{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:PD4HLFRDUC4K4HW7UYXNGYTVNO","short_pith_number":"pith:PD4HLFRD","schema_version":"1.0","canonical_sha256":"78f8759623a0b8ae1edfa62ed362756ba8734b2c7f6ce542a2ab6b88ec35a275","source":{"kind":"arxiv","id":"0812.4208","version":4},"attestation_state":"computed","paper":{"title":"Influence of conservative corrections on parameter estimation for extreme-mass-ratio inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"E. A. Huerta, Jonathan R. Gair","submitted_at":"2008-12-22T14:58:36Z","abstract_excerpt":"We present an improved numerical kludge waveform model for circular, equatorial EMRIs. The model is based on true Kerr geodesics, augmented by radiative self-force corrections derived from perturbative calculations, and in this paper for the first time we include conservative self-force corrections that we derive by comparison to post-Newtonian results. We present results of a Monte Carlo simulation of parameter estimation errors computed using the Fisher Matrix and also assess the theoretical errors that would arise form omitting the conservative correction terms we include here. We present r"},"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":"0812.4208","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2008-12-22T14:58:36Z","cross_cats_sorted":[],"title_canon_sha256":"951ad781612a3b8fb2cc96eb31c795e831ccd38d02b8e48d01289218f4aabbc3","abstract_canon_sha256":"1a37df31878bc2e3b8a8a408601b9b061905332645553492ac0151068a202596"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:12:43.214904Z","signature_b64":"T6VH4iP0r5Uv3DMq2DBkFbMLAYynrfBvLkkR6eNqjdepCQmCvedjfxyGcm4s4x8n2ZKxdL4PA/HP/KeYKtW2Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"78f8759623a0b8ae1edfa62ed362756ba8734b2c7f6ce542a2ab6b88ec35a275","last_reissued_at":"2026-05-18T04:12:43.214329Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:12:43.214329Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Influence of conservative corrections on parameter estimation for extreme-mass-ratio inspirals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"E. A. Huerta, Jonathan R. Gair","submitted_at":"2008-12-22T14:58:36Z","abstract_excerpt":"We present an improved numerical kludge waveform model for circular, equatorial EMRIs. The model is based on true Kerr geodesics, augmented by radiative self-force corrections derived from perturbative calculations, and in this paper for the first time we include conservative self-force corrections that we derive by comparison to post-Newtonian results. We present results of a Monte Carlo simulation of parameter estimation errors computed using the Fisher Matrix and also assess the theoretical errors that would arise form omitting the conservative correction terms we include here. We present r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0812.4208","kind":"arxiv","version":4},"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":"0812.4208","created_at":"2026-05-18T04:12:43.214411+00:00"},{"alias_kind":"arxiv_version","alias_value":"0812.4208v4","created_at":"2026-05-18T04:12:43.214411+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0812.4208","created_at":"2026-05-18T04:12:43.214411+00:00"},{"alias_kind":"pith_short_12","alias_value":"PD4HLFRDUC4K","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_16","alias_value":"PD4HLFRDUC4K4HW7","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_8","alias_value":"PD4HLFRD","created_at":"2026-05-18T12:25:57.157939+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":83,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO","json":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO.json","graph_json":"https://pith.science/api/pith-number/PD4HLFRDUC4K4HW7UYXNGYTVNO/graph.json","events_json":"https://pith.science/api/pith-number/PD4HLFRDUC4K4HW7UYXNGYTVNO/events.json","paper":"https://pith.science/paper/PD4HLFRD"},"agent_actions":{"view_html":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO","download_json":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO.json","view_paper":"https://pith.science/paper/PD4HLFRD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0812.4208&json=true","fetch_graph":"https://pith.science/api/pith-number/PD4HLFRDUC4K4HW7UYXNGYTVNO/graph.json","fetch_events":"https://pith.science/api/pith-number/PD4HLFRDUC4K4HW7UYXNGYTVNO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO/action/storage_attestation","attest_author":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO/action/author_attestation","sign_citation":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO/action/citation_signature","submit_replication":"https://pith.science/pith/PD4HLFRDUC4K4HW7UYXNGYTVNO/action/replication_record"}},"created_at":"2026-05-18T04:12:43.214411+00:00","updated_at":"2026-05-18T04:12:43.214411+00:00"}