{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:EW5OPAKYRKYULTJI4TJSSVKH3Y","short_pith_number":"pith:EW5OPAKY","schema_version":"1.0","canonical_sha256":"25bae781588ab145cd28e4d3295547de192d79258be32d9449b996c9f07e0b76","source":{"kind":"arxiv","id":"1106.2547","version":2},"attestation_state":"computed","paper":{"title":"Estimating parameters of coalescing compact binaries with a detector network including LIGO Australia","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Alberto Vecchio, Benjamin Aylott, Benjamin Farr, Carl Rodriguez, Ilya Mandel, John Veitch, Marc van der Sluys, Vassiliki Kalogera, Vivien Raymond","submitted_at":"2011-06-13T20:00:03Z","abstract_excerpt":"One of the goals of gravitational-wave astronomy is simultaneous detection of gravitational-wave signals from merging compact-object binaries and the electromagnetic transients from these mergers. With the next generation of advanced ground-based gravitational wave detectors under construction, we examine the benefits of the proposed extension of the detector network to include a fourth site in Australia in addition to the network of Hanford, Livingston and Cascina sites. Using Bayesian parameter-estimation analyses of simulated gravitational-wave signals from a range of coalescing-binary loca"},"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":"1106.2547","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-06-13T20:00:03Z","cross_cats_sorted":["astro-ph.IM","gr-qc"],"title_canon_sha256":"2168749bd34b9e503c44448a3ca7476fa0025820bb3ef37ab1e5038b1443b870","abstract_canon_sha256":"3921dab32712e536fe46c7d349aaf71f7039764466ff083a564cb9443f0d1513"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:20:37.221765Z","signature_b64":"DSQ6qrpcgx70nFX792bhgViJ39+kixmTLkAGyVKjBxOvKBBbJcMm+teX0pUSAj4JpEFCVEOK0oND3Cg48ZSCAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"25bae781588ab145cd28e4d3295547de192d79258be32d9449b996c9f07e0b76","last_reissued_at":"2026-05-18T01:20:37.221234Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:20:37.221234Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Estimating parameters of coalescing compact binaries with a detector network including LIGO Australia","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Alberto Vecchio, Benjamin Aylott, Benjamin Farr, Carl Rodriguez, Ilya Mandel, John Veitch, Marc van der Sluys, Vassiliki Kalogera, Vivien Raymond","submitted_at":"2011-06-13T20:00:03Z","abstract_excerpt":"One of the goals of gravitational-wave astronomy is simultaneous detection of gravitational-wave signals from merging compact-object binaries and the electromagnetic transients from these mergers. With the next generation of advanced ground-based gravitational wave detectors under construction, we examine the benefits of the proposed extension of the detector network to include a fourth site in Australia in addition to the network of Hanford, Livingston and Cascina sites. Using Bayesian parameter-estimation analyses of simulated gravitational-wave signals from a range of coalescing-binary loca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.2547","kind":"arxiv","version":2},"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":"1106.2547","created_at":"2026-05-18T01:20:37.221301+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.2547v2","created_at":"2026-05-18T01:20:37.221301+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.2547","created_at":"2026-05-18T01:20:37.221301+00:00"},{"alias_kind":"pith_short_12","alias_value":"EW5OPAKYRKYU","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_16","alias_value":"EW5OPAKYRKYULTJI","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_8","alias_value":"EW5OPAKY","created_at":"2026-05-18T12:26:28.662955+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/EW5OPAKYRKYULTJI4TJSSVKH3Y","json":"https://pith.science/pith/EW5OPAKYRKYULTJI4TJSSVKH3Y.json","graph_json":"https://pith.science/api/pith-number/EW5OPAKYRKYULTJI4TJSSVKH3Y/graph.json","events_json":"https://pith.science/api/pith-number/EW5OPAKYRKYULTJI4TJSSVKH3Y/events.json","paper":"https://pith.science/paper/EW5OPAKY"},"agent_actions":{"view_html":"https://pith.science/pith/EW5OPAKYRKYULTJI4TJSSVKH3Y","download_json":"https://pith.science/pith/EW5OPAKYRKYULTJI4TJSSVKH3Y.json","view_paper":"https://pith.science/paper/EW5OPAKY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.2547&json=true","fetch_graph":"https://pith.science/api/pith-number/EW5OPAKYRKYULTJI4TJSSVKH3Y/graph.json","fetch_events":"https://pith.science/api/pith-number/EW5OPAKYRKYULTJI4TJSSVKH3Y/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EW5OPAKYRKYULTJI4TJSSVKH3Y/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EW5OPAKYRKYULTJI4TJSSVKH3Y/action/storage_attestation","attest_author":"https://pith.science/pith/EW5OPAKYRKYULTJI4TJSSVKH3Y/action/author_attestation","sign_citation":"https://pith.science/pith/EW5OPAKYRKYULTJI4TJSSVKH3Y/action/citation_signature","submit_replication":"https://pith.science/pith/EW5OPAKYRKYULTJI4TJSSVKH3Y/action/replication_record"}},"created_at":"2026-05-18T01:20:37.221301+00:00","updated_at":"2026-05-18T01:20:37.221301+00:00"}