{"paper":{"title":"H.E.S.S. programme searching for VHE gamma rays associated with FRBs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Archaryya, A.A. Zdziarski, A. Brown, A. Chen, A. Djannati-Ata\\\"i, A. Dmytriiev, A. Jaitly, A. Kundu, A. Lemi\\`ere, A. Luashvili, A. Mehta, A. Mitchell, A. Quirrenbach, A. Santangelo, A. Sharma, A. Wierzcholska, A. Zech, B. Bruno, B. He\\ss, B. Kh\\'elifi, B. Reville, B. Rudak, C. Boisson, C. Burger-Scheidlin, C. Esca\\~nuela. Nieves, C. Steppa, C. van. Eldik, C. Venter, D. Berge, D. Horns, D. Kerszberg, D. Kostunin, D. Malyshev, E. de. Ona. Wilhelmi, E. Kasai, E. Moulin, F. Aharonian, F. Bradascio, F. Brun, F. Jankowsky, F. Rieger, F. Sch\\\"ussler, G. Fontaine, G. Grolleron, G. P\\\"uhlhofer, G. Rowell, H. Ashkar, H.M. Schutte, H. Ren, H. Salzmann, I. Jung-Richardt, J. Aschersleben, J. Bolmont, J. Borowska, J. Celic, J. Chibueze, J. Damascene. Mbarubucyeye, J. de. Assis. Scarpin, J. Djuvsland, J.F. Glicenstein, J. Glombitza, J. Mackey, J. Niemiec, J.N.S. Shapopi, J.-P. Ernenwein, J.-P. Lenain, J. Sch\\\"afer, K. Bernl\\\"ohr, K. Egberts, K. Katarzy\\'nski, K. Kosack, K. Sabri, L. Olivera-Nieto, {\\L}. Stawarz, M. Backes, M. B\\\"ottcher, M. Cerruti, M. de. Bony. de. Lavergne, M. de. Naurois, M. Filipovic, M. Holler, M. Jamrozy, M. Lemoine-Goumard, M. Meyer, M.O. Moghadam, M. Ostrowski, M. Panter, M. Punch, M. Regeard, M. Sasaki, M. Tsirou, M. Vecchi, Nu. Komin, N. \\.Zywucka, O. Chibueze, O. Reimer, P. O'Brien, R. Batzofin, R. Brose, R.D. Parsons, R.G. Lang, R. Khatoon, R. Marx, R. Moderski, R. Steenkamp, S. Casanova, S. Chandra, S. Einecke, S. Funk, S. Gabici, S.J. Wagner, S. Le. Stum, S. Panny, S. Pita, S. Ravikularaman, S. Spencer, S. Steinmassl, T. Chand, T. L. Holch, T. Takahashi, T. Tanaka, T. Wach, U. Pensec, V. Barbosa. Martins, V. Marandon, V. Sahakian, W. Hofmann, W. Klu\\'zniak, Y. Becherini, Zhiqiu. Huang","submitted_at":"2025-07-02T20:59:02Z","abstract_excerpt":"Fast Radio Bursts (FRBs) are highly energetic, extremely short-lived bursts of radio flashes. Despite extensive research, the exact cause of these outbursts remains speculative. The high luminosity, short duration, and high dispersion measure of these events suggest they result from extreme, high-energy extragalactic sources, such as highly magnetized and rapidly spinning neutron stars known as magnetars. The number of detected FRBs, including repeating ones, has grown rapidly in recent years. Except for FRB 20200428D, and FRB-like radio burst that is associated to Galactic magnetar SGR 1935+2"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.02143","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/2507.02143/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"}