{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:FENSTUK3LRPF66IMDNTJPFFESM","short_pith_number":"pith:FENSTUK3","schema_version":"1.0","canonical_sha256":"291b29d15b5c5e5f790c1b669794a4931b6a19b42fd1a826e61461a903e92f0c","source":{"kind":"arxiv","id":"1305.7353","version":1},"attestation_state":"computed","paper":{"title":"The quenching of star formation in accretion-driven clumpy turbulent tori of active galactic nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Max Planck Insitut fuer extraterrestrische Physik, B. Vollmer (1), France, Garching, Germany), Observatoire astronomique de Strasbourg, R.I. Davies (2) ((1) CDS","submitted_at":"2013-05-31T10:58:50Z","abstract_excerpt":"Galactic gas-gas collisions involving a turbulent multiphase ISM share common ISM properties: dense extraplanar gas visible in CO, large linewidths (>= 50 km/s), strong mid-infrared H_2 line emission, low star formation activity, and strong radio continuum emission. Gas-gas collisions can occur in the form of ICM ram pressure stripping, galaxy head-on collisions, compression of the intragroup gas and/or galaxy ISM by an intruder galaxy which flies through the galaxy group at a high velocity, or external gas accretion on an existing gas torus in a galactic center. We suggest that the common the"},"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":"1305.7353","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-05-31T10:58:50Z","cross_cats_sorted":[],"title_canon_sha256":"4e2292958047c53f54de3abfd471f395c1886e9e0f27c7dd33ab8b35e3c580fd","abstract_canon_sha256":"d7a100c5b3b03a31f3df60bfcc71cd34c085d7c1d318f7b59bd5a4289571cf2b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:39.265756Z","signature_b64":"RvjCRmXUjXG+NuxXMqj9J/98pJCvc58sbomJH9lM0FhrW7Ec8NdG2JAL4emELaM+17zmdmNVnFfQzV7zxcrfBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"291b29d15b5c5e5f790c1b669794a4931b6a19b42fd1a826e61461a903e92f0c","last_reissued_at":"2026-05-18T01:49:39.265217Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:39.265217Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The quenching of star formation in accretion-driven clumpy turbulent tori of active galactic nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Max Planck Insitut fuer extraterrestrische Physik, B. Vollmer (1), France, Garching, Germany), Observatoire astronomique de Strasbourg, R.I. Davies (2) ((1) CDS","submitted_at":"2013-05-31T10:58:50Z","abstract_excerpt":"Galactic gas-gas collisions involving a turbulent multiphase ISM share common ISM properties: dense extraplanar gas visible in CO, large linewidths (>= 50 km/s), strong mid-infrared H_2 line emission, low star formation activity, and strong radio continuum emission. Gas-gas collisions can occur in the form of ICM ram pressure stripping, galaxy head-on collisions, compression of the intragroup gas and/or galaxy ISM by an intruder galaxy which flies through the galaxy group at a high velocity, or external gas accretion on an existing gas torus in a galactic center. We suggest that the common the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.7353","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":"1305.7353","created_at":"2026-05-18T01:49:39.265301+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.7353v1","created_at":"2026-05-18T01:49:39.265301+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.7353","created_at":"2026-05-18T01:49:39.265301+00:00"},{"alias_kind":"pith_short_12","alias_value":"FENSTUK3LRPF","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_16","alias_value":"FENSTUK3LRPF66IM","created_at":"2026-05-18T12:27:45.050594+00:00"},{"alias_kind":"pith_short_8","alias_value":"FENSTUK3","created_at":"2026-05-18T12:27:45.050594+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/FENSTUK3LRPF66IMDNTJPFFESM","json":"https://pith.science/pith/FENSTUK3LRPF66IMDNTJPFFESM.json","graph_json":"https://pith.science/api/pith-number/FENSTUK3LRPF66IMDNTJPFFESM/graph.json","events_json":"https://pith.science/api/pith-number/FENSTUK3LRPF66IMDNTJPFFESM/events.json","paper":"https://pith.science/paper/FENSTUK3"},"agent_actions":{"view_html":"https://pith.science/pith/FENSTUK3LRPF66IMDNTJPFFESM","download_json":"https://pith.science/pith/FENSTUK3LRPF66IMDNTJPFFESM.json","view_paper":"https://pith.science/paper/FENSTUK3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.7353&json=true","fetch_graph":"https://pith.science/api/pith-number/FENSTUK3LRPF66IMDNTJPFFESM/graph.json","fetch_events":"https://pith.science/api/pith-number/FENSTUK3LRPF66IMDNTJPFFESM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FENSTUK3LRPF66IMDNTJPFFESM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FENSTUK3LRPF66IMDNTJPFFESM/action/storage_attestation","attest_author":"https://pith.science/pith/FENSTUK3LRPF66IMDNTJPFFESM/action/author_attestation","sign_citation":"https://pith.science/pith/FENSTUK3LRPF66IMDNTJPFFESM/action/citation_signature","submit_replication":"https://pith.science/pith/FENSTUK3LRPF66IMDNTJPFFESM/action/replication_record"}},"created_at":"2026-05-18T01:49:39.265301+00:00","updated_at":"2026-05-18T01:49:39.265301+00:00"}