{"paper":{"title":"Synchrotron Self-inverse Compton Radiation From Reverse-shock on GRB120326A","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jae-Woo Kim (CEOU, Kazutaka Yamaoka (STE, Kuiyun Huang (ASIAA/NTNU), Makoto Tashiro (Saitama U), Minsung Jang (CEOU, Myungshin Im (CEOU, Nagoya U), Satoko Takahashi (JAO/NAOJ/ASIAA), SNU), Soojong Pak (Kyung Hee U), Yuji Urata (NCU)","submitted_at":"2014-05-16T23:51:45Z","abstract_excerpt":"We present multi-wavelength observations of a typical long duration GRB 120326A at $z=1.798$, including rapid observations using a submillimeter array (SMA), and a comprehensive monitoring in X-ray and optical. The SMA observation provided the fastest detection to date among seven submillimeter afterglows at 230 GHz. The prompt spectral analysis, using Swift and Suzaku yielded a spectral peak energy of $E^{\\rm src}_{\\rm peak}=107.8^{+15.3}_{-15.3}$ keV and equivalent isotropic energy of $E_{\\rm iso}$ as $3.18^{+0.40}_{-0.32}\\times 10^{52}$ erg. The temporal evolution and spectral properties in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.4331","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"}