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The ANTARES telescope is well-suited for detecting astrophysical transientneutrino sources as it can observe a full hemisphere of the sky at all timeswith a high duty cycle. The background due to atmospheric particles can bedrastically reduced, and the point-source sensitivity improved, by selecting anarrow time window around possible neutrino production periods. Blazars, beingradio-loud active galactic nuclei with their jets pointing almost directlytowards the observer, are particularly attractive potential neutrino pointsources, since they are among the most likely sources of the very high-energycosmic rays. Neutrinos and gamma rays may be produced in hadronic interactionswith the surrounding medium. Moreover, blazars generally show high timevariability in their light curves at different wavelengths and on various timescales. This paper presents a time-dependent analysis applied to a selection offlaring gamma-ray blazars observed by the FERMI/LAT experiment and by TeVCherenkov telescopes using five years of ANTARES data taken from 2008 to 2012.The results are compatible with fluctuations of the background. Upper limits onthe neutrino fluence have been produced and compared to the measured gamma-rayspectral energy distribution.

Search for muon-neutrino emission from GeV and TeV gamma-ray flaring blazars using five years of data of the ANTARES telescope