{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:SGAYOF7AWUUHOKBYZLJMLJFFW3","short_pith_number":"pith:SGAYOF7A","schema_version":"1.0","canonical_sha256":"91818717e0b528772838cad2c5a4a5b6ed38f468da731dfd01b1e20869d018fb","source":{"kind":"arxiv","id":"2012.09552","version":1},"attestation_state":"computed","paper":{"title":"SWIGLAL: Python and Octave interfaces to the LALSuite gravitational-wave data analysis libraries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.IM","authors_text":"Karl Wette","submitted_at":"2020-12-17T12:50:35Z","abstract_excerpt":"The LALSuite data analysis libraries, written in C, implement key routines critical to the successful detection of gravitational waves, such as the template waveforms describing the merger of two black holes or two neutron stars. SWIGLAL is a component of LALSuite which provides interfaces for Python and Octave, making LALSuite routines accessible directly from scripts written in those languages. It has enabled modern gravitational-wave data analysis software, used in the first detection of gravitational waves, to be written in Python, thereby benefiting from its ease of development and rich f"},"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":"2012.09552","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2020-12-17T12:50:35Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"1c8c3bc8a42e9d15bbad3ff38b39072c0a38fa30438ffc652405908336813c77","abstract_canon_sha256":"c5057d6827f551a457f552cd4c84870e17a0bf8d55438948f0103e2ae3862d35"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:00:18.865701Z","signature_b64":"iM7U+M09v2n/gK8/zE0nASusml1kq+9kbuB4ySbGTpdxCmaYa4dESoOWoAbhXu5WKu8UnB/jkm0d9xwWTsP8DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"91818717e0b528772838cad2c5a4a5b6ed38f468da731dfd01b1e20869d018fb","last_reissued_at":"2026-07-05T02:00:18.865268Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:00:18.865268Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SWIGLAL: Python and Octave interfaces to the LALSuite gravitational-wave data analysis libraries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.IM","authors_text":"Karl Wette","submitted_at":"2020-12-17T12:50:35Z","abstract_excerpt":"The LALSuite data analysis libraries, written in C, implement key routines critical to the successful detection of gravitational waves, such as the template waveforms describing the merger of two black holes or two neutron stars. SWIGLAL is a component of LALSuite which provides interfaces for Python and Octave, making LALSuite routines accessible directly from scripts written in those languages. It has enabled modern gravitational-wave data analysis software, used in the first detection of gravitational waves, to be written in Python, thereby benefiting from its ease of development and rich f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.09552","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/2012.09552/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":"2012.09552","created_at":"2026-07-05T02:00:18.865324+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.09552v1","created_at":"2026-07-05T02:00:18.865324+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.09552","created_at":"2026-07-05T02:00:18.865324+00:00"},{"alias_kind":"pith_short_12","alias_value":"SGAYOF7AWUUH","created_at":"2026-07-05T02:00:18.865324+00:00"},{"alias_kind":"pith_short_16","alias_value":"SGAYOF7AWUUHOKBY","created_at":"2026-07-05T02:00:18.865324+00:00"},{"alias_kind":"pith_short_8","alias_value":"SGAYOF7A","created_at":"2026-07-05T02:00:18.865324+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.12496","citing_title":"Artifact-Conditioned Interval Diagnostics for Flow-Matching Neural Posterior Estimation in a Controlled Gravitational-Wave Benchmark","ref_index":19,"is_internal_anchor":false},{"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":100,"is_internal_anchor":false},{"citing_arxiv_id":"2511.12642","citing_title":"Auto-encoder model for faster generation of effective one-body gravitational waveform approximations","ref_index":78,"is_internal_anchor":false},{"citing_arxiv_id":"2509.08099","citing_title":"Black Hole Spectroscopy and Tests of General Relativity with GW250114","ref_index":203,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11703","citing_title":"GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors","ref_index":156,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04579","citing_title":"The Impact of Spin Priors on Parameterized Tests of General Relativity","ref_index":39,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3","json":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3.json","graph_json":"https://pith.science/api/pith-number/SGAYOF7AWUUHOKBYZLJMLJFFW3/graph.json","events_json":"https://pith.science/api/pith-number/SGAYOF7AWUUHOKBYZLJMLJFFW3/events.json","paper":"https://pith.science/paper/SGAYOF7A"},"agent_actions":{"view_html":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3","download_json":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3.json","view_paper":"https://pith.science/paper/SGAYOF7A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.09552&json=true","fetch_graph":"https://pith.science/api/pith-number/SGAYOF7AWUUHOKBYZLJMLJFFW3/graph.json","fetch_events":"https://pith.science/api/pith-number/SGAYOF7AWUUHOKBYZLJMLJFFW3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3/action/storage_attestation","attest_author":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3/action/author_attestation","sign_citation":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3/action/citation_signature","submit_replication":"https://pith.science/pith/SGAYOF7AWUUHOKBYZLJMLJFFW3/action/replication_record"}},"created_at":"2026-07-05T02:00:18.865324+00:00","updated_at":"2026-07-05T02:00:18.865324+00:00"}