{"paper":{"title":"The LOFT perspective on neutron star thermonuclear bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Cumming, A. Heger, A.L. Watts, A. R\\'ozanska, C.M. Malone, D. Altamirano, D. Chakrabarty, D.K. Galloway, D.R. Ballantyne, E.F. Brown, F.B.S. Paerels, F.-K. Thielemann, H. Schatz, J. Chenevez, J.J.M. in 't Zand, J. Jos\\'e, J. Poutanen, L. Keek, M.C. Miller, M. Falanga, M. Linares, M. M\\'endez, M. Serino, M. Zingale, N. Degenaar, N.N. Weinberg, S. Bhattacharyya, S.E. Woosley, S. Mahmoodifar, S. Zhang, T.E. Strohmayer, V.F. Suleimanov, W. Yu, Y. Cavecchi","submitted_at":"2015-01-12T19:47:43Z","abstract_excerpt":"This is a White Paper in support of the mission concept of the Large Observatory for X-ray Timing (LOFT), proposed as a medium-sized ESA mission. We discuss the potential of LOFT for the study of thermonuclear X-ray bursts on accreting neutron stars. For a summary, we refer to the paper."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.02776","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":""},"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"}