jet of an active galaxy pointed towards the Earth. However a combined analysis of many similar active galaxies revealed no excess from the broader population, leaving the vast majority of the cosmic neutrino flux unexplained. Here we present the likely association of a radio-emitting tidal disruption event, AT2019dsg, with a second high-energy neutrino. AT2019dsg was identified as part of our systematic search for optical counterparts to high-energy neutrinos with the Zwicky Transient Facility. The probability of finding any coincident radio-emitting tidal disruption event by chance is 0.5%, while the probability of finding one as bright in bolometric energy flux as AT2019dsg is 0.2%. Our electromagnetic observations can be explained through a multizone model, with radio analysis revealing a central engine, embedded in a UV photosphere, that powers an extended synchrotron-emitting outflow. This provides an ideal site for petaelectronvolt neutrino production. Assuming that the association is genuine, our observations suggest that tidal disruption events with mildly relativistic outflows contribute to the cosmic neutrino flux. 2021 Journal Article http://hdl.handle.net/20.500.11937/91523 10.1038/s41550-020-01295-8 English http://purl.org/au-research/grants/arc/DP200102471 NATURE RESEARCH fulltext
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
Stein, R.
Velzen, S.V.
Kowalski, M.
Franckowiak, A.
Gezari, S.
Miller-Jones, James
Frederick, S.
Sfaradi, I.
Bietenholz, M.F.
Horesh, A.
Fender, R.
Garrappa, S.
Ahumada, T.
Andreoni, I.
Belicki, J.
Bellm, E.C.
Böttcher, M.
Brinnel, V.
Burruss, R.
Cenko, S.B.
Coughlin, M.W.
Cunningham, V.
Drake, A.
Farrar, G.R.
Feeney, M.
Foley, R.J.
Gal-Yam, A.
Golkhou, V.Z.
Goobar, A.
Graham, M.J.
Hammerstein, E.
Helou, G.
Hung, T.
Kasliwal, M.M.
Kilpatrick, C.D.
Kong, A.K.H.
Kupfer, T.
Laher, R.R.
Mahabal, A.A.
Masci, F.J.
Necker, J.
Nordin, J.
Perley, D.A.
Rigault, M.
Reusch, S.
Rodriguez, H.
Rojas-Bravo, C.
Rusholme, B.
Shupe, D.L.
Singer, L.P.
Sollerman, J.
Soumagnac, M.T.
Stern, D.
Taggart, K.
van Santen, J.
Ward, C.
Woudt, P.
Yao, Y.
A tidal disruption event coincident with a high-energy neutrino
title A tidal disruption event coincident with a high-energy neutrino
title_full A tidal disruption event coincident with a high-energy neutrino
title_fullStr A tidal disruption event coincident with a high-energy neutrino
title_full_unstemmed A tidal disruption event coincident with a high-energy neutrino
title_short A tidal disruption event coincident with a high-energy neutrino
title_sort tidal disruption event coincident with a high-energy neutrino
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
url http://purl.org/au-research/grants/arc/DP200102471
http://hdl.handle.net/20.500.11937/91523