Publications des scientifiques de l'IRD

Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J. J., Avgitas T., Baret B., Barrios-Marti J., Basa S., Bertin V., Biagi S., Bormuth R., Bourret S., Bouwhuis M. C., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Celli S., Chiarusi T., Circella M., Coelho J. A. B., Coleiro A., Coniglione R., Costantini H., Coyle P., Creusot A., Deschamps A., De Bonis G., Distefano C., Di Palma I., Donzaud C., Dornic D., Drouhin D., Eberl T., Bojaddaini I., Elsasser D., Enzenhofer A., Felis I., Fusco L. A., Galata S., Gay P., Geisselsoder S., Geyer K., Giordano V., Gleixner A., Glotin H., Gregoire T., Ruiz R. G., Graf K., Hallmann S., van Haren H., Heijboer A. J., Hello Yann, Hernandez-Rey J. J., Hossl J., Hofestadt J., Hugon C., Illuminati G., James C. W., de Jong M., Jongen M., Kadler M., Kalekin O., Katz U., Kiessling D., Kouchner A., Kreter M., Kreykenbohm I., Kulikovskiy V., Lachaud C., Lahmann R., Lefevre D., Leonora E., Lotze M., Loucatos S., Marcelin M., Margiotta A., Marinelli A., Martinez-Mora J. A., Mathieu A., Mele R., Melis K., Michael T., Migliozzi P., Moussa A., Mueller C., Nezri E., Pavalas G. E., Pellegrino C., Perrina C., Piattelli P., Popa V., Pradier T., Quinn L., Racca C., Riccobene G., Roensch K., Sanchez-Losa A., Saldana M., Salvadori I., Samtleben D. F. E., Sanguineti M., Sapienza P., Schnabel J., Schussler F., Seitz T., Sieger C., Spurio M., Stolarczyk T., Taiuti M., Tayalati Y., Trovato A., Tselengidou M., Turpin D., Tonnis C., Vallage B., Vallee C., Van Elewyck V., Vivolo D., Vizzoca A., Wagner S., Wilms J., Zornoza J. D., Zuniga J. (2020). Model-independent search for neutrino sources with the ANTARES neutrino telescope. Astroparticle Physics, 114, p. 35-47. ISSN 0927-6505.

Titre du document
Model-independent search for neutrino sources with the ANTARES neutrino telescope
Année de publication
2020
Type de document
Article référencé dans le Web of Science WOS:000489353300005
Auteurs
Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J. J., Avgitas T., Baret B., Barrios-Marti J., Basa S., Bertin V., Biagi S., Bormuth R., Bourret S., Bouwhuis M. C., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Celli S., Chiarusi T., Circella M., Coelho J. A. B., Coleiro A., Coniglione R., Costantini H., Coyle P., Creusot A., Deschamps A., De Bonis G., Distefano C., Di Palma I., Donzaud C., Dornic D., Drouhin D., Eberl T., Bojaddaini I., Elsasser D., Enzenhofer A., Felis I., Fusco L. A., Galata S., Gay P., Geisselsoder S., Geyer K., Giordano V., Gleixner A., Glotin H., Gregoire T., Ruiz R. G., Graf K., Hallmann S., van Haren H., Heijboer A. J., Hello Yann, Hernandez-Rey J. J., Hossl J., Hofestadt J., Hugon C., Illuminati G., James C. W., de Jong M., Jongen M., Kadler M., Kalekin O., Katz U., Kiessling D., Kouchner A., Kreter M., Kreykenbohm I., Kulikovskiy V., Lachaud C., Lahmann R., Lefevre D., Leonora E., Lotze M., Loucatos S., Marcelin M., Margiotta A., Marinelli A., Martinez-Mora J. A., Mathieu A., Mele R., Melis K., Michael T., Migliozzi P., Moussa A., Mueller C., Nezri E., Pavalas G. E., Pellegrino C., Perrina C., Piattelli P., Popa V., Pradier T., Quinn L., Racca C., Riccobene G., Roensch K., Sanchez-Losa A., Saldana M., Salvadori I., Samtleben D. F. E., Sanguineti M., Sapienza P., Schnabel J., Schussler F., Seitz T., Sieger C., Spurio M., Stolarczyk T., Taiuti M., Tayalati Y., Trovato A., Tselengidou M., Turpin D., Tonnis C., Vallage B., Vallee C., Van Elewyck V., Vivolo D., Vizzoca A., Wagner S., Wilms J., Zornoza J. D., Zuniga J.
Source
Astroparticle Physics, 2020, 114, p. 35-47 ISSN 0927-6505
A novel method to analyse the spatial distribution of neutrino candidates recorded with the ANTARES neutrino telescope is introduced, searching for an excess of neutrinos in a region of arbitrary size and shape from any direction in the sky. Techniques originating from the domains of machine learning, pattern recognition and image processing are used to purify the sample of neutrino candidates and for the analysis of the obtained skymap. In contrast to a dedicated search for a specific neutrino emission model, this approach is sensitive to a wide range of possible morphologies of potential sources of high-energy neutrino emission. The application of these methods to ANTARES data yields a large-scale excess with a post-trial significance of 2.5 sigma. Applied to public data from IceCube in its IC40 configuration, an excess consistent with the results from ANTARES is observed with a post-trial significance of 2.1 sigma.
Plan de classement
Sciences fondamentales / Techniques d'analyse et de recherche [020]
Localisation
Fonds IRD [F B010077093]
Identifiant IRD
fdi:010077093
Contact