{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:D4V5UAGLEXJMBYTHAO33EFD42L","short_pith_number":"pith:D4V5UAGL","schema_version":"1.0","canonical_sha256":"1f2bda00cb25d2c0e26703b7b2147cd2f2432649d2f16f85c753437b47632ab4","source":{"kind":"arxiv","id":"2402.15110","version":2},"attestation_state":"computed","paper":{"title":"A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Md Arif Shaikh, Sajad A. Bhat, Shasvath J. Kapadia","submitted_at":"2024-02-23T05:47:10Z","abstract_excerpt":"The Inspiral Merger Ringdown Consistency Test (IMRCT) is one among a battery of tests of general relativity (GR) employed by the LIGO-Virgo-KAGRA (LVK) collaboration. It is used to search for deviations from GR in detected gravitational waves (GWs) from compact binary coalescences (CBCs) in a model-agnostic way. The test compares source parameter estimates extracted independently from the inspiral and post-inspiral portions of the CBC signals and, therefore, crucially relies on the accurate modeling of the waveform. Current implementations of the IMRCT routinely use quasicircular waveforms, un"},"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":"2402.15110","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-02-23T05:47:10Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"b91d2a9eabf87d5c13b1f526f9f5dabfc3be33401a65883325cf88422018163c","abstract_canon_sha256":"bf38fbd1e84d4e35a7fb68c4a814691dace6372d038dc63546f4c157887ef3be"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:45:25.385307Z","signature_b64":"o6KAd1Tj84nswV6amYJsBwrAl5f2M1JvclaE0wnmYAX/c9bwYj7OmqB4E+EF7Dp4FR6uUrjbGt0+J6/btlCgAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1f2bda00cb25d2c0e26703b7b2147cd2f2432649d2f16f85c753437b47632ab4","last_reissued_at":"2026-07-05T08:45:25.384839Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:45:25.384839Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Md Arif Shaikh, Sajad A. Bhat, Shasvath J. Kapadia","submitted_at":"2024-02-23T05:47:10Z","abstract_excerpt":"The Inspiral Merger Ringdown Consistency Test (IMRCT) is one among a battery of tests of general relativity (GR) employed by the LIGO-Virgo-KAGRA (LVK) collaboration. It is used to search for deviations from GR in detected gravitational waves (GWs) from compact binary coalescences (CBCs) in a model-agnostic way. The test compares source parameter estimates extracted independently from the inspiral and post-inspiral portions of the CBC signals and, therefore, crucially relies on the accurate modeling of the waveform. Current implementations of the IMRCT routinely use quasicircular waveforms, un"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.15110","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/2402.15110/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":"2402.15110","created_at":"2026-07-05T08:45:25.384892+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.15110v2","created_at":"2026-07-05T08:45:25.384892+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.15110","created_at":"2026-07-05T08:45:25.384892+00:00"},{"alias_kind":"pith_short_12","alias_value":"D4V5UAGLEXJM","created_at":"2026-07-05T08:45:25.384892+00:00"},{"alias_kind":"pith_short_16","alias_value":"D4V5UAGLEXJMBYTH","created_at":"2026-07-05T08:45:25.384892+00:00"},{"alias_kind":"pith_short_8","alias_value":"D4V5UAGL","created_at":"2026-07-05T08:45:25.384892+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"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":89,"is_internal_anchor":false},{"citing_arxiv_id":"2404.14286","citing_title":"Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA","ref_index":108,"is_internal_anchor":false},{"citing_arxiv_id":"2601.13173","citing_title":"Plunge-Merger-Ringdown Tests of General Relativity with GW250114","ref_index":101,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25582","citing_title":"Lessons from binary dynamics of inspiralling equal-mass boson-star mergers","ref_index":76,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15431","citing_title":"Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms","ref_index":94,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L","json":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L.json","graph_json":"https://pith.science/api/pith-number/D4V5UAGLEXJMBYTHAO33EFD42L/graph.json","events_json":"https://pith.science/api/pith-number/D4V5UAGLEXJMBYTHAO33EFD42L/events.json","paper":"https://pith.science/paper/D4V5UAGL"},"agent_actions":{"view_html":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L","download_json":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L.json","view_paper":"https://pith.science/paper/D4V5UAGL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.15110&json=true","fetch_graph":"https://pith.science/api/pith-number/D4V5UAGLEXJMBYTHAO33EFD42L/graph.json","fetch_events":"https://pith.science/api/pith-number/D4V5UAGLEXJMBYTHAO33EFD42L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L/action/storage_attestation","attest_author":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L/action/author_attestation","sign_citation":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L/action/citation_signature","submit_replication":"https://pith.science/pith/D4V5UAGLEXJMBYTHAO33EFD42L/action/replication_record"}},"created_at":"2026-07-05T08:45:25.384892+00:00","updated_at":"2026-07-05T08:45:25.384892+00:00"}