{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:TXSP7IQBI6DRHDEUETA573OYJL","short_pith_number":"pith:TXSP7IQB","schema_version":"1.0","canonical_sha256":"9de4ffa2014787138c9424c1dfedd84af3b05d0ff56d66a849692c43e18b11e4","source":{"kind":"arxiv","id":"2109.07642","version":3},"attestation_state":"computed","paper":{"title":"Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Alan J. Weinstein, Jack Y. L. Kwok, Rico K. L. Lo, Tjonnie G. F. Li","submitted_at":"2021-09-16T00:48:52Z","abstract_excerpt":"The detection of gravitational waves from compact binary coalescence by Advanced LIGO and Advanced Virgo provides an opportunity to study the strong-field, highly relativistic regime of gravity. Gravitational-wave tests of general relativity (GR) typically assume Gaussian and stationary detector noise and, thus, do not account for non-Gaussian, transient noise features (glitches). We present the results obtained by performing parametrized gravitational-wave tests on simulated signals from binary-black-hole coalescence overlapped with three classes of frequently occurring instrumental glitches "},"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":"2109.07642","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2021-09-16T00:48:52Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"01a196c0c19a3e7a98b60667afc105db624a395bc69e0fa28ba2275d8cc388d4","abstract_canon_sha256":"3c419275b4e7056f25e0762bb41c3e100edb5818c7e43394153745b833552181"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:53:04.769840Z","signature_b64":"CUin2H42ZPStncrCfGeZAnmDrB6V8HstdA16SDkDlhr55UURh2Mg3+22pKs4P0Nq/qIYnggunTOZUh1wM3DwBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9de4ffa2014787138c9424c1dfedd84af3b05d0ff56d66a849692c43e18b11e4","last_reissued_at":"2026-07-05T03:53:04.769322Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:53:04.769322Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigation of the effects of non-Gaussian noise transients and their mitigation in parameterized gravitational-wave tests of general relativity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Alan J. Weinstein, Jack Y. L. Kwok, Rico K. L. Lo, Tjonnie G. F. Li","submitted_at":"2021-09-16T00:48:52Z","abstract_excerpt":"The detection of gravitational waves from compact binary coalescence by Advanced LIGO and Advanced Virgo provides an opportunity to study the strong-field, highly relativistic regime of gravity. Gravitational-wave tests of general relativity (GR) typically assume Gaussian and stationary detector noise and, thus, do not account for non-Gaussian, transient noise features (glitches). We present the results obtained by performing parametrized gravitational-wave tests on simulated signals from binary-black-hole coalescence overlapped with three classes of frequently occurring instrumental glitches "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2109.07642","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/2109.07642/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":"2109.07642","created_at":"2026-07-05T03:53:04.769382+00:00"},{"alias_kind":"arxiv_version","alias_value":"2109.07642v3","created_at":"2026-07-05T03:53:04.769382+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2109.07642","created_at":"2026-07-05T03:53:04.769382+00:00"},{"alias_kind":"pith_short_12","alias_value":"TXSP7IQBI6DR","created_at":"2026-07-05T03:53:04.769382+00:00"},{"alias_kind":"pith_short_16","alias_value":"TXSP7IQBI6DRHDEU","created_at":"2026-07-05T03:53:04.769382+00:00"},{"alias_kind":"pith_short_8","alias_value":"TXSP7IQB","created_at":"2026-07-05T03:53:04.769382+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2406.03568","citing_title":"Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object","ref_index":110,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16183","citing_title":"Rapid data quality investigations of gravitational-wave events with the Data Quality Report Builder toolkit","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2508.13923","citing_title":"Hunting for new glitches in LIGO data using community science","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2509.03360","citing_title":"The Early Career Workshop of GR-Amaldi 2025","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2509.14924","citing_title":"Residual Test for the Third Gravitational-Wave Transient Catalog","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2112.06861","citing_title":"Tests of General Relativity with GWTC-3","ref_index":300,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL","json":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL.json","graph_json":"https://pith.science/api/pith-number/TXSP7IQBI6DRHDEUETA573OYJL/graph.json","events_json":"https://pith.science/api/pith-number/TXSP7IQBI6DRHDEUETA573OYJL/events.json","paper":"https://pith.science/paper/TXSP7IQB"},"agent_actions":{"view_html":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL","download_json":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL.json","view_paper":"https://pith.science/paper/TXSP7IQB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2109.07642&json=true","fetch_graph":"https://pith.science/api/pith-number/TXSP7IQBI6DRHDEUETA573OYJL/graph.json","fetch_events":"https://pith.science/api/pith-number/TXSP7IQBI6DRHDEUETA573OYJL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL/action/storage_attestation","attest_author":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL/action/author_attestation","sign_citation":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL/action/citation_signature","submit_replication":"https://pith.science/pith/TXSP7IQBI6DRHDEUETA573OYJL/action/replication_record"}},"created_at":"2026-07-05T03:53:04.769382+00:00","updated_at":"2026-07-05T03:53:04.769382+00:00"}