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000598568 1001_ $$0P:(DE-H253)PIP1028022$$aStein, Robert$$b0$$eCorresponding author$$udesy
000598568 245__ $$aNeutrino follow-up with the Zwicky Transient Facility: Results from the first 24 campaigns
000598568 260__ $$aOxford$$bOxford Univ. Press$$c2023
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000598568 520__ $$aThe Zwicky Transient Transient Facility (ZTF) performs a systematic neutrino follow-up program, searching for optical counterparts to high-energy neutrinos with dedicated Target-of-Opportunity (ToO) observations. Since first light in March 2018, ZTF has taken prompt observations for 24 high-quality neutrino alerts from the IceCube Neutrino Observatory, with a median latency of 12.2 hours from initial neutrino detection. From two of these campaigns, we have already reported tidal disruption event (TDE) AT2019dsg and likely TDE AT2019fdr as probable counterparts, suggesting that TDEs contribute >7.8% of the astrophysical neutrino flux. We here present the full results of our program through to December 2021. No additional candidate neutrino sources were identified by our program, allowing us to place the first constraints on the underlying optical luminosity function of astrophysical neutrino sources. Transients with optical absolutes magnitudes brighter that -21 can contribute no more than 87% of the total, while transients brighter than -22 can contribute no more than 58% of the total, neglecting the effect of extinction. These are the the first observational constraints on the neutrino emission of bright populations such as superluminous supernovae. None of the neutrinos were coincident with bright optical AGN flares comparable to that observed for TXS 0506+056/IC170922A, suggesting that most astrophysical neutrinos are not produced during such optical flares. We highlight the outlook for electromagnetic neutrino follow-up programs, including the expected potential for the Rubin Observatory.
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000598568 7001_ $$0P:(DE-H253)PIP1090061$$aReusch, Simeon$$b1
000598568 7001_ $$0P:(DE-H253)PIP1006092$$aFranckowiak, Anna$$b2
000598568 7001_ $$0P:(DE-H253)PIP1006050$$aKowalski, Marek$$b3
000598568 7001_ $$0P:(DE-H253)PIP1080689$$aNecker, Jannis$$b4
000598568 7001_ $$aWeimann, Sven$$b5
000598568 7001_ $$aKasliwal, Mansi M.$$b6
000598568 7001_ $$aSollerman, Jesper$$b7
000598568 7001_ $$aAhumada, Tomas$$b8
000598568 7001_ $$aAmaro-Seoane, Pau$$b9
000598568 7001_ $$aAnand, Shreya$$b10
000598568 7001_ $$aAndreoni, Igor$$b11
000598568 7001_ $$aBellm, Eric C.$$b12
000598568 7001_ $$aBloom, Joshua S.$$b13
000598568 7001_ $$aCoughlin, Michael$$b14
000598568 7001_ $$aDe, Kishalay$$b15
000598568 7001_ $$aFremling, Christoffer$$b16
000598568 7001_ $$aGezari, Suvi$$b17
000598568 7001_ $$aGraham, Matthew$$b18
000598568 7001_ $$aGroom, Steven L.$$b19
000598568 7001_ $$aHelou, George$$b20
000598568 7001_ $$aKaplan, David L.$$b21
000598568 7001_ $$aKarambelkar, Viraj$$b22
000598568 7001_ $$aKong, Albert K. H.$$b23
000598568 7001_ $$aKool, Erik C.$$b24
000598568 7001_ $$aLincetto, Massimiliano$$b25
000598568 7001_ $$aMahabal, Ashish A.$$b26
000598568 7001_ $$aMasci, Frank J.$$b27
000598568 7001_ $$aMedford, Michael S.$$b28
000598568 7001_ $$aMorgan, Robert$$b29
000598568 7001_ $$aNordin, Jakob$$b30
000598568 7001_ $$aRodriguez, Hector$$b31
000598568 7001_ $$aSharma, Yashvi$$b32
000598568 7001_ $$avan Santen, Jakob$$b33
000598568 7001_ $$avan Velzen, Sjoert$$b34
000598568 7001_ $$aYan, Lin$$b35
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