{"paper":{"title":"A low-luminosity soft state in the short period black hole X-ray binary Swift J1753.5-0127","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. W. Shaw, D. Altamirano, D. J. Walton, F. F\\\"urst, F. Rahoui, J. A. Tomsick, P. A. Charles, P. Gandhi, P. Uttley","submitted_at":"2016-02-18T14:36:38Z","abstract_excerpt":"We present results from the spectral fitting of the candidate black hole X-ray binary Swift J1753.5-0127 in an accretion state previously unseen in this source. We fit the 0.7-78 keV spectrum with a number of models, however the preferred model is one of a multi-temperature disk with an inner disk temperature $\\mathrm{k}T_\\mathrm{in}=0.252\\pm0.003$ keV scattered into a steep power-law with photon index $\\Gamma=6.39^{+0.08}_{-0.02}$ and an additional hard power law tail ($\\Gamma=1.79\\pm0.02$). We report on the emergence of a strong disk-dominated component in the X-ray spectrum and we conclude "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.05816","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"}