{"paper":{"title":"The 2006 Radio Outburst of a Microquasar Cyg X-3: Observation and Data","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Doi, E. Kawai, H. Kobayashi, H. Sudou, H. Takaba, K. Fujisawa, K. Kohno, K. Nakanishi, K. Wakamatsu, M. Tsuboi, N. Kawai, N. Kuno, N. Mochizuki, O. Kameya, S. A. Trushkin, T. Handa, T. Kotani, T. Omodaka, T. Sawada, T. Tosaki, T. Tsukagoshi, T. Umemoto, Y. Koyama, Y. Kurono, Y. Murata","submitted_at":"2007-10-15T06:01:33Z","abstract_excerpt":"We present the results of the multi-frequency observations of radio outburst of the microquasar Cyg X-3 in February and March 2006 with the Nobeyama 45-m telescope, the Nobeyama Millimeter Array, and the Yamaguchi 32-m telescope. Since the prediction of a flare by RATAN-600, the source has been monitored from Jan 27 (UT) with these radio telescopes. At the eighteenth day after the quench of the activity, successive flares exceeding 1 Jy were observed successfully. The time scale of the variability in the active phase is presumably shorter in higher frequency bands.\n  We also present the result"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0710.2722","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"}