{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:K2OVEV76OOOOF5APHC5YZH2UE6","short_pith_number":"pith:K2OVEV76","schema_version":"1.0","canonical_sha256":"569d5257fe739ce2f40f38bb8c9f5427a78da8e06b8e533f19e330e8d8739410","source":{"kind":"arxiv","id":"astro-ph/0102420","version":1},"attestation_state":"computed","paper":{"title":"Kinematics of Molecular Gas in the Nucleus of NGC1068, from H2 line emission observed with VLT","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Franceschini, D. Alloin, D. Rouan, E. Galliano, G.L. Granato, J.G. Cuby, O. Marco, Y. Clenet","submitted_at":"2001-02-23T21:33:23Z","abstract_excerpt":"We present results about the distribution and kinematics of the molecular environment of the AGN in NGC1068, over a 1.5'' x 3.5'' region around the central engine in NGC1068, derived from H2 line emission detected with ISAAC at VLT/ANTU on ESO/Paranal. The H2 emitting molecular gas is found to be distributed along the East-West direction and with two main peak emission (knots) located at a distance of about 70 pc from the central engine. The eastern H2 knot is more intense than the western one. The line profiles mapped across the entire 1.5'' x 3.5'' region, at a spatial resolution of 0.3'' x "},"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":"astro-ph/0102420","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-02-23T21:33:23Z","cross_cats_sorted":[],"title_canon_sha256":"de65d262eb025dfb6002d1489572b6bc9b1460a68463615ea045466f832ab819","abstract_canon_sha256":"459f63603174bdf789ffbccc800ac8bf495d4456c477e6ba23a888bbe8b9ce62"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:22:46.661550Z","signature_b64":"lhIMCF3t4nJduUUmcroN/sb6/KPnI9iy31tmjkBccbE7Ud5SRilcKOIWauvqfjBYSTlh1oRmpQzkPybXSKX/DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"569d5257fe739ce2f40f38bb8c9f5427a78da8e06b8e533f19e330e8d8739410","last_reissued_at":"2026-07-04T16:22:46.661132Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:22:46.661132Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinematics of Molecular Gas in the Nucleus of NGC1068, from H2 line emission observed with VLT","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Franceschini, D. Alloin, D. Rouan, E. Galliano, G.L. Granato, J.G. Cuby, O. Marco, Y. Clenet","submitted_at":"2001-02-23T21:33:23Z","abstract_excerpt":"We present results about the distribution and kinematics of the molecular environment of the AGN in NGC1068, over a 1.5'' x 3.5'' region around the central engine in NGC1068, derived from H2 line emission detected with ISAAC at VLT/ANTU on ESO/Paranal. The H2 emitting molecular gas is found to be distributed along the East-West direction and with two main peak emission (knots) located at a distance of about 70 pc from the central engine. The eastern H2 knot is more intense than the western one. The line profiles mapped across the entire 1.5'' x 3.5'' region, at a spatial resolution of 0.3'' x "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0102420","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0102420/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0102420","created_at":"2026-07-04T16:22:46.661192+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0102420v1","created_at":"2026-07-04T16:22:46.661192+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0102420","created_at":"2026-07-04T16:22:46.661192+00:00"},{"alias_kind":"pith_short_12","alias_value":"K2OVEV76OOOO","created_at":"2026-07-04T16:22:46.661192+00:00"},{"alias_kind":"pith_short_16","alias_value":"K2OVEV76OOOOF5AP","created_at":"2026-07-04T16:22:46.661192+00:00"},{"alias_kind":"pith_short_8","alias_value":"K2OVEV76","created_at":"2026-07-04T16:22:46.661192+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/K2OVEV76OOOOF5APHC5YZH2UE6","json":"https://pith.science/pith/K2OVEV76OOOOF5APHC5YZH2UE6.json","graph_json":"https://pith.science/api/pith-number/K2OVEV76OOOOF5APHC5YZH2UE6/graph.json","events_json":"https://pith.science/api/pith-number/K2OVEV76OOOOF5APHC5YZH2UE6/events.json","paper":"https://pith.science/paper/K2OVEV76"},"agent_actions":{"view_html":"https://pith.science/pith/K2OVEV76OOOOF5APHC5YZH2UE6","download_json":"https://pith.science/pith/K2OVEV76OOOOF5APHC5YZH2UE6.json","view_paper":"https://pith.science/paper/K2OVEV76","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0102420&json=true","fetch_graph":"https://pith.science/api/pith-number/K2OVEV76OOOOF5APHC5YZH2UE6/graph.json","fetch_events":"https://pith.science/api/pith-number/K2OVEV76OOOOF5APHC5YZH2UE6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K2OVEV76OOOOF5APHC5YZH2UE6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K2OVEV76OOOOF5APHC5YZH2UE6/action/storage_attestation","attest_author":"https://pith.science/pith/K2OVEV76OOOOF5APHC5YZH2UE6/action/author_attestation","sign_citation":"https://pith.science/pith/K2OVEV76OOOOF5APHC5YZH2UE6/action/citation_signature","submit_replication":"https://pith.science/pith/K2OVEV76OOOOF5APHC5YZH2UE6/action/replication_record"}},"created_at":"2026-07-04T16:22:46.661192+00:00","updated_at":"2026-07-04T16:22:46.661192+00:00"}