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Utilizing Gamma Flares for Cosmic Neutrino Analysis in ANTARES: A Multi-Messenger Approach

Explore the potential of transient sources like AGNs or Gamma Ray Bursters for neutrino telescope analyses, leveraging efficient background rejection mechanisms. Signals are concentrated around source positions and correlated in time with flares or bursts, enhancing detection capabilities. ANTARES presents initial results from flare analysis using FERMI light curves and continues studies with coordination from X-ray observations by SWIFT and ASM.

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Utilizing Gamma Flares for Cosmic Neutrino Analysis in ANTARES: A Multi-Messenger Approach

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  1. Using gamma-flares for cosmic neutrino analysis in ANTARES • A multi-messenger analysis AgustínSánchez-Losa - IFIC (CSIC-Universitat de València) - e-mail: Agustin.Sanchez@ific.uv.es Transient sources, like AGNs or Gamma Ray Bursters, are among the most promising candidates for neutrino telescopes, where the rejection of background is much more efficient. • The signal would be concentrated around the source position, but also would be correlated in time with the flare or burst, typified by the light curves from different monitored sources and gamma flares detected by telescopes. AGN ν γ • First results from ANTARES flare analysis using FERMI light curves are also presented. There are also ongoing studies for the last years data, including coordination with flares observed in X-rays by SWIFT and ASM. FERMI/LAT ANTARES

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