{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:IDHUYFGAIGAPGQCTAKCAWDNLIL","short_pith_number":"pith:IDHUYFGA","schema_version":"1.0","canonical_sha256":"40cf4c14c04180f3405302840b0dab42d95993f15bb1212863603a0cd1fb5128","source":{"kind":"arxiv","id":"2303.05419","version":1},"attestation_state":"computed","paper":{"title":"A catalogue of precessing black-hole-binary numerical-relativity simulations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alex Vano-Vinuales, Charlie Hoy, Chinmay Kalaghatgi, Dave Yeeles, Edward Fauchon-Jones, Eleanor Hamilton, Jonathan E. Thompson, Lionel London, Mark Hannam, Panagiota Kolitsidou, Sebastian Khan, Shrobana Ghosh","submitted_at":"2023-03-09T17:09:43Z","abstract_excerpt":"We present a public catalogue of numerical-relativity binary-black-hole simulations. The catalogue contains datasets from 80 distinct configurations of precessing binary-black-hole systems, with mass ratios up to $m_2/m_1 = 8$, dimensionless spin magnitudes on the larger black hole up to $|\\vec{S}_2|/m_2^2 = 0.8$ (the small black hole is non-spinning), and a range of five values of spin misalignment for each mass-ratio/spin combination. We discuss the physical properties of the configurations in our catalogue, and assess the accuracy of the initial configuration of each simulation and of the g"},"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":"2303.05419","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-03-09T17:09:43Z","cross_cats_sorted":[],"title_canon_sha256":"a8c676c470af38883bbaca4b83dbb023fdb1bfd10123aa964ba9aecd2e50de2c","abstract_canon_sha256":"1beb745dd3927a2950c9ec5c78997abce077d36dae6c283929ab05f3e175afb3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:53:53.233568Z","signature_b64":"jE0vcUh7zVP6PPyYlQJrXTgkylkvKx2g9E9BSuAmLzgjjDYoeydggNCxSkAf8OfkRKeynTrqsocBRygtTdACAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40cf4c14c04180f3405302840b0dab42d95993f15bb1212863603a0cd1fb5128","last_reissued_at":"2026-07-05T05:53:53.233114Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:53:53.233114Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A catalogue of precessing black-hole-binary numerical-relativity simulations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alex Vano-Vinuales, Charlie Hoy, Chinmay Kalaghatgi, Dave Yeeles, Edward Fauchon-Jones, Eleanor Hamilton, Jonathan E. Thompson, Lionel London, Mark Hannam, Panagiota Kolitsidou, Sebastian Khan, Shrobana Ghosh","submitted_at":"2023-03-09T17:09:43Z","abstract_excerpt":"We present a public catalogue of numerical-relativity binary-black-hole simulations. The catalogue contains datasets from 80 distinct configurations of precessing binary-black-hole systems, with mass ratios up to $m_2/m_1 = 8$, dimensionless spin magnitudes on the larger black hole up to $|\\vec{S}_2|/m_2^2 = 0.8$ (the small black hole is non-spinning), and a range of five values of spin misalignment for each mass-ratio/spin combination. We discuss the physical properties of the configurations in our catalogue, and assess the accuracy of the initial configuration of each simulation and of the g"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.05419","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/2303.05419/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":"2303.05419","created_at":"2026-07-05T05:53:53.233171+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.05419v1","created_at":"2026-07-05T05:53:53.233171+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.05419","created_at":"2026-07-05T05:53:53.233171+00:00"},{"alias_kind":"pith_short_12","alias_value":"IDHUYFGAIGAP","created_at":"2026-07-05T05:53:53.233171+00:00"},{"alias_kind":"pith_short_16","alias_value":"IDHUYFGAIGAPGQCT","created_at":"2026-07-05T05:53:53.233171+00:00"},{"alias_kind":"pith_short_8","alias_value":"IDHUYFGA","created_at":"2026-07-05T05:53:53.233171+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2510.16113","citing_title":"Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary","ref_index":159,"is_internal_anchor":false},{"citing_arxiv_id":"2601.23019","citing_title":"Toward claiming a detection of gravitational memory","ref_index":178,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL","json":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL.json","graph_json":"https://pith.science/api/pith-number/IDHUYFGAIGAPGQCTAKCAWDNLIL/graph.json","events_json":"https://pith.science/api/pith-number/IDHUYFGAIGAPGQCTAKCAWDNLIL/events.json","paper":"https://pith.science/paper/IDHUYFGA"},"agent_actions":{"view_html":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL","download_json":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL.json","view_paper":"https://pith.science/paper/IDHUYFGA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.05419&json=true","fetch_graph":"https://pith.science/api/pith-number/IDHUYFGAIGAPGQCTAKCAWDNLIL/graph.json","fetch_events":"https://pith.science/api/pith-number/IDHUYFGAIGAPGQCTAKCAWDNLIL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL/action/storage_attestation","attest_author":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL/action/author_attestation","sign_citation":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL/action/citation_signature","submit_replication":"https://pith.science/pith/IDHUYFGAIGAPGQCTAKCAWDNLIL/action/replication_record"}},"created_at":"2026-07-05T05:53:53.233171+00:00","updated_at":"2026-07-05T05:53:53.233171+00:00"}