{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:VCJEWF6CTVPISIYT7Z5ZZE3MC2","short_pith_number":"pith:VCJEWF6C","schema_version":"1.0","canonical_sha256":"a8924b17c29d5e892313fe7b9c936c16893b30ef91f638a02fd72c8d5cf2eb02","source":{"kind":"arxiv","id":"2405.04186","version":1},"attestation_state":"computed","paper":{"title":"Detectability of eccentric binary black holes with PyCBC and cWB pipelines during the third observing run of LIGO-Virgo-KAGRA","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Antoni Ramos-Buades, Bhooshan Gadre, Kanchan Soni, Maria Haney, Sanjit Mitra, Shubhanshu Tiwari","submitted_at":"2024-05-07T10:46:20Z","abstract_excerpt":"Detecting binary black hole (BBH) mergers with quantifiable orbital eccentricity would confirm the existence of a dynamical formation channel for these binaries. The current state-of-the-art gravitational wave searches of LIGO-Virgo-KAGRA strain data focus more on quasicircular mergers due to increased dimensionality and lack of efficient eccentric waveform models. In this work, we compare the sensitivities of two search pipelines, the matched filter-based \\texttt{PyCBC} and the unmodelled coherent Wave Burst (\\texttt{cWB}) algorithms towards the spinning eccentric BBH mergers, using a multipo"},"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":"2405.04186","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-05-07T10:46:20Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"682c16e43edd33e5e2d1f8d4ae67e497f121d55bfb4af77cf88bab5d0714fdc2","abstract_canon_sha256":"66cacc5737953e0b0fef13adedab28dff40a6a13092a8e46d5d89907c036800f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:16:33.165481Z","signature_b64":"4xSZ1Pr3qRORsy7HUeG3w47oOqIefHr2oUsnT8nrRuuM/ZAq3rgblvsQLkO0unzYfZ25lWboNWJ5beZr6HZvCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a8924b17c29d5e892313fe7b9c936c16893b30ef91f638a02fd72c8d5cf2eb02","last_reissued_at":"2026-07-05T08:16:33.164992Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:16:33.164992Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detectability of eccentric binary black holes with PyCBC and cWB pipelines during the third observing run of LIGO-Virgo-KAGRA","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Antoni Ramos-Buades, Bhooshan Gadre, Kanchan Soni, Maria Haney, Sanjit Mitra, Shubhanshu Tiwari","submitted_at":"2024-05-07T10:46:20Z","abstract_excerpt":"Detecting binary black hole (BBH) mergers with quantifiable orbital eccentricity would confirm the existence of a dynamical formation channel for these binaries. The current state-of-the-art gravitational wave searches of LIGO-Virgo-KAGRA strain data focus more on quasicircular mergers due to increased dimensionality and lack of efficient eccentric waveform models. In this work, we compare the sensitivities of two search pipelines, the matched filter-based \\texttt{PyCBC} and the unmodelled coherent Wave Burst (\\texttt{cWB}) algorithms towards the spinning eccentric BBH mergers, using a multipo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.04186","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/2405.04186/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":"2405.04186","created_at":"2026-07-05T08:16:33.165050+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.04186v1","created_at":"2026-07-05T08:16:33.165050+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.04186","created_at":"2026-07-05T08:16:33.165050+00:00"},{"alias_kind":"pith_short_12","alias_value":"VCJEWF6CTVPI","created_at":"2026-07-05T08:16:33.165050+00:00"},{"alias_kind":"pith_short_16","alias_value":"VCJEWF6CTVPISIYT","created_at":"2026-07-05T08:16:33.165050+00:00"},{"alias_kind":"pith_short_8","alias_value":"VCJEWF6C","created_at":"2026-07-05T08:16:33.165050+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"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":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2","json":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2.json","graph_json":"https://pith.science/api/pith-number/VCJEWF6CTVPISIYT7Z5ZZE3MC2/graph.json","events_json":"https://pith.science/api/pith-number/VCJEWF6CTVPISIYT7Z5ZZE3MC2/events.json","paper":"https://pith.science/paper/VCJEWF6C"},"agent_actions":{"view_html":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2","download_json":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2.json","view_paper":"https://pith.science/paper/VCJEWF6C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.04186&json=true","fetch_graph":"https://pith.science/api/pith-number/VCJEWF6CTVPISIYT7Z5ZZE3MC2/graph.json","fetch_events":"https://pith.science/api/pith-number/VCJEWF6CTVPISIYT7Z5ZZE3MC2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2/action/storage_attestation","attest_author":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2/action/author_attestation","sign_citation":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2/action/citation_signature","submit_replication":"https://pith.science/pith/VCJEWF6CTVPISIYT7Z5ZZE3MC2/action/replication_record"}},"created_at":"2026-07-05T08:16:33.165050+00:00","updated_at":"2026-07-05T08:16:33.165050+00:00"}