{"paper":{"title":"First Searches for Dark Matter with the KM3NeT Neutrino Telescopes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Ambrosone, A. Bariego-Quintana, A. B. Bouasla, A. Capone, A. Chen, A. Coleiro, A. Condorelli, A. Creusot, A. De Benedittis, A. Domi, A. Eddymaoui, A. Enzenh\\\"ofer, A. F. D\\'iaz, A. Garcia Soto, A. Heijboer, A. Kouchner, A. Lazo, A. Manfreda, A. Margiotta, A. Marinelli, A. Moussa, A. M. P\\u{a}un, A. Nayerhoda, A. Orlando, A. Plavin, A. R. Alhebsi, A. Romanov, A. S\\'anchez Losa, A. Sharma, A. Simonelli, A. Sinopoulou, A. Tudorache, A. Ukleja, A. Vacheret, A. van Vliet, A. Veutro, A. \\v{S}aina, A. Zegarelli, B. Baret, B. Caiffi, B. De Martino, B. Guillon, B. J. Jung, B. K. Gibson, B. Nkosi, B. \\'O Fearraigh, B. Spisso, B. Trocm\\'e, C. A. Nicolau, C.A. Quiroz-Rangel, C. Bozza, C. Distefano, C. Donzaud, C. Gatius Oliver, C. Guidi, C. Haack, C. Kopper, C. Lastoria, C. Markou, C. M. Mollo, C. Pastore, C. Poir\\'e, D. Bonanno, D. Calvo, D. Diego-Tortosa, D. Dornic, D. Drouhin, D. F. E. Samtleben, D. Franciotti, D. Joly, D. M. Benoit, D. Paesani, D. Real, D. Santonocito, D. Stavropoulos, D. van Eijk, D. Vivolo, D. Zito, E. Berbee, E. Buis, E. De Wolf, E. Drakopoulou, E. Eckerov\\'a, E. Genton, E. Giorgio, E.J. Pastor G\\'omez, E. Leonora, E. Migneco, E. Oukacha, E. Ros, E. Tzamariudaki, F. Ameli, F. Badaracco, F. Benfenati, F. Bretaudeau, F. Carenini, F. Filippini, F. Longhitano, F. Magnani, F. Mamedov, F. Salesa Greus, F. Vazquez de Sola, F. \\v{S}imkovic, G. Cuttone, G. de Wasseige, G. E. P\\u{a}v\\u{a}la\\c{s}, G. Ferrara, G. Illuminati, G. Kistauri, G. Larosa, G. Lehaut, G. Levi, G. Miele, G. Papalashvili, G. Riccobene, G. Takadze, G. Vannoye, G. Vasileiadis, H. Br\\^anz\\u{a}\\c{s}, H. Ghaddari, H. M. Schutte, H. Thiersen, H. van Haren, I. C. Rea, I. Del Rosso, I. Di Palma, I. El Bojaddaini, I. Goos, I. Lhenry-Yvon, I. Mozun Mateo, I. Sgura, I. Tosta e Melo, I. \\v{S}tekl, J. A. B. Coelho, J. Aublin, J. Boumaaza, J. Brunner, J. Busto, J. D. Zornoza, J. Garc\\'ia M\\'endez, J.-G. Ducoin, J. J. Hern\\'andez-Rey, J. Lazar, J. Majumdar, J. Mauro, J. Palacios Gonz\\'alez, J. Prado, J. Schnabel, J. Schumann, J. Seneca, J. Z\\'u\\~niga, KM3NeT Collaboration: S. Aiello, L. A. Fusco, L. Aphecetche, L. Bailly-Salins, L. Cerisy, L. Gialanella, L. Hennig, L. Malerba, L. Martin, L. Morales-Gallegos, L. S. Di Mauro, M. Alshamsi, M. Andre, M. Ardid, M. Bendahman, M. Benhassi, M. Bennani, M. Boettcher, M. Bouta, M. Bouwhuis, M. Breuhaus, M. Chabab, M. Circella, M. de Jong, M. D. Filipovi\\'c, M. Eff, M. Guti\\'errez, M. Labalme, M. Lamoureux, M. Lindsey Clark, M. L. Mitsou, M. Marconi, M. Mastrodicasa, M. Musumeci, M. Perrin-Terrin, M. R. Musone, M. Sanguineti, M. Spurio, M. Taiuti, N. Gei{\\ss}elbrecht, N. Lessing, N. Randazzo, N. Sennan, N. Zywucka, P. Castaldi, P. Coyle, P. De Jong, P. Goswami, P. Migliozzi, P. Piattelli, P. Sapienza, P. Sevle, R. Bruijn, R. Bruno, R. Buompane, R. Clark, R. Cocimano, R. Coniglione, R. Dallier, R. Dvornick\\'y, R. Gracia, R. Kvatadze, R. Lahmann, R. M. Bozza, R. Muller, R. Pestes, R. Shanidze, S. Alves Garre, S. Ardid, S. Biagi, S. Celli, S. Cherubini, S. El Hedri, S. Gagliardini, S. Le Stum, S. Mastroianni, S. Navas, S. Pe\\~na Mart\\'inez, S. Pulvirenti, S. Razzaque, S. R. Gozzini, S. Sanfilippo, S. Thoudam, S. Viola, S. Zavatarelli, T. Cartraud, T. Chiarusi, T. Eberl, T. Gal, T. Pradier, T. Van Eeden, V. Bertin, V. Carretero, V. Cecchini, V. Decoene, V. Ellajosyula, V. Kueviakoe, V. Kulikovskiy, V. Lema\\^itre, V. Oliviero, V. Parisi, V. Pestel, V. Popa, V. Tsourapis, V. Valsecchi, V. Van Elewyck, W. Idrissi Ibnsalih, Y. Becherini, Y. Shitov, Y. Tayalati, Y. Y. Kovalev, Z. Barda\\v{c}ov\\'a","submitted_at":"2024-11-15T10:37:13Z","abstract_excerpt":"Indirect dark matter detection methods are used to observe the products of dark matter annihilations or decays originating from astrophysical objects where large amounts of dark matter are thought to accumulate. With neutrino telescopes, an excess of neutrinos is searched for in nearby dark matter reservoirs, such as the Sun and the Galactic Centre, which could potentially produce a sizeable flux of Standard Model particles.\n  The KM3NeT infrastructure, currently under construction, comprises the ARCA and ORCA undersea \\v{C}erenkov neutrino detectors located at two different sites in the Medit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.10092","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2411.10092/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}