{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:TSGUGVCYVW2GWNHQU2WTWQVARQ","short_pith_number":"pith:TSGUGVCY","schema_version":"1.0","canonical_sha256":"9c8d435458adb46b34f0a6ad3b42a08c27b26e55a18b605f3ef37ff68b6c2dc4","source":{"kind":"arxiv","id":"0710.2722","version":1},"attestation_state":"computed","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"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"0710.2722","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-10-15T06:01:33Z","cross_cats_sorted":[],"title_canon_sha256":"d2f40526beadf8b5396ddd4184e481869a588f4edd0bedc61f362fc3e9b0646a","abstract_canon_sha256":"2d6e87601aac2578a1a8e206857f3eff31201f3eeb13b977eed76ef44650834f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:16:10.471834Z","signature_b64":"SON/lVzBXJ9OFKogg8LMmngt2rJGfU8LvqOgh93vehQYthU/JAxxUFZCZS6lPuDUComwJ2sc96h61HgvbIXIBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c8d435458adb46b34f0a6ad3b42a08c27b26e55a18b605f3ef37ff68b6c2dc4","last_reissued_at":"2026-05-18T02:16:10.471114Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:16:10.471114Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"0710.2722","created_at":"2026-05-18T02:16:10.471219+00:00"},{"alias_kind":"arxiv_version","alias_value":"0710.2722v1","created_at":"2026-05-18T02:16:10.471219+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0710.2722","created_at":"2026-05-18T02:16:10.471219+00:00"},{"alias_kind":"pith_short_12","alias_value":"TSGUGVCYVW2G","created_at":"2026-05-18T12:25:56.245647+00:00"},{"alias_kind":"pith_short_16","alias_value":"TSGUGVCYVW2GWNHQ","created_at":"2026-05-18T12:25:56.245647+00:00"},{"alias_kind":"pith_short_8","alias_value":"TSGUGVCY","created_at":"2026-05-18T12:25:56.245647+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ","json":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ.json","graph_json":"https://pith.science/api/pith-number/TSGUGVCYVW2GWNHQU2WTWQVARQ/graph.json","events_json":"https://pith.science/api/pith-number/TSGUGVCYVW2GWNHQU2WTWQVARQ/events.json","paper":"https://pith.science/paper/TSGUGVCY"},"agent_actions":{"view_html":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ","download_json":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ.json","view_paper":"https://pith.science/paper/TSGUGVCY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0710.2722&json=true","fetch_graph":"https://pith.science/api/pith-number/TSGUGVCYVW2GWNHQU2WTWQVARQ/graph.json","fetch_events":"https://pith.science/api/pith-number/TSGUGVCYVW2GWNHQU2WTWQVARQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ/action/storage_attestation","attest_author":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ/action/author_attestation","sign_citation":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ/action/citation_signature","submit_replication":"https://pith.science/pith/TSGUGVCYVW2GWNHQU2WTWQVARQ/action/replication_record"}},"created_at":"2026-05-18T02:16:10.471219+00:00","updated_at":"2026-05-18T02:16:10.471219+00:00"}