{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:G3SGW27WA3JNMD4TIMLDF35MWS","short_pith_number":"pith:G3SGW27W","schema_version":"1.0","canonical_sha256":"36e46b6bf606d2d60f93431632efacb49ac381fc154733b1ef70033f8dd1070d","source":{"kind":"arxiv","id":"1612.00634","version":2},"attestation_state":"computed","paper":{"title":"The giant radio flare of Cygnus X-3 in September 2016","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"G.V. Zhekanis, N.A. Nizhelskij, P.G. Tsybulev, S.A. Trushkin","submitted_at":"2016-12-02T11:14:40Z","abstract_excerpt":"In the long-term multi-frequency monitoring program of the microquasars with RATAN-600 we discovered the giant flare from the X-ray binary Cygnus X-3 on 13 September 2016. It happened after 2000 days of the 'quiescent state' of the source passed after the former giant flare (~18 Jy) in March 2011. We have found that during this quiet period the hard X-ray flux (Swift/BAT, 15-50 keV) and radio flux (RATAN-600, 11 GHz) have been strongly anti-correlated. Both radio flares occurred after transitions of the microquasar to a 'hypersoft' X-ray state that occurred in February 2011 and in the end of A"},"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":"1612.00634","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-12-02T11:14:40Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"2227e5b81ab92ae45b3e3b4f756cbabf6635114fb8a45bc02303d2eebe16e4b4","abstract_canon_sha256":"74a951af2371e39f2663279566a9d734f2a449c273d83f0870a246d06f61d078"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:55:20.200754Z","signature_b64":"n3Stlwk+gKo0HqG2l1wEojKkgf6AvEFkUl//2YSAYxEU7AEXOl0Ky9lcYjd/UuAx5ODARDQrA81cAdw/mEWCBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"36e46b6bf606d2d60f93431632efacb49ac381fc154733b1ef70033f8dd1070d","last_reissued_at":"2026-05-18T00:55:20.200095Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:55:20.200095Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The giant radio flare of Cygnus X-3 in September 2016","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"G.V. Zhekanis, N.A. Nizhelskij, P.G. Tsybulev, S.A. Trushkin","submitted_at":"2016-12-02T11:14:40Z","abstract_excerpt":"In the long-term multi-frequency monitoring program of the microquasars with RATAN-600 we discovered the giant flare from the X-ray binary Cygnus X-3 on 13 September 2016. It happened after 2000 days of the 'quiescent state' of the source passed after the former giant flare (~18 Jy) in March 2011. We have found that during this quiet period the hard X-ray flux (Swift/BAT, 15-50 keV) and radio flux (RATAN-600, 11 GHz) have been strongly anti-correlated. Both radio flares occurred after transitions of the microquasar to a 'hypersoft' X-ray state that occurred in February 2011 and in the end of A"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.00634","kind":"arxiv","version":2},"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":"1612.00634","created_at":"2026-05-18T00:55:20.200191+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.00634v2","created_at":"2026-05-18T00:55:20.200191+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.00634","created_at":"2026-05-18T00:55:20.200191+00:00"},{"alias_kind":"pith_short_12","alias_value":"G3SGW27WA3JN","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_16","alias_value":"G3SGW27WA3JNMD4T","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_8","alias_value":"G3SGW27W","created_at":"2026-05-18T12:30:15.759754+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/G3SGW27WA3JNMD4TIMLDF35MWS","json":"https://pith.science/pith/G3SGW27WA3JNMD4TIMLDF35MWS.json","graph_json":"https://pith.science/api/pith-number/G3SGW27WA3JNMD4TIMLDF35MWS/graph.json","events_json":"https://pith.science/api/pith-number/G3SGW27WA3JNMD4TIMLDF35MWS/events.json","paper":"https://pith.science/paper/G3SGW27W"},"agent_actions":{"view_html":"https://pith.science/pith/G3SGW27WA3JNMD4TIMLDF35MWS","download_json":"https://pith.science/pith/G3SGW27WA3JNMD4TIMLDF35MWS.json","view_paper":"https://pith.science/paper/G3SGW27W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.00634&json=true","fetch_graph":"https://pith.science/api/pith-number/G3SGW27WA3JNMD4TIMLDF35MWS/graph.json","fetch_events":"https://pith.science/api/pith-number/G3SGW27WA3JNMD4TIMLDF35MWS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G3SGW27WA3JNMD4TIMLDF35MWS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G3SGW27WA3JNMD4TIMLDF35MWS/action/storage_attestation","attest_author":"https://pith.science/pith/G3SGW27WA3JNMD4TIMLDF35MWS/action/author_attestation","sign_citation":"https://pith.science/pith/G3SGW27WA3JNMD4TIMLDF35MWS/action/citation_signature","submit_replication":"https://pith.science/pith/G3SGW27WA3JNMD4TIMLDF35MWS/action/replication_record"}},"created_at":"2026-05-18T00:55:20.200191+00:00","updated_at":"2026-05-18T00:55:20.200191+00:00"}