{"paper":{"title":"Study of long-term spectral evolution and X-ray and Gamma-ray correlation of blazars seen by HAWC","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Andr\\'es, A. Bernal, Abraham D. Falcone, A. Carrami\\~nana, A. Gonzalez Mu\\~noz, A. Iriarte, A.J. Smith, A. Lara, A.L. Longinotti, A. Nayerhoda, A. Sandoval, B.L. Dingus, C. Alvarez, C. de Le\\'on, C.D. Rho, C. Espinoza, D. Avila Rojas, D. Depaoli, D. Huang, D. Kieda, D. Rosa-Gonz\\'alez, D. Salazar-Gallegos, E. Belmont-Moreno, E. De la Fuente, E.G. P\\'erez-P\\'erez, E. Moreno, E. Ruiz-Velasco, E. Varela, E. Willox, F. Carre\\'on, F. Garfias, F. Hueyotl-Zahuantitla, Fredric Hancock, F. Ure\\~na-Mena, G. Luis-Raya, H.A. Ayala Solares, H. Le\\'on Vargas, H. Salazar, H. Zhou, I. Herzog, I.J. Watson, I. Martinez-Castellanos, I. Torres, J.A. Garc\\'ia-Gonz\\'alez, J.A. Goodman, J.A. Matthews, J.A. Montes, J.C. Arteaga-Vel\\'azquez, J.C. D\\'iaz-V\\'elez, J. Cotzomi, J. Lee, J. Mart\\'inez-Castro, J.P. Harding, J. Serna-Franco, J.T. Linnemann, K. Engel, K.L. Fan, K. Malone, K.S. Caballero-Mora, K. Tollefson, K. Whitaker, L. Nellen, L. Villase\\~nor, M.A. DuVernois, M. Durocher, M.M. Gonz\\'alez, M. Mostaf\\'a, M. Osorio, M. Schneider, M.U. Nisa, N. Di Lalla, N. Fraija, N. Omodei, O. Martinez, O. Tibolla, P. Miranda-Romagnoli, R. Alfaro, R. Babu, R. Diaz Hernandez, R. Noriega-Papaqui, R. Torres-Escobedo, R. Turner, R.W. Springer, S. Casanova, S. Couti\\~no de Le\\'on, S. Fraija, S. Groetsch, S. Hern\\'andez-Cadena, S. Kaufmann, S. Yun-C\\'arcamo, T. Capistr\\'an, U. Cotti, V. Joshi, W.H. Lee, X. Wang, Y. P\\'erez Araujo, Y. Son","submitted_at":"2025-01-25T02:55:54Z","abstract_excerpt":"The HAWC Observatory collected 6 years of extensive data, providing an ideal platform for long-term monitoring of blazars in the Very High Energy (VHE) band, without bias towards specific flux states. HAWC continuously monitors blazar activity at TeV energies, focusing on sources with a redshift of {z \\lt 0.3}, based on the Third Fermi-LAT Catalog of High-Energy sources. We specifically focused our analysis on Mrk 421 and Mrk 501, as they are the brightest blazars observed by the HAWC Observatory. With a dataset of 2143 days, this work significantly extends the monitoring previously published,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.15041","kind":"arxiv","version":1},"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/2501.15041/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"}