{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:XNSB5HTEQS6WKBO2R3UR62NX4T","short_pith_number":"pith:XNSB5HTE","schema_version":"1.0","canonical_sha256":"bb641e9e6484bd6505da8ee91f69b7e4d8332d0d01e0e5a9087b9e66a2a97a4e","source":{"kind":"arxiv","id":"2502.03929","version":2},"attestation_state":"computed","paper":{"title":"Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Geraint Pratten, Gonzalo Morras, Patricia Schmidt","submitted_at":"2025-02-06T10:09:38Z","abstract_excerpt":"The measurement of spin-precession and orbital eccentricity in gravitational-wave (GW) signals is a key priority in GW astronomy, as these effects not only provide insights into the astrophysical formation and evolution of compact binaries but also, if neglected, could introduce significant biases in parameter estimation, searches, and tests of General Relativity. Despite the growing potential of upcoming LIGO-Virgo-KAGRA observing runs and future detectors to measure eccentric-precessing signals, accurately and efficiently modeling them remains a challenge. In this work, we present pyEFPE, a "},"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":"2502.03929","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-02-06T10:09:38Z","cross_cats_sorted":["astro-ph.HE","astro-ph.IM"],"title_canon_sha256":"a8abe9c9f10157087231bf45f2969dbb18dd05ff61bc46b4eda85e90a40b3167","abstract_canon_sha256":"a0bb8a5ae5410e395e0b07498658363dbd588f4cad7c290c157630c835e99ad3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:51:05.246433Z","signature_b64":"v3DzjgbS2JfOycVHfufUW3q/nmVoR5ec/mtr3rIyMvchX0rI6I/ZEuC7rPzJ6PsR0H0IpmH2IdYrXjrSI1/YBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bb641e9e6484bd6505da8ee91f69b7e4d8332d0d01e0e5a9087b9e66a2a97a4e","last_reissued_at":"2026-07-05T10:51:05.245964Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:51:05.245964Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Geraint Pratten, Gonzalo Morras, Patricia Schmidt","submitted_at":"2025-02-06T10:09:38Z","abstract_excerpt":"The measurement of spin-precession and orbital eccentricity in gravitational-wave (GW) signals is a key priority in GW astronomy, as these effects not only provide insights into the astrophysical formation and evolution of compact binaries but also, if neglected, could introduce significant biases in parameter estimation, searches, and tests of General Relativity. Despite the growing potential of upcoming LIGO-Virgo-KAGRA observing runs and future detectors to measure eccentric-precessing signals, accurately and efficiently modeling them remains a challenge. In this work, we present pyEFPE, a "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.03929","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2502.03929/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":"2502.03929","created_at":"2026-07-05T10:51:05.246020+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.03929v2","created_at":"2026-07-05T10:51:05.246020+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.03929","created_at":"2026-07-05T10:51:05.246020+00:00"},{"alias_kind":"pith_short_12","alias_value":"XNSB5HTEQS6W","created_at":"2026-07-05T10:51:05.246020+00:00"},{"alias_kind":"pith_short_16","alias_value":"XNSB5HTEQS6WKBO2","created_at":"2026-07-05T10:51:05.246020+00:00"},{"alias_kind":"pith_short_8","alias_value":"XNSB5HTE","created_at":"2026-07-05T10:51:05.246020+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":14,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.11705","citing_title":"Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis","ref_index":104,"is_internal_anchor":false},{"citing_arxiv_id":"2606.08838","citing_title":"Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2606.02690","citing_title":"Speed and accuracy for long signals: Frequency-domain effective-one-body waveforms for compact binary coalescences","ref_index":116,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28156","citing_title":"Joint inference of line-of-sight acceleration and orbital eccentricity in neutron-star--black-hole binaries","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2606.30594","citing_title":"Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations","ref_index":46,"is_internal_anchor":false},{"citing_arxiv_id":"2605.28716","citing_title":"Eccentric and unbound compact binaries in the LIGO-Virgo-KAGRA catalog: parameter estimation and waveform systematics with SEOBNRv6EHM","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2605.28715","citing_title":"Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM","ref_index":182,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18742","citing_title":"A universal framework to identify eccentric binary mergers: GW200105 case study","ref_index":36,"is_internal_anchor":false},{"citing_arxiv_id":"2512.10803","citing_title":"Detection of GW200105 with a targeted eccentric search","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2603.20031","citing_title":"Analytical Solution of Spinning, Eccentric Binary Black Hole Dynamics at the Second Post-Newtonian Order","ref_index":30,"is_internal_anchor":false},{"citing_arxiv_id":"2605.12818","citing_title":"Assessing the imprint of eccentricity in GW signatures using two independent waveform models","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14270","citing_title":"Fast neural network surrogate for multimodal effective-one-body gravitational waveforms from generically precessing compact binaries","ref_index":126,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11903","citing_title":"Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17868","citing_title":"Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions","ref_index":67,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T","json":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T.json","graph_json":"https://pith.science/api/pith-number/XNSB5HTEQS6WKBO2R3UR62NX4T/graph.json","events_json":"https://pith.science/api/pith-number/XNSB5HTEQS6WKBO2R3UR62NX4T/events.json","paper":"https://pith.science/paper/XNSB5HTE"},"agent_actions":{"view_html":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T","download_json":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T.json","view_paper":"https://pith.science/paper/XNSB5HTE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.03929&json=true","fetch_graph":"https://pith.science/api/pith-number/XNSB5HTEQS6WKBO2R3UR62NX4T/graph.json","fetch_events":"https://pith.science/api/pith-number/XNSB5HTEQS6WKBO2R3UR62NX4T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T/action/storage_attestation","attest_author":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T/action/author_attestation","sign_citation":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T/action/citation_signature","submit_replication":"https://pith.science/pith/XNSB5HTEQS6WKBO2R3UR62NX4T/action/replication_record"}},"created_at":"2026-07-05T10:51:05.246020+00:00","updated_at":"2026-07-05T10:51:05.246020+00:00"}