{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:SPH7WJ5O2EQJJQ5N2SBSV73ON2","short_pith_number":"pith:SPH7WJ5O","schema_version":"1.0","canonical_sha256":"93cffb27aed12094c3add4832aff6e6e981dbe35a2ac140df9cf66e2008ccb1f","source":{"kind":"arxiv","id":"2312.14702","version":2},"attestation_state":"computed","paper":{"title":"The ALMaQUEST Survey XIV: do radial molecular gas flows affect the star-forming ability of barred galaxies?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Am\\'elie Saintonge, Carlos L\\'opez-Cob\\'a, Hsi-An Pan, Lihwai Lin, Lucy M. Hogarth, Mallory D. Thorp, Sara L. Ellison, Tim A. Davis","submitted_at":"2023-12-22T14:03:29Z","abstract_excerpt":"We investigate whether barred galaxies are statistically more likely to harbour radial molecular gas flows and what effect those flows have on their global properties. Using 46 galaxies from the ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey, we identify galaxies hosting optical bars using a combination of the morphological classifications in Galaxy Zoo 2 and HyperLEDA. In order to detect radial molecular gas flows, we employ full 3D kinematic modelling of the ALMaQUEST CO(1-0) datacubes. By combining our bar classifications with our radial bar-driven flow detections, we find that "},"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":"2312.14702","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-12-22T14:03:29Z","cross_cats_sorted":[],"title_canon_sha256":"9500e8749b0805468b9a2c6d28bbcaf105fedf3e3c3a3b5f43391d9add711584","abstract_canon_sha256":"2ec81ee6c7717200549db2d722cac5f94bbc442e4b4231d3c46dd327be8bb731"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:48:02.097190Z","signature_b64":"OYyw9mB2djSjIu9Bud5Xy/s2vnxT0UsISbZDD1YGgqQ251CCStG9ayVXPhS9vS6xVV3FFuhQtqivVe/glSy9DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"93cffb27aed12094c3add4832aff6e6e981dbe35a2ac140df9cf66e2008ccb1f","last_reissued_at":"2026-07-05T07:48:02.096756Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:48:02.096756Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The ALMaQUEST Survey XIV: do radial molecular gas flows affect the star-forming ability of barred galaxies?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Am\\'elie Saintonge, Carlos L\\'opez-Cob\\'a, Hsi-An Pan, Lihwai Lin, Lucy M. Hogarth, Mallory D. Thorp, Sara L. Ellison, Tim A. Davis","submitted_at":"2023-12-22T14:03:29Z","abstract_excerpt":"We investigate whether barred galaxies are statistically more likely to harbour radial molecular gas flows and what effect those flows have on their global properties. Using 46 galaxies from the ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey, we identify galaxies hosting optical bars using a combination of the morphological classifications in Galaxy Zoo 2 and HyperLEDA. In order to detect radial molecular gas flows, we employ full 3D kinematic modelling of the ALMaQUEST CO(1-0) datacubes. By combining our bar classifications with our radial bar-driven flow detections, we find that "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.14702","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2312.14702/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":"2312.14702","created_at":"2026-07-05T07:48:02.096819+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.14702v2","created_at":"2026-07-05T07:48:02.096819+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.14702","created_at":"2026-07-05T07:48:02.096819+00:00"},{"alias_kind":"pith_short_12","alias_value":"SPH7WJ5O2EQJ","created_at":"2026-07-05T07:48:02.096819+00:00"},{"alias_kind":"pith_short_16","alias_value":"SPH7WJ5O2EQJJQ5N","created_at":"2026-07-05T07:48:02.096819+00:00"},{"alias_kind":"pith_short_8","alias_value":"SPH7WJ5O","created_at":"2026-07-05T07:48:02.096819+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/SPH7WJ5O2EQJJQ5N2SBSV73ON2","json":"https://pith.science/pith/SPH7WJ5O2EQJJQ5N2SBSV73ON2.json","graph_json":"https://pith.science/api/pith-number/SPH7WJ5O2EQJJQ5N2SBSV73ON2/graph.json","events_json":"https://pith.science/api/pith-number/SPH7WJ5O2EQJJQ5N2SBSV73ON2/events.json","paper":"https://pith.science/paper/SPH7WJ5O"},"agent_actions":{"view_html":"https://pith.science/pith/SPH7WJ5O2EQJJQ5N2SBSV73ON2","download_json":"https://pith.science/pith/SPH7WJ5O2EQJJQ5N2SBSV73ON2.json","view_paper":"https://pith.science/paper/SPH7WJ5O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.14702&json=true","fetch_graph":"https://pith.science/api/pith-number/SPH7WJ5O2EQJJQ5N2SBSV73ON2/graph.json","fetch_events":"https://pith.science/api/pith-number/SPH7WJ5O2EQJJQ5N2SBSV73ON2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SPH7WJ5O2EQJJQ5N2SBSV73ON2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SPH7WJ5O2EQJJQ5N2SBSV73ON2/action/storage_attestation","attest_author":"https://pith.science/pith/SPH7WJ5O2EQJJQ5N2SBSV73ON2/action/author_attestation","sign_citation":"https://pith.science/pith/SPH7WJ5O2EQJJQ5N2SBSV73ON2/action/citation_signature","submit_replication":"https://pith.science/pith/SPH7WJ5O2EQJJQ5N2SBSV73ON2/action/replication_record"}},"created_at":"2026-07-05T07:48:02.096819+00:00","updated_at":"2026-07-05T07:48:02.096819+00:00"}