{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:K3DQQSW5G6MYC5FX2TZRVW6D6R","short_pith_number":"pith:K3DQQSW5","schema_version":"1.0","canonical_sha256":"56c7084add37998174b7d4f31adbc3f46470c1381f51d4fd466d85bfdabbdd83","source":{"kind":"arxiv","id":"1209.0512","version":1},"attestation_state":"computed","paper":{"title":"Fingerprints of the hierarchical building up of the structure on the gas kinematics of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"2, 2), 2) ((1) Consejo Nacional de Investigaciones Cientificas y Tecnicas, (2) Instituto de Astronomia y Fisica del Espacio, 3), (3) Facultad de Ciencias Exactas y Naturales, Argentina, Argentina), CONICET, IAFE, Maria E. De Rossi (1, Patricia B. Tissera (1, Susana E. Pedrosa (1, Universidad de Buenos Aires","submitted_at":"2012-09-04T02:11:40Z","abstract_excerpt":"Recent observational and theoretical works have suggested that the Tully-Fisher Relation might be generalised to include dispersion-dominated systems by combining the rotation and dispersion velocity in the definition of the kinematical indicator. Mergers and interactions have been pointed out as responsible of driving turbulent and disordered gas kinematics, which could generate Tully-Fisher Relation outliers. We intend to investigate the gas kinematics of galaxies by using a simulated sample which includes both, gas disc-dominated and spheroid-dominated systems. Cosmological hydrodynamical s"},"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":"1209.0512","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-09-04T02:11:40Z","cross_cats_sorted":[],"title_canon_sha256":"f0f6dd9f82bf321afd2b0ca01a71d5ff1cd5cd11f187b5c4f3de3755cc2d07b7","abstract_canon_sha256":"53b17dc86271148d1b5ef92743fbce634fdacdfd2a7c31f63440e14d0ff29618"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:47.730549Z","signature_b64":"YkCmZMLWmfpvCVFe+GcDfMDSG+QUV8igVy/5gf0DIUW5BREPo+YL/38L1FmuWOppD7QGa5jy4rAXJ3QGZN9fBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"56c7084add37998174b7d4f31adbc3f46470c1381f51d4fd466d85bfdabbdd83","last_reissued_at":"2026-05-18T01:54:47.729745Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:47.729745Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fingerprints of the hierarchical building up of the structure on the gas kinematics of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"2, 2), 2) ((1) Consejo Nacional de Investigaciones Cientificas y Tecnicas, (2) Instituto de Astronomia y Fisica del Espacio, 3), (3) Facultad de Ciencias Exactas y Naturales, Argentina, Argentina), CONICET, IAFE, Maria E. De Rossi (1, Patricia B. Tissera (1, Susana E. Pedrosa (1, Universidad de Buenos Aires","submitted_at":"2012-09-04T02:11:40Z","abstract_excerpt":"Recent observational and theoretical works have suggested that the Tully-Fisher Relation might be generalised to include dispersion-dominated systems by combining the rotation and dispersion velocity in the definition of the kinematical indicator. Mergers and interactions have been pointed out as responsible of driving turbulent and disordered gas kinematics, which could generate Tully-Fisher Relation outliers. We intend to investigate the gas kinematics of galaxies by using a simulated sample which includes both, gas disc-dominated and spheroid-dominated systems. Cosmological hydrodynamical s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1209.0512","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":"1209.0512","created_at":"2026-05-18T01:54:47.729849+00:00"},{"alias_kind":"arxiv_version","alias_value":"1209.0512v1","created_at":"2026-05-18T01:54:47.729849+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1209.0512","created_at":"2026-05-18T01:54:47.729849+00:00"},{"alias_kind":"pith_short_12","alias_value":"K3DQQSW5G6MY","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_16","alias_value":"K3DQQSW5G6MYC5FX","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_8","alias_value":"K3DQQSW5","created_at":"2026-05-18T12:27:11.947152+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/K3DQQSW5G6MYC5FX2TZRVW6D6R","json":"https://pith.science/pith/K3DQQSW5G6MYC5FX2TZRVW6D6R.json","graph_json":"https://pith.science/api/pith-number/K3DQQSW5G6MYC5FX2TZRVW6D6R/graph.json","events_json":"https://pith.science/api/pith-number/K3DQQSW5G6MYC5FX2TZRVW6D6R/events.json","paper":"https://pith.science/paper/K3DQQSW5"},"agent_actions":{"view_html":"https://pith.science/pith/K3DQQSW5G6MYC5FX2TZRVW6D6R","download_json":"https://pith.science/pith/K3DQQSW5G6MYC5FX2TZRVW6D6R.json","view_paper":"https://pith.science/paper/K3DQQSW5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1209.0512&json=true","fetch_graph":"https://pith.science/api/pith-number/K3DQQSW5G6MYC5FX2TZRVW6D6R/graph.json","fetch_events":"https://pith.science/api/pith-number/K3DQQSW5G6MYC5FX2TZRVW6D6R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K3DQQSW5G6MYC5FX2TZRVW6D6R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K3DQQSW5G6MYC5FX2TZRVW6D6R/action/storage_attestation","attest_author":"https://pith.science/pith/K3DQQSW5G6MYC5FX2TZRVW6D6R/action/author_attestation","sign_citation":"https://pith.science/pith/K3DQQSW5G6MYC5FX2TZRVW6D6R/action/citation_signature","submit_replication":"https://pith.science/pith/K3DQQSW5G6MYC5FX2TZRVW6D6R/action/replication_record"}},"created_at":"2026-05-18T01:54:47.729849+00:00","updated_at":"2026-05-18T01:54:47.729849+00:00"}