Search for multi-flare neutrino emissions in 10 years of IceCube data from a catalog of sources
IceCube collaboration: R. Abbasi, M. Ackermann, J. Adams, J. A., Aguilar, M. Ahlers, M. Ahrens, C. Alispach, A. A. Alves Jr., N. M. Amin, R., An, K. Andeen, T. Anderson, G. Anton, C. Arg\"uelles, Y. Ashida, S. Axani, X., Bai, A. Balagopal V., A. Barbano, S. W. Barwick

TL;DR
This study conducts time-dependent searches for neutrino emissions from a catalog of sources using 10 years of IceCube data, identifying potential flares and cumulative excesses, and advancing methods to detect multiple flares from individual sources.
Contribution
Introduces novel time-dependent analysis methods to identify multiple neutrino flares from sources, improving sensitivity over previous approaches.
Findings
M87 is the most significant time-dependent source at 1.7σ post-trial.
Two flares are reconstructed from TXS 0506+056.
A cumulative excess at 3.0σ is associated with four sources.
Abstract
A recent time-integrated analysis of a catalog of 110 candidate neutrino sources revealed a cumulative neutrino excess in the data collected by IceCube between April 6, 2008 and July 10, 2018. This excess, inconsistent with the background hypothesis in the Northern hemisphere at the level, is associated with four sources: NGC 1068, TXS 0506+056, PKS 1424+240 and GB6 J1542+6129. This letter presents two time-dependent neutrino emission searches on the same data sample and catalog: a point-source search that looks for the most significant time-dependent source of the catalog by combining space, energy and time information of the events, and a population test based on binomial statistics that looks for a cumulative time-dependent neutrino excess from a subset of sources. Compared to previous time-dependent searches, these analyses enable a feature to possibly find multiple…
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