{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:DMFKF7XO4D37VY33TX4E4IGDNO","short_pith_number":"pith:DMFKF7XO","schema_version":"1.0","canonical_sha256":"1b0aa2feeee0f7fae37b9df84e20c36b999a524c08bc8de0d22403656ccb03d8","source":{"kind":"arxiv","id":"2010.15202","version":3},"attestation_state":"computed","paper":{"title":"Gwbench: a novel Fisher information package for gravitational-wave benchmarking","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Ssohrab Borhanian","submitted_at":"2020-10-28T19:52:19Z","abstract_excerpt":"We present a new Python package, gwbench, implementing the well-established Fisher information formalism as a fast and straightforward tool for the purpose of gravitational-wave benchmarking, i.e. the estimation of signal-to-noise ratios and measurement errors of gravitational waves observed by a network of detectors. Such an infrastructure is necessary due to the high computational cost of Bayesian parameter estimation methods which renders them less effective for the scientific assessment of gravitational waveforms, detectors, and networks of detectors, especially when determining their effe"},"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":"2010.15202","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2020-10-28T19:52:19Z","cross_cats_sorted":[],"title_canon_sha256":"83afc75d6f5d5e83d625a7075c16e7b284e8c4421eb3930f0c85b0e700435265","abstract_canon_sha256":"8bc60336b0773acde0f3f903a34e8d87c3bfb9f39606a89a28ac3de06b416618"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:09:43.481978Z","signature_b64":"s8RrNQihGjGbgJLlev3o1nkk3w7ABi50c3if5URDOfFzjG2TgMygNenCOSZl/bSKLW4VYEhf5689Ae6lG6KiDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b0aa2feeee0f7fae37b9df84e20c36b999a524c08bc8de0d22403656ccb03d8","last_reissued_at":"2026-07-05T03:09:43.481551Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:09:43.481551Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gwbench: a novel Fisher information package for gravitational-wave benchmarking","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Ssohrab Borhanian","submitted_at":"2020-10-28T19:52:19Z","abstract_excerpt":"We present a new Python package, gwbench, implementing the well-established Fisher information formalism as a fast and straightforward tool for the purpose of gravitational-wave benchmarking, i.e. the estimation of signal-to-noise ratios and measurement errors of gravitational waves observed by a network of detectors. Such an infrastructure is necessary due to the high computational cost of Bayesian parameter estimation methods which renders them less effective for the scientific assessment of gravitational waveforms, detectors, and networks of detectors, especially when determining their effe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2010.15202","kind":"arxiv","version":3},"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/2010.15202/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":"2010.15202","created_at":"2026-07-05T03:09:43.481608+00:00"},{"alias_kind":"arxiv_version","alias_value":"2010.15202v3","created_at":"2026-07-05T03:09:43.481608+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2010.15202","created_at":"2026-07-05T03:09:43.481608+00:00"},{"alias_kind":"pith_short_12","alias_value":"DMFKF7XO4D37","created_at":"2026-07-05T03:09:43.481608+00:00"},{"alias_kind":"pith_short_16","alias_value":"DMFKF7XO4D37VY33","created_at":"2026-07-05T03:09:43.481608+00:00"},{"alias_kind":"pith_short_8","alias_value":"DMFKF7XO","created_at":"2026-07-05T03:09:43.481608+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.04216","citing_title":"Shape of U: Measuring the Curvature of the Universe with Gravitational Waves","ref_index":68,"is_internal_anchor":false},{"citing_arxiv_id":"2606.03776","citing_title":"Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors","ref_index":12,"is_internal_anchor":false},{"citing_arxiv_id":"2404.16103","citing_title":"Validating Prior-informed Fisher-matrix Analyses against GWTC Data","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2509.04028","citing_title":"Primordial black holes versus their impersonators at gravitational wave observatories","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18428","citing_title":"Probing (sub-)solar-mass black holes and superspinars with current and next-generation gravitational-wave observatories","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2510.11861","citing_title":"Impact of facility timing and coordination for next-generation gravitational-wave detectors","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2510.16955","citing_title":"On the use of the Derivative Approximation for Likelihoods for Gravitational Wave Inference","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2303.15923","citing_title":"Science with the Einstein Telescope: a comparison of different designs","ref_index":30,"is_internal_anchor":false},{"citing_arxiv_id":"2512.09978","citing_title":"Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123","ref_index":57,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO","json":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO.json","graph_json":"https://pith.science/api/pith-number/DMFKF7XO4D37VY33TX4E4IGDNO/graph.json","events_json":"https://pith.science/api/pith-number/DMFKF7XO4D37VY33TX4E4IGDNO/events.json","paper":"https://pith.science/paper/DMFKF7XO"},"agent_actions":{"view_html":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO","download_json":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO.json","view_paper":"https://pith.science/paper/DMFKF7XO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2010.15202&json=true","fetch_graph":"https://pith.science/api/pith-number/DMFKF7XO4D37VY33TX4E4IGDNO/graph.json","fetch_events":"https://pith.science/api/pith-number/DMFKF7XO4D37VY33TX4E4IGDNO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO/action/storage_attestation","attest_author":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO/action/author_attestation","sign_citation":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO/action/citation_signature","submit_replication":"https://pith.science/pith/DMFKF7XO4D37VY33TX4E4IGDNO/action/replication_record"}},"created_at":"2026-07-05T03:09:43.481608+00:00","updated_at":"2026-07-05T03:09:43.481608+00:00"}