{"paper":{"title":"On the interpretation of the Fermi GBM transient observed in coincidence with LIGO Gravitational Wave Event GW150914","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Goldstein, A. von Kienlin, C. A. Meegan, C. A. Wilson-Hodge, C. M. Hui, D. Kocevski, E. Bissaldi, E. Burns, J. E. McEnery, J. Racusin, J. Veitch, L. Blackburn, M. H. Gibby, M. M. Giles, M. S. Briggs, M. Stanbro, N. Christensen, O. J. Roberts, P. N. Bhat, P. Shawhan, P. Veres, R. D. Preece, R. M. Kippen, S. McBreen, T. Littenberg, V. Connaughton, W. Cleveland, W. S. Paciesas","submitted_at":"2018-01-08T04:23:29Z","abstract_excerpt":"The weak transient detected by the Fermi Gamma-ray Burst Monitor (GBM) 0.4 s after GW150914 has generated much speculation regarding its possible association with the black-hole binary merger. Investigation of the GBM data by Connaughton et al. (2016) revealed a source location consistent with GW150914 and a spectrum consistent with a weak, short Gamma-Ray Burst.\n  Greiner et al. (2016) present an alternative technique for fitting background-limited data in the low-count regime, and call into question the spectral analysis and the significance of the detection of GW150914-GBM presented in Conn"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.02305","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"}