{"paper":{"title":"X-ray and gamma-ray study for 2023 nova eruption of V1716 Sco","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"H.-D. Yan, H.-H. Wang, J. Takata, L.C.-C. Lin","submitted_at":"2024-06-27T14:58:05Z","abstract_excerpt":"We report the results of X-ray and gamma-ray analyses of the classical-nova V1716 Sco using data taken by \\verb|Swift|, \\verb|NICER|, \\verb|NuSTAR| and \\verb|Fermi|-LAT. We confirm gamma-ray emission at a significant level exceeding 8~$\\sigma$ in the one-day bin immediately following the optical eruption. The gamma-ray emission, with a Test Statistic value more than four, persists for approximately 40 days. The X-ray emission being concurrent with the gamma-ray emission is described by the optically thin thermal plasma emission and it is likely dominated by the emission from the gas heated up "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.19233","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/2406.19233/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"}