{"paper":{"title":"Search for Astrophysical Nanosecond Optical Transients with TAIGA-HiSCORE Array","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. A. Grinyuk, A. A. Krivopalova, A. A. Lagutin, A. A. Petrukhin, A. A. Pushnin, A. A. Silaev, A. A. Silaev (junior), A. B. Tanaev, A. Chiavassa, A. D. Lukanov, A. D. Panov, A. K. Awad, A. L. Ivanova, A. L. Pakhorukov, A. N. Borodin, A. N. Dyachok, A. Pan, A. P. Kryukov, A. Porelli, A. Razumov, A. R. Gafarov, A. Vaidyanathan, A. V. Bulan, A. V. Skurikhin, A. V. Sokolov, A. V. Zagorodnikov, A. Yu. Garmash, A. Yu. Sidorenkov, B. A. Tarashansky, B. K. Lubsandorzhiev, D. A. Podgrudkov, D. Horns, D. P. Zhurov, D. V. Chernov, D. Voronin, E. A. Bonvech, E. A. Kravchenko, E. A. Osipova, E. B. Postnikov, E. E. Korosteleva, E. G. Popova, E. Rjabov, G. I. Rubtsov, G. M. Beskin, I. I. Astapov, I. I. Yashin, I. Satyshev, K. G. Kompaniets, L. A. Kuzmichev, L. G. Sveshnikova, L. G. Tkachev, L. V. Pankov, M. Blank, M. Bruckner, M. Ternovoy, M. Tluczykont, M. V. Lavrova, N. B. Lubsandorzhiev, N. M. Budnev, N. N. Kalmykov, N. Ushakov, N. V. Volkov, O. A. Gress, O. G. Grishin, P. A. Bezyazeekov, P. A. Volchugov, R. D. Monkhoev, R. I. Raikin, R. Mirzoyan, R. P. Kokoulin, R. R. Mirgazov, R. Wischnewski, S. N. Kiryuhin, T. I. Gress, V. A. Kozhin, V. A. Poleschuk, V. A. Tabolenko, V. M. Grebenyuk, V. S. Ptuskin, V. S. Samoliga, V. V. Kindin, V. V. Prosin, Y. I. Sagan, Y. Suvorkin, Yu. Lemeshev","submitted_at":"2021-09-20T15:44:28Z","abstract_excerpt":"A wide-angle Cerenkov array TAIGA-HiSCORE (FOV $\\sim$0.6 sr), was originally created as a part of TAIGA installation for high-energy gamma-ray astronomy and cosmic ray physics. Array now consist on nearly 100 optical stations on the area of 1 km$^2$. Due to high accuracy and stability ($\\sim$1 ns) of time synchronization of the optical stations the accuracy of EAS arrival direction reconstruction is reached 0.1$^\\mathrm{o}$. It was proven that the array can also be used to search for nanosecond events of the optical range. The report discusses the method of searching for optical transients usi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2109.09637","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/2109.09637/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"}