{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:JDU4WKB3PPKF4AMNEJAHSXRCTL","short_pith_number":"pith:JDU4WKB3","schema_version":"1.0","canonical_sha256":"48e9cb283b7bd45e018d2240795e229ae6296a1885754e62fa101704a14d7bca","source":{"kind":"arxiv","id":"1508.03634","version":6},"attestation_state":"computed","paper":{"title":"Rapid Bayesian position reconstruction for gravitational-wave transients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Larry R. Price, Leo P. Singer","submitted_at":"2015-08-14T20:05:01Z","abstract_excerpt":"Within the next few years, Advanced LIGO and Virgo should detect gravitational waves from binary neutron star and neutron star-black hole mergers. These sources are also predicted to power a broad array of electromagnetic transients. Because the electromagnetic signatures can be faint and fade rapidly, observing them hinges on rapidly inferring the sky location from the gravitational-wave observations. Markov chain Monte Carlo methods for gravitational-wave parameter estimation can take hours or more. We introduce BAYESTAR, a rapid, Bayesian, non-Markov chain Monte Carlo sky localization algor"},"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":"1508.03634","kind":"arxiv","version":6},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2015-08-14T20:05:01Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"6722e4f526c106386ed290a5bdd1e6121051ad29ecfd272844bf324190b81eb1","abstract_canon_sha256":"6ee06ff89c1feb48acfa24d4ef4eedcfa0a8980b55678fdbd71453c593f81a8a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:22:37.005666Z","signature_b64":"vR9Si8cCKIlZPk2iu/SBhKNFillhRdd3KpJXWV8roEaOAnO3G+Qq41UT/7jIx/IEELCBWrmnbx8KoR5gzd5tCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"48e9cb283b7bd45e018d2240795e229ae6296a1885754e62fa101704a14d7bca","last_reissued_at":"2026-05-18T01:22:37.005259Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:22:37.005259Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rapid Bayesian position reconstruction for gravitational-wave transients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Larry R. Price, Leo P. Singer","submitted_at":"2015-08-14T20:05:01Z","abstract_excerpt":"Within the next few years, Advanced LIGO and Virgo should detect gravitational waves from binary neutron star and neutron star-black hole mergers. These sources are also predicted to power a broad array of electromagnetic transients. Because the electromagnetic signatures can be faint and fade rapidly, observing them hinges on rapidly inferring the sky location from the gravitational-wave observations. Markov chain Monte Carlo methods for gravitational-wave parameter estimation can take hours or more. We introduce BAYESTAR, a rapid, Bayesian, non-Markov chain Monte Carlo sky localization algor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.03634","kind":"arxiv","version":6},"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":"1508.03634","created_at":"2026-05-18T01:22:37.005325+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.03634v6","created_at":"2026-05-18T01:22:37.005325+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.03634","created_at":"2026-05-18T01:22:37.005325+00:00"},{"alias_kind":"pith_short_12","alias_value":"JDU4WKB3PPKF","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_16","alias_value":"JDU4WKB3PPKF4AMN","created_at":"2026-05-18T12:29:27.538025+00:00"},{"alias_kind":"pith_short_8","alias_value":"JDU4WKB3","created_at":"2026-05-18T12:29:27.538025+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.19153","citing_title":"GstLAL O4 Online Results Paper","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2108.01045","citing_title":"GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","ref_index":289,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11703","citing_title":"GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors","ref_index":64,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25116","citing_title":"Gauge Theoretic Signal Processing II: Zero-Latency Whitening for Early Warning Pipelines","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11871","citing_title":"Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors","ref_index":87,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13580","citing_title":"Investigating the effect of sensitivity of KAGRA on sky localization of gravitational-wave sources from compact binary coalescences","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL","json":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL.json","graph_json":"https://pith.science/api/pith-number/JDU4WKB3PPKF4AMNEJAHSXRCTL/graph.json","events_json":"https://pith.science/api/pith-number/JDU4WKB3PPKF4AMNEJAHSXRCTL/events.json","paper":"https://pith.science/paper/JDU4WKB3"},"agent_actions":{"view_html":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL","download_json":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL.json","view_paper":"https://pith.science/paper/JDU4WKB3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.03634&json=true","fetch_graph":"https://pith.science/api/pith-number/JDU4WKB3PPKF4AMNEJAHSXRCTL/graph.json","fetch_events":"https://pith.science/api/pith-number/JDU4WKB3PPKF4AMNEJAHSXRCTL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL/action/storage_attestation","attest_author":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL/action/author_attestation","sign_citation":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL/action/citation_signature","submit_replication":"https://pith.science/pith/JDU4WKB3PPKF4AMNEJAHSXRCTL/action/replication_record"}},"created_at":"2026-05-18T01:22:37.005325+00:00","updated_at":"2026-05-18T01:22:37.005325+00:00"}