{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:XXRARLOZSB5C632BEXFUGJ7NG3","short_pith_number":"pith:XXRARLOZ","schema_version":"1.0","canonical_sha256":"bde208add9907a2f6f4125cb4327ed36f55189ec94bf4e665df62be19f9071ff","source":{"kind":"arxiv","id":"1610.08981","version":2},"attestation_state":"computed","paper":{"title":"One Law To Rule Them All: The Radial Acceleration Relation of Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"2), (2) European Southern Observatory, (3) University of Oregon, 4) ((1) Case Western Reserve University, (4) University of California, Federico Lelli (1, Irvine), James M. Schombert (3), Marcel S. Pawlowski (1, Stacy S. McGaugh (1)","submitted_at":"2016-10-27T20:00:02Z","abstract_excerpt":"We study the link between baryons and dark matter in 240 galaxies with spatially resolved kinematic data. Our sample spans 9 dex in stellar mass and includes all morphological types. We consider (i) 153 late-type galaxies (LTGs; spirals and irregulars) with gas rotation curves from the SPARC database; (ii) 25 early-type galaxies (ETGs; ellipticals and lenticulars) with stellar and HI data from ATLAS^3D or X-ray data from Chandra; and (iii) 62 dwarf spheroidals (dSphs) with individual-star spectroscopy. We find that LTGs, ETGs, and \"classical\" dSphs follow the same radial acceleration relation:"},"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":"1610.08981","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-10-27T20:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"8a0d265562ee2ccbf292bad64eeab5e0993b2aa0f30e0a0b96eef7491cf2b5ec","abstract_canon_sha256":"060b5a4c12c23a4496706db247c6063bf229a852718770bfe40a9e87ba5feaf8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:50:18.404028Z","signature_b64":"iemNyNHfY2ISwiYl0BmgONT26KerVRzRykpGlOvcMIjC7XrYn8lldIMeTr7zbHssubg50/GJDjJU/9Yc85qjAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bde208add9907a2f6f4125cb4327ed36f55189ec94bf4e665df62be19f9071ff","last_reissued_at":"2026-05-18T00:50:18.403373Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:50:18.403373Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"One Law To Rule Them All: The Radial Acceleration Relation of Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"2), (2) European Southern Observatory, (3) University of Oregon, 4) ((1) Case Western Reserve University, (4) University of California, Federico Lelli (1, Irvine), James M. Schombert (3), Marcel S. Pawlowski (1, Stacy S. McGaugh (1)","submitted_at":"2016-10-27T20:00:02Z","abstract_excerpt":"We study the link between baryons and dark matter in 240 galaxies with spatially resolved kinematic data. Our sample spans 9 dex in stellar mass and includes all morphological types. We consider (i) 153 late-type galaxies (LTGs; spirals and irregulars) with gas rotation curves from the SPARC database; (ii) 25 early-type galaxies (ETGs; ellipticals and lenticulars) with stellar and HI data from ATLAS^3D or X-ray data from Chandra; and (iii) 62 dwarf spheroidals (dSphs) with individual-star spectroscopy. We find that LTGs, ETGs, and \"classical\" dSphs follow the same radial acceleration relation:"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.08981","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":""},"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":"1610.08981","created_at":"2026-05-18T00:50:18.403453+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.08981v2","created_at":"2026-05-18T00:50:18.403453+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.08981","created_at":"2026-05-18T00:50:18.403453+00:00"},{"alias_kind":"pith_short_12","alias_value":"XXRARLOZSB5C","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_16","alias_value":"XXRARLOZSB5C632B","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_8","alias_value":"XXRARLOZ","created_at":"2026-05-18T12:30:51.357362+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"1906.09798","citing_title":"Investigating Dark Matter and MOND Models with Galactic Rotation Curve Data: Analysing the Gas-Dominated Galaxies","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2512.10513","citing_title":"A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems","ref_index":37,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3","json":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3.json","graph_json":"https://pith.science/api/pith-number/XXRARLOZSB5C632BEXFUGJ7NG3/graph.json","events_json":"https://pith.science/api/pith-number/XXRARLOZSB5C632BEXFUGJ7NG3/events.json","paper":"https://pith.science/paper/XXRARLOZ"},"agent_actions":{"view_html":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3","download_json":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3.json","view_paper":"https://pith.science/paper/XXRARLOZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.08981&json=true","fetch_graph":"https://pith.science/api/pith-number/XXRARLOZSB5C632BEXFUGJ7NG3/graph.json","fetch_events":"https://pith.science/api/pith-number/XXRARLOZSB5C632BEXFUGJ7NG3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3/action/storage_attestation","attest_author":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3/action/author_attestation","sign_citation":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3/action/citation_signature","submit_replication":"https://pith.science/pith/XXRARLOZSB5C632BEXFUGJ7NG3/action/replication_record"}},"created_at":"2026-05-18T00:50:18.403453+00:00","updated_at":"2026-05-18T00:50:18.403453+00:00"}