Search for Multi-flare Neutrino Emissions in 10 yr of IceCube Data from a Catalog of Sources
Author(s)
Conrad, Or
DownloadPublished version (3.361Mb)
Publisher Policy
Publisher Policy
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Terms of use
Metadata
Show full item recordAbstract
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 $3.3~\sigma$ 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 flares from a single
direction with an unbinned maximum-likelihood method. M87 is found to be the
most significant time-dependent source of this catalog at the level of
$1.7~\sigma$ post-trial, and TXS 0506+056 is the only source for which two
flares are reconstructed. The binomial test reports a cumulative time-dependent
neutrino excess in the Northern hemisphere at the level of $3.0~\sigma$
associated with four sources: M87, TXS 0506+056, GB6 J1542+6129 and NGC 1068.
Date issued
2021Department
Massachusetts Institute of Technology. Department of PhysicsJournal
The Astrophysical Journal Letters
Publisher
American Astronomical Society
Citation
Conrad, Or. 2021. "Search for Multi-flare Neutrino Emissions in 10 yr of IceCube Data from a Catalog of Sources." The Astrophysical Journal Letters, 920 (2).
Version: Final published version