{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:47H6NYHVLCC6CQR7XUPBQIPZV3","short_pith_number":"pith:47H6NYHV","schema_version":"1.0","canonical_sha256":"e7cfe6e0f55885e1423fbd1e1821f9aecc29f615081da23cc30b9aeb66df06ba","source":{"kind":"arxiv","id":"1204.1392","version":1},"attestation_state":"computed","paper":{"title":"VLBI and Single Dish Monitoring of 3C84 in the Period of 2009-2011","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Akihiro Doi, Anne Lahteenmaki, Filippo D'Ammando, Gabriele Giovannini, Hiroshi Nagai, Jonathan Leon-Tavares, Jun Kataoka, Keiichi Asada, Kenta Suzuki, Makoto Inoue, Marcello Giroletti, Merja Tornikoski, Monica Orienti, Motoki Kino, Seiji Kameno, Uwe Bach","submitted_at":"2012-04-06T01:34:42Z","abstract_excerpt":"The radio galaxy 3C 84 is a representative of gamma-ray-bright misaligned active galactic nuclei (AGNs) and one of the best laboratories to study the radio properties of the sub-pc jet in connection with the gamma-ray emission. In order to identify possible radio counterparts of the gamma-ray emissions in 3C 84, we study the change in structure within the central 1 pc and the light curve of sub-pc-size components C1, C2, and C3. We search for any correlation between changes in the radio components and the gamma-ray flares by making use of VLBI and single dish data. Throughout the radio monitor"},"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":"1204.1392","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-04-06T01:34:42Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"a6ff827c4ac47474ba199ee189633bb954bb0a7f4c7b872a9d52c7762277c39a","abstract_canon_sha256":"0e29788e85d7b8f506011efc689cc86f030159773ead943bd6905dc686be50ef"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:56.287916Z","signature_b64":"1Ae85945WmJFL/F6DX6cKfzLHO4Yrt9Xdl9qA33Vrk7X4GLlD3iiCMRS6NAck3omiH/N3b2mtm6TXJ3m6P2qBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e7cfe6e0f55885e1423fbd1e1821f9aecc29f615081da23cc30b9aeb66df06ba","last_reissued_at":"2026-05-18T01:57:56.287231Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:56.287231Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"VLBI and Single Dish Monitoring of 3C84 in the Period of 2009-2011","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Akihiro Doi, Anne Lahteenmaki, Filippo D'Ammando, Gabriele Giovannini, Hiroshi Nagai, Jonathan Leon-Tavares, Jun Kataoka, Keiichi Asada, Kenta Suzuki, Makoto Inoue, Marcello Giroletti, Merja Tornikoski, Monica Orienti, Motoki Kino, Seiji Kameno, Uwe Bach","submitted_at":"2012-04-06T01:34:42Z","abstract_excerpt":"The radio galaxy 3C 84 is a representative of gamma-ray-bright misaligned active galactic nuclei (AGNs) and one of the best laboratories to study the radio properties of the sub-pc jet in connection with the gamma-ray emission. In order to identify possible radio counterparts of the gamma-ray emissions in 3C 84, we study the change in structure within the central 1 pc and the light curve of sub-pc-size components C1, C2, and C3. We search for any correlation between changes in the radio components and the gamma-ray flares by making use of VLBI and single dish data. Throughout the radio monitor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.1392","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":"1204.1392","created_at":"2026-05-18T01:57:56.287347+00:00"},{"alias_kind":"arxiv_version","alias_value":"1204.1392v1","created_at":"2026-05-18T01:57:56.287347+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.1392","created_at":"2026-05-18T01:57:56.287347+00:00"},{"alias_kind":"pith_short_12","alias_value":"47H6NYHVLCC6","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_16","alias_value":"47H6NYHVLCC6CQR7","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_8","alias_value":"47H6NYHV","created_at":"2026-05-18T12:26:53.410803+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/47H6NYHVLCC6CQR7XUPBQIPZV3","json":"https://pith.science/pith/47H6NYHVLCC6CQR7XUPBQIPZV3.json","graph_json":"https://pith.science/api/pith-number/47H6NYHVLCC6CQR7XUPBQIPZV3/graph.json","events_json":"https://pith.science/api/pith-number/47H6NYHVLCC6CQR7XUPBQIPZV3/events.json","paper":"https://pith.science/paper/47H6NYHV"},"agent_actions":{"view_html":"https://pith.science/pith/47H6NYHVLCC6CQR7XUPBQIPZV3","download_json":"https://pith.science/pith/47H6NYHVLCC6CQR7XUPBQIPZV3.json","view_paper":"https://pith.science/paper/47H6NYHV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1204.1392&json=true","fetch_graph":"https://pith.science/api/pith-number/47H6NYHVLCC6CQR7XUPBQIPZV3/graph.json","fetch_events":"https://pith.science/api/pith-number/47H6NYHVLCC6CQR7XUPBQIPZV3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/47H6NYHVLCC6CQR7XUPBQIPZV3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/47H6NYHVLCC6CQR7XUPBQIPZV3/action/storage_attestation","attest_author":"https://pith.science/pith/47H6NYHVLCC6CQR7XUPBQIPZV3/action/author_attestation","sign_citation":"https://pith.science/pith/47H6NYHVLCC6CQR7XUPBQIPZV3/action/citation_signature","submit_replication":"https://pith.science/pith/47H6NYHVLCC6CQR7XUPBQIPZV3/action/replication_record"}},"created_at":"2026-05-18T01:57:56.287347+00:00","updated_at":"2026-05-18T01:57:56.287347+00:00"}