{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:E3POAH5NROXXQSCDLKF6KNVQZU","short_pith_number":"pith:E3POAH5N","schema_version":"1.0","canonical_sha256":"26dee01fad8baf7848435a8be536b0cd35ee43f08309a2de3b0fb4cc8f1c39a5","source":{"kind":"arxiv","id":"astro-ph/0201276","version":1},"attestation_state":"computed","paper":{"title":"H alpha rotation curves of Low Surface Brightness galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Bosma (2) ((1) ATNF, Australia (2) Observatoire de Marseille, France), Sydney, W.J.G. de Blok (1)","submitted_at":"2002-01-16T23:48:29Z","abstract_excerpt":"We present high-resolution rotation curves of a sample of 26 low surface brightness galaxies. From these curves we derive mass distributions using a variety of assumptions for the stellar mass-to-light ratio. We show that the predictions of current Cold Dark Matter models for the density profiles of dark matter halos are inconsistent with the observed curves. The latter indicate a core-dominated structure, rather than the theoretically preferred cuspy structure."},"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/0201276","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2002-01-16T23:48:29Z","cross_cats_sorted":[],"title_canon_sha256":"6299fdef477b8341b5b6a241ee0dd661591f3ff6ef1cf5a3915090521108a8e3","abstract_canon_sha256":"755553d75f0c727c7c0bb7d45ca6c116aaadfee225a54471c1565a585c59da74"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:22:56.940115Z","signature_b64":"VcxrJRjfWVfPXrMy0aCHN5Xjn9LhAQiedCX5IIqesrXppNzwocxGK6Z0h4wIK6VmG6NGwV5bsrSYmo03f/v/Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"26dee01fad8baf7848435a8be536b0cd35ee43f08309a2de3b0fb4cc8f1c39a5","last_reissued_at":"2026-07-04T15:22:56.939693Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:22:56.939693Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"H alpha rotation curves of Low Surface Brightness galaxies","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Bosma (2) ((1) ATNF, Australia (2) Observatoire de Marseille, France), Sydney, W.J.G. de Blok (1)","submitted_at":"2002-01-16T23:48:29Z","abstract_excerpt":"We present high-resolution rotation curves of a sample of 26 low surface brightness galaxies. From these curves we derive mass distributions using a variety of assumptions for the stellar mass-to-light ratio. We show that the predictions of current Cold Dark Matter models for the density profiles of dark matter halos are inconsistent with the observed curves. The latter indicate a core-dominated structure, rather than the theoretically preferred cuspy structure."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0201276","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/0201276/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/0201276","created_at":"2026-07-04T15:22:56.939752+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0201276v1","created_at":"2026-07-04T15:22:56.939752+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0201276","created_at":"2026-07-04T15:22:56.939752+00:00"},{"alias_kind":"pith_short_12","alias_value":"E3POAH5NROXX","created_at":"2026-07-04T15:22:56.939752+00:00"},{"alias_kind":"pith_short_16","alias_value":"E3POAH5NROXXQSCD","created_at":"2026-07-04T15:22:56.939752+00:00"},{"alias_kind":"pith_short_8","alias_value":"E3POAH5N","created_at":"2026-07-04T15:22:56.939752+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.19371","citing_title":"Velocity-dependent self-interacting dark matter and composite Higgs","ref_index":6,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU","json":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU.json","graph_json":"https://pith.science/api/pith-number/E3POAH5NROXXQSCDLKF6KNVQZU/graph.json","events_json":"https://pith.science/api/pith-number/E3POAH5NROXXQSCDLKF6KNVQZU/events.json","paper":"https://pith.science/paper/E3POAH5N"},"agent_actions":{"view_html":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU","download_json":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU.json","view_paper":"https://pith.science/paper/E3POAH5N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0201276&json=true","fetch_graph":"https://pith.science/api/pith-number/E3POAH5NROXXQSCDLKF6KNVQZU/graph.json","fetch_events":"https://pith.science/api/pith-number/E3POAH5NROXXQSCDLKF6KNVQZU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU/action/storage_attestation","attest_author":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU/action/author_attestation","sign_citation":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU/action/citation_signature","submit_replication":"https://pith.science/pith/E3POAH5NROXXQSCDLKF6KNVQZU/action/replication_record"}},"created_at":"2026-07-04T15:22:56.939752+00:00","updated_at":"2026-07-04T15:22:56.939752+00:00"}