{"paper":{"title":"Probing stellar winds and accretion physics in high-mass X-ray binaries and ultra-luminous X-ray sources with LOFT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Baykal, A. D'A\\`i, A. Manousakis, A. Santangelo, B. Paul, C. Ferrigno, C. Wilson-Hodge, D. Klochkov, E. Bozzo, I. Kreykenbohm, J.-C. Leyder, J.M. Torrej\\'on, J. Wilms, K. Postnov, L. Zampieri, M. Chernyakova, M. Finger, M. Orlandini, N. Masetti, N. Shakura, P. Blay, P. Jenke, P. Reig, P. Romano, R. Corbet, R. Staubert, R. Walter, S.C. Inam, T. Enoto, T. Mihara, V. Doroshenko","submitted_at":"2015-01-12T19:47:47Z","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 high-mass X-ray binaries and ultra-luminous X-ray sources. For a summary, we refer to the paper."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.02777","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":""},"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"}