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The ANtarctic Impulsive Transient Antenna (ANITA) long-duration balloonexperiment is sensitive to interactions of ultra high-energy (E > 10^{18} eV)neutrinos in the Antarctic ice sheet. The third flight of ANITA, lasting 22days, began in December 2014. We develop a methodology to search for energeticneutrinos spatially and temporally coincident with potential source classes inANITA data. This methodology is applied to several source classes: the TXS0506+056 blazar and NGC 1068, the first potential TeV neutrino sourcesidentified by IceCube, flaring high-energy blazars reported by the FermiAll-Sky Variability Analysis, gamma-ray bursts, and supernovae. Among searcheswithin the five source classes, one candidate was identified as associated withSN 2015D, although not at a statistically significant level. We proceed toplace upper limits on the source classes. We further comment on potentialapplications of this methodology to more sensitive future instruments.

A search for ultrahigh-energy neutrinos associated with astrophysical sources using the third flight of ANITA