Follow-up of high energy neutrinos detected by the ANTARES telescope

Abstract : The ANTARES telescope is well-suited to detect high energy neutrinos produced in astrophysical transient sources as it can observe a full hemisphere of the sky with a high duty cycle. Potential neutrino sources are gamma-ray bursts, core-collapse supernovae and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a detection method based on follow-up observations from the neutrino direction has been developed. This program, denoted as TAToO, includes a network of robotic optical telescopes (TAROT, Zadko and MASTER) and the Swift-XRT telescope, which are triggered when an 'interesting' neutrino is detected by ANTARES. A follow-up of special events, such as neutrino doublets in time/space coincidence or a single neutrino having a very high energy or in the specific direction of a local galaxy, significantly improves the perspective for the detection of transient sources. The analysis of early and long term follow-up observations to search for fast and slowly varying transient sources, respectively, has been performed and the results covering optical and X-ray data are presented in this contribution.
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Contributeur : Danielle Cristofol <>
Soumis le : jeudi 21 avril 2016 - 09:41:44
Dernière modification le : jeudi 18 janvier 2018 - 01:55:52

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A. Mathieu. Follow-up of high energy neutrinos detected by the ANTARES telescope. Very Large Volume Neutrino Telescope (VLVnT-2015) , Sep 2015, Rome, Italy. EPJ Web of Conferences 116, pp.10003, 2016, 〈http://www.epj-conferences.org/articles/epjconf/abs/2016/11/epjconf-VLVnT2015_10003/epjconf-VLVnT2015_10003.html〉. 〈10.1051/epjconf/201611610003 〉. 〈in2p3-01305401〉

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