학술논문

Search for neutrinos from the tidal disruption events AT2019dsg and AT2019fdr with the ANTARES telescope
Document Type
Working Paper
Author
ANTARES CollaborationAlbert, A.Alves, S.André, M.Anghinolfi, M.Anton, G.Ardid, M.Aubert, J. -J.Aublin, J.Baret, B.Basa, S.Belhorma, B.Bendahman, M.Benfenati, F.Bertin, V.Biagi, S.Bissinger, M.Boumaaza, J.Bouta, M.Bouwhuis, M. C.Brânzaş, H.Bruijn, R.Brunner, J.Busto, J.Caiffi, B.Capone, A.Caramete, L.Carr, J.Carretero, V.Celli, S.Chabab, M.Chau, T. N.Moursli, R. Cherkaoui ElChiarusi, T.Circella, M.Coleiro, A.Colomer-Molla, M.Coniglione, R.Coyle, P.Creusot, A.Díaz, A. F.de Wasseige, G.Deschamps, A.Distefano, C.Di Palma, I.Domi, A.Donzaud, C.Dornic, D.Drouhin, D.Eberl, T.van Eeden, T.Khayati, N. ElEnzenhöfer, A.Fermani, P.Ferrara, G.Filippini, F.Fusco, L.García, R.Gatelet, Y.Gay, P.Glotin, H.Gozzini, R.Graf, K.Guidi, C.Hallmann, S.van Haren, H.Heijboer, A. J.Hello, Y.Hernández-Rey, J. J.Hößl, J.Hofestädt, J.Huang, F.Illuminati, G.James, C. W.Jisse-Jung, B.de Jong, M.de Jong, P.Jongen, M.Kadler, M.Kalekin, O.Katz, U.Khan-Chowdhury, N. R.Kouchner, A.Kreykenbohm, I.Kulikovskiy, V.Lahmann, R.Breton, R. LeLefèvre, D.Leonora, E.Levi, G.Lincetto, M.Lopez-Coto, D.Loucatos, S.Maderer, L.Manczak, J.Marcelin, M.Margiotta, A.Marinelli, A.Martínez-Mora, J. A.Melis, K.Migliozzi, P.Moser, M.Moussa, A.Muller, R.Nauta, L.Navas, S.Nezri, E.Fearraigh, B. ÓOrganokov, M.Păvălaş, G. E.Pellegrino, C.Perrin-Terrin, M.Piattelli, P.Pieterse, C.Poirè, C.Popa, V.Pradier, T.Randazzo, N.Reck, S.Riccobene, G.Romanov, A.Greus, F. SalesaSamtleben, D. F. E.Sánchez-Losa, A.Sanguineti, M.Sapienza, P.Schnabel, J.Schumann, J.Schüssler, F.Spurio, M.Stolarczyk, Th.Taiuti, M.Tayalati, Y.Tingay, S. J.Vallage, B.Van Elewyck, V.Versari, F.Viola, S.Vivolo, D.Wilms, J.Zavatarelli, S.Zegarelli, A.Zornoza, J. D.Zúñiga, J.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
Language
Abstract
On October 1, 2019, the IceCube Collaboration detected a muon track neutrino with high probability of being of astrophysical origin, IC191001A. After a few hours, the tidal disruption event (TDE) AT2019dsg, observed by the Zwicky Transient Facility (ZTF), was indicated as the most likely counterpart of the IceCube track. More recently, the follow-up campaign of the IceCube alerts by ZTF suggested a second TDE, AT2019fdr, as a promising counterpart of another IceCube muon track candidate, IC200530A, detected on May 30, 2020. These are the second and third associations between astrophysical sources and high-energy neutrinos after the compelling identification of the blazar TXS 0506+056. Here, the search for ANTARES neutrinos from the directions of AT2019dsg and AT2019fdr using a time-integrated approach is presented. As no significant evidence for space clustering is found in the ANTARES data, upper limits on the one-flavour neutrino flux and fluence are set.
Comment: 10 pages, 1 figure