%0 Journal Article
%A Stein, Robert
%A Van Velzen, Sjoert
%A Kowalski, Marek
%A Franckowiak, Anna
%A Gezari, Suvi
%A Miller-Jones, James C. A.
%A Frederick, Sara
%A Sfaradi, Itai
%A Bietenholz, Michael F.
%A Horesh, Assaf
%A Fender, Rob
%A Garrappa, Simone
%A Ahumada, Tomás
%A Andreoni, Igor
%A Belicki, Justin
%A Bellm, Eric C.
%A Böttcher, Markus
%A Brinnel, Valery
%A Burruss, Rick
%A Cenko, S. Bradley
%A Coughlin, Michael W.
%A Cunningham, Virginia
%A Drake, Andrew
%A Farrar, Glennys R.
%A Feeney, Michael
%A Foley, Ryan J.
%A Gal-Yam, Avishay
%A Golkhou, V. Zach
%A Goobar, Ariel
%A Graham, Matthew J.
%A Hammerstein, Erica
%A Helou, George
%A Hung, Tiara
%A Kasliwal, Mansi M.
%A Kilpatrick, Charles D.
%A Kong, Al-Bert K. H.
%A Kupfer, Thomas
%A Laher, Russ R.
%A Mahabal, Ashish A.
%A Masci, Frank J.
%A Necker, Jannis David
%A Nordin, Jakob
%A Perley, Daniel A.
%A Rigault, Mickael
%A Reusch, Simeon
%A Rodriguez, Hector
%A Rojas-Bravo, César
%A Rusholme, Ben
%A Shupe, David L.
%A Singer, Leo P.
%A Sollerman, Jesper
%A Soumagnac, Maayane T.
%A Stern, Daniel
%A Taggart, Kirsty
%A Santen, Jakob van
%A Ward, Charlotte
%A Woudt, Patrick
%A Yao, Yuhan
%T A tidal disruption event coincident with a high-energy neutrino
%J Nature astronomy
%V 5
%N 5
%@ 2397-3366
%C London
%I Nature Publishing Group
%M PUBDB-2021-02627
%M arXiv:2005.05340
%P 510 - 518
%D 2021
%Z Waiting for fulltext   55 pages, 8 figures, 8 tables
%X The tidal disruption event AT2019dsg is probably associated with a high-energy neutrino, suggesting that such events can contribute to the cosmic neutrino flux. The electromagnetic emission is explained in terms of a central engine, a photosphere and an extended synchrotron-emitting outflow.
%K neutrino: flux (INSPIRE)
%K jet: relativistic (INSPIRE)
%K neutrino: production (INSPIRE)
%K neutrino: spectrum (INSPIRE)
%K neutrino: energy: high (INSPIRE)
%K energy: flux (INSPIRE)
%K particle: acceleration (INSPIRE)
%K galaxy (INSPIRE)
%K electromagnetic (INSPIRE)
%K bolometer (INSPIRE)
%K optical (INSPIRE)
%K IceCube (INSPIRE)
%K site (INSPIRE)
%K ultraviolet (INSPIRE)
%K synchrotron radiation (INSPIRE)
%K electron (INSPIRE)
%K gamma ray (INSPIRE)
%K Cherenkov counter (INSPIRE)
%K GLAST (INSPIRE)
%K neutrino: oscillation (INSPIRE)
%K pi: production (INSPIRE)
%K star: mass (INSPIRE)
%K photon: thermal (INSPIRE)
%K p: accelerator (INSPIRE)
%K interaction (INSPIRE)
%K p p (INSPIRE)
%K cross section (INSPIRE)
%K radio wave (INSPIRE)
%K black hole (INSPIRE)
%K cosmic radiation: UHE (INSPIRE)
%K X-ray (INSPIRE)
%K Doppler effect (INSPIRE)
%K black body (INSPIRE)
%F PUB:(DE-HGF)16
%9 Journal Article
%U <Go to ISI:>//WOS:000620431500002
%R 10.1038/s41550-020-01295-8
%U https://bib-pubdb1.desy.de/record/459603