{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:NMWRWDI2GHG6K7ZWRLDDEGFIN3","short_pith_number":"pith:NMWRWDI2","schema_version":"1.0","canonical_sha256":"6b2d1b0d1a31cde57f368ac63218a86ee0bb5a837de7b0a6be96d1cf58eb0b93","source":{"kind":"arxiv","id":"1108.0925","version":1},"attestation_state":"computed","paper":{"title":"Gamma-ray emission region located in the parsec scale jet of OJ287","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Alan P. Marscher, Anne Lahteenmaki, Clemens Thum, Helmut Wiesemeyer, Ivan Agudo, Jochen Heidt, Jose L. Gomez, Mark Gurwell, Paul S. Smith, Svetlana G. Jorstad, Valeri M. Larionov","submitted_at":"2011-08-03T14:35:31Z","abstract_excerpt":"We report on the location of the gamma-ray emission region in flares of the BL Lacertae object OJ287 at >14pc from the central supermassive black hole. We employ data from multi-spectral range (total flux and linear polarization) monitoring programs combined with sequences of ultra-high-resolution 7mm VLBA images. The correlation between the brightest gamma-ray and mm flares is found to be statistically significant. The two gamma-ray peaks, detected by Fermi-LAT, that we report here happened at the rising phase of two exceptionally bright mm flares accompanied by sharp linear polarization peak"},"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":"1108.0925","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-08-03T14:35:31Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"7f6637d7305723a68cc3ba76317d018c122e84eb7d192d9bbe1b0ee904151d5e","abstract_canon_sha256":"b4a86aee57d3c4f25d2a80b400a8e58dcd0389099e6523a90caf8508b4c61113"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:03.357110Z","signature_b64":"UKuuEvR3izAWBauGLSgyjZyoroL695uaHPr76r8S/fCijXE87YyIW4nAkvVD6MjG/rraunas0vEr7wxcS9NiDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6b2d1b0d1a31cde57f368ac63218a86ee0bb5a837de7b0a6be96d1cf58eb0b93","last_reissued_at":"2026-05-18T02:01:03.356326Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:03.356326Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma-ray emission region located in the parsec scale jet of OJ287","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Alan P. Marscher, Anne Lahteenmaki, Clemens Thum, Helmut Wiesemeyer, Ivan Agudo, Jochen Heidt, Jose L. Gomez, Mark Gurwell, Paul S. Smith, Svetlana G. Jorstad, Valeri M. Larionov","submitted_at":"2011-08-03T14:35:31Z","abstract_excerpt":"We report on the location of the gamma-ray emission region in flares of the BL Lacertae object OJ287 at >14pc from the central supermassive black hole. We employ data from multi-spectral range (total flux and linear polarization) monitoring programs combined with sequences of ultra-high-resolution 7mm VLBA images. The correlation between the brightest gamma-ray and mm flares is found to be statistically significant. The two gamma-ray peaks, detected by Fermi-LAT, that we report here happened at the rising phase of two exceptionally bright mm flares accompanied by sharp linear polarization peak"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.0925","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":"1108.0925","created_at":"2026-05-18T02:01:03.356470+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.0925v1","created_at":"2026-05-18T02:01:03.356470+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.0925","created_at":"2026-05-18T02:01:03.356470+00:00"},{"alias_kind":"pith_short_12","alias_value":"NMWRWDI2GHG6","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_16","alias_value":"NMWRWDI2GHG6K7ZW","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_8","alias_value":"NMWRWDI2","created_at":"2026-05-18T12:26:37.096874+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/NMWRWDI2GHG6K7ZWRLDDEGFIN3","json":"https://pith.science/pith/NMWRWDI2GHG6K7ZWRLDDEGFIN3.json","graph_json":"https://pith.science/api/pith-number/NMWRWDI2GHG6K7ZWRLDDEGFIN3/graph.json","events_json":"https://pith.science/api/pith-number/NMWRWDI2GHG6K7ZWRLDDEGFIN3/events.json","paper":"https://pith.science/paper/NMWRWDI2"},"agent_actions":{"view_html":"https://pith.science/pith/NMWRWDI2GHG6K7ZWRLDDEGFIN3","download_json":"https://pith.science/pith/NMWRWDI2GHG6K7ZWRLDDEGFIN3.json","view_paper":"https://pith.science/paper/NMWRWDI2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.0925&json=true","fetch_graph":"https://pith.science/api/pith-number/NMWRWDI2GHG6K7ZWRLDDEGFIN3/graph.json","fetch_events":"https://pith.science/api/pith-number/NMWRWDI2GHG6K7ZWRLDDEGFIN3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NMWRWDI2GHG6K7ZWRLDDEGFIN3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NMWRWDI2GHG6K7ZWRLDDEGFIN3/action/storage_attestation","attest_author":"https://pith.science/pith/NMWRWDI2GHG6K7ZWRLDDEGFIN3/action/author_attestation","sign_citation":"https://pith.science/pith/NMWRWDI2GHG6K7ZWRLDDEGFIN3/action/citation_signature","submit_replication":"https://pith.science/pith/NMWRWDI2GHG6K7ZWRLDDEGFIN3/action/replication_record"}},"created_at":"2026-05-18T02:01:03.356470+00:00","updated_at":"2026-05-18T02:01:03.356470+00:00"}