{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:P4CYFB5H7G2AH6LE3U5RJRMW2N","short_pith_number":"pith:P4CYFB5H","schema_version":"1.0","canonical_sha256":"7f058287a7f9b403f964dd3b14c596d34ab763ddcc35cdc97e7d0cbb075d9b58","source":{"kind":"arxiv","id":"1207.3361","version":1},"attestation_state":"computed","paper":{"title":"Systematic errors in measuring parameters of non-spinning compact binary coalescences with post-Newtonian templates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Ajith Parameswaran, Shaon Ghosh, Sukanta Bose","submitted_at":"2012-07-13T20:32:20Z","abstract_excerpt":"We study the astrophysical impact of inaccurate and incomplete modeling of the gravitational waveforms from compact binary coalescences (CBCs). We do so by the matched filtering of complete inspiral-merger-ringdown (IMR) signals with a bank of inspiral-phase templates modeled after the 3.5 post-Newtonian TaylorT1 approximant. The rationale for the choice of the templates is threefold: (1) The inspiral phase of the Phenomenological signals, which are an example of complete IMR signals, is modeled on the same TaylorT1 approximant. (2) In the low-mass limit, where the merger and ringdown phases l"},"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":"1207.3361","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2012-07-13T20:32:20Z","cross_cats_sorted":[],"title_canon_sha256":"daae80b27fcd258fd82813a43802d42230ccf9ef8da8f4c117efc7f42a0476ea","abstract_canon_sha256":"e16b17433d9709836d9f53426eb9987fc83ef4815c1c098bca98a9ab287af1a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:51:01.408881Z","signature_b64":"zXnlsBzzrS2oOOvfGJWokhJ+5GeDX7qD6SYL6PpHW/MyVSSyE5YuPuuv0Ew6q+9G/3lYNqHY17JYlHiwIiMOCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7f058287a7f9b403f964dd3b14c596d34ab763ddcc35cdc97e7d0cbb075d9b58","last_reissued_at":"2026-05-18T03:51:01.408197Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:51:01.408197Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Systematic errors in measuring parameters of non-spinning compact binary coalescences with post-Newtonian templates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Ajith Parameswaran, Shaon Ghosh, Sukanta Bose","submitted_at":"2012-07-13T20:32:20Z","abstract_excerpt":"We study the astrophysical impact of inaccurate and incomplete modeling of the gravitational waveforms from compact binary coalescences (CBCs). We do so by the matched filtering of complete inspiral-merger-ringdown (IMR) signals with a bank of inspiral-phase templates modeled after the 3.5 post-Newtonian TaylorT1 approximant. The rationale for the choice of the templates is threefold: (1) The inspiral phase of the Phenomenological signals, which are an example of complete IMR signals, is modeled on the same TaylorT1 approximant. (2) In the low-mass limit, where the merger and ringdown phases l"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.3361","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":""},"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":"1207.3361","created_at":"2026-05-18T03:51:01.408333+00:00"},{"alias_kind":"arxiv_version","alias_value":"1207.3361v1","created_at":"2026-05-18T03:51:01.408333+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1207.3361","created_at":"2026-05-18T03:51:01.408333+00:00"},{"alias_kind":"pith_short_12","alias_value":"P4CYFB5H7G2A","created_at":"2026-05-18T12:27:18.751474+00:00"},{"alias_kind":"pith_short_16","alias_value":"P4CYFB5H7G2AH6LE","created_at":"2026-05-18T12:27:18.751474+00:00"},{"alias_kind":"pith_short_8","alias_value":"P4CYFB5H","created_at":"2026-05-18T12:27:18.751474+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N","json":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N.json","graph_json":"https://pith.science/api/pith-number/P4CYFB5H7G2AH6LE3U5RJRMW2N/graph.json","events_json":"https://pith.science/api/pith-number/P4CYFB5H7G2AH6LE3U5RJRMW2N/events.json","paper":"https://pith.science/paper/P4CYFB5H"},"agent_actions":{"view_html":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N","download_json":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N.json","view_paper":"https://pith.science/paper/P4CYFB5H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1207.3361&json=true","fetch_graph":"https://pith.science/api/pith-number/P4CYFB5H7G2AH6LE3U5RJRMW2N/graph.json","fetch_events":"https://pith.science/api/pith-number/P4CYFB5H7G2AH6LE3U5RJRMW2N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N/action/storage_attestation","attest_author":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N/action/author_attestation","sign_citation":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N/action/citation_signature","submit_replication":"https://pith.science/pith/P4CYFB5H7G2AH6LE3U5RJRMW2N/action/replication_record"}},"created_at":"2026-05-18T03:51:01.408333+00:00","updated_at":"2026-05-18T03:51:01.408333+00:00"}