{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:AQI6LCOSA72DIC552TABNEKI3T","short_pith_number":"pith:AQI6LCOS","schema_version":"1.0","canonical_sha256":"0411e589d207f4340bbdd4c0169148dcf1f26689f055d5c54fb7423067675dbb","source":{"kind":"arxiv","id":"1612.09566","version":2},"attestation_state":"computed","paper":{"title":"The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Alessandro Nagar, David Keitel, Enno Harms, Geraint Pratten, Lionel London, Mark Hannam, Michael P\\\"urrer, Sascha Husa, Sebastian Khan, Sebastiano Bernuzzi, Vivek Chaurasia, Xisco Jim\\'enez Forteza","submitted_at":"2016-12-30T19:29:07Z","abstract_excerpt":"For a brief moment, a binary black hole (BBH) merger can be the most powerful astrophysical event in the visible universe. Here we present a model fit for this gravitational-wave peak luminosity of nonprecessing quasicircular BBH systems as a function of the masses and spins of the component black holes, based on numerical relativity (NR) simulations and the hierarchical fitting approach introduced by X. Jim\\'enez-Forteza et al. [Phys. Rev. D 95, 064024 (2017), arXiv:1611.00332]. This fit improves over previous results in accuracy and parameter-space coverage and can be used to infer posterior"},"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":"1612.09566","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-12-30T19:29:07Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"b59ce5cb2a4c5b6eaa43de5cfaa27ca0a4bdbec83ac98da751d54356f36a48f6","abstract_canon_sha256":"7e8bace193f1a9d5b95dd86038eb564ddd643be2b201a4640c60b8453d0bb407"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:40:07.544275Z","signature_b64":"WXDTGJgpc5/JebsBxjuZsOIM6f6drbtjPwmKvzobX3WMJWE5lFtzcqhqgv2WpJPCKA9KtwBajxsnlMbL8y8tDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0411e589d207f4340bbdd4c0169148dcf1f26689f055d5c54fb7423067675dbb","last_reissued_at":"2026-05-18T00:40:07.543596Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:40:07.543596Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Alessandro Nagar, David Keitel, Enno Harms, Geraint Pratten, Lionel London, Mark Hannam, Michael P\\\"urrer, Sascha Husa, Sebastian Khan, Sebastiano Bernuzzi, Vivek Chaurasia, Xisco Jim\\'enez Forteza","submitted_at":"2016-12-30T19:29:07Z","abstract_excerpt":"For a brief moment, a binary black hole (BBH) merger can be the most powerful astrophysical event in the visible universe. Here we present a model fit for this gravitational-wave peak luminosity of nonprecessing quasicircular BBH systems as a function of the masses and spins of the component black holes, based on numerical relativity (NR) simulations and the hierarchical fitting approach introduced by X. Jim\\'enez-Forteza et al. [Phys. Rev. D 95, 064024 (2017), arXiv:1611.00332]. This fit improves over previous results in accuracy and parameter-space coverage and can be used to infer posterior"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.09566","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":"1612.09566","created_at":"2026-05-18T00:40:07.543703+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.09566v2","created_at":"2026-05-18T00:40:07.543703+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.09566","created_at":"2026-05-18T00:40:07.543703+00:00"},{"alias_kind":"pith_short_12","alias_value":"AQI6LCOSA72D","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"AQI6LCOSA72DIC55","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"AQI6LCOS","created_at":"2026-05-18T12:30:07.202191+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2108.01045","citing_title":"GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","ref_index":150,"is_internal_anchor":true},{"citing_arxiv_id":"2004.06503","citing_title":"Computationally efficient models for the dominant and sub-dominant harmonic modes of precessing binary black holes","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2010.14527","citing_title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","ref_index":185,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T","json":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T.json","graph_json":"https://pith.science/api/pith-number/AQI6LCOSA72DIC552TABNEKI3T/graph.json","events_json":"https://pith.science/api/pith-number/AQI6LCOSA72DIC552TABNEKI3T/events.json","paper":"https://pith.science/paper/AQI6LCOS"},"agent_actions":{"view_html":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T","download_json":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T.json","view_paper":"https://pith.science/paper/AQI6LCOS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.09566&json=true","fetch_graph":"https://pith.science/api/pith-number/AQI6LCOSA72DIC552TABNEKI3T/graph.json","fetch_events":"https://pith.science/api/pith-number/AQI6LCOSA72DIC552TABNEKI3T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T/action/storage_attestation","attest_author":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T/action/author_attestation","sign_citation":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T/action/citation_signature","submit_replication":"https://pith.science/pith/AQI6LCOSA72DIC552TABNEKI3T/action/replication_record"}},"created_at":"2026-05-18T00:40:07.543703+00:00","updated_at":"2026-05-18T00:40:07.543703+00:00"}