{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:LNNR3SRS34MG2RK77TQR3R3NW6","short_pith_number":"pith:LNNR3SRS","schema_version":"1.0","canonical_sha256":"5b5b1dca32df186d455ffce11dc76db7aa69079b07362c35b974f6f56888afdc","source":{"kind":"arxiv","id":"astro-ph/0605227","version":1},"attestation_state":"computed","paper":{"title":"The LISA verification binaries","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph","authors_text":"A. Stroeer, A. Vecchio","submitted_at":"2006-05-09T11:32:02Z","abstract_excerpt":"The Laser Interferometer Space Antenna (LISA) guarantees the detection of gravitational waves by monitoring a handful of known nearby galactic binary systems, the so-called ``verification binaries''. We consider the most updated information on the source parameters for the thirty more promising verification binaries. We investigate which of them are indeed guaranteed sources for LISA and estimate the accuracy of the additional information that can be extracted during the mission. Our analysis considers the two independent Michelson outputs that can be synthesised from the LISA constellation, a"},"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":"astro-ph/0605227","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-05-09T11:32:02Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"dd4756cd767e3d42263f3e2a89d547adedbc89ba46e2e2bfe8058acd5b8a938f","abstract_canon_sha256":"9537af95d6fb8637cb59ce2e8fb3831d065b42505efbd80579eb82780c9e5fa0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:58:42.530594Z","signature_b64":"O+oW8/Q4NGU5DCPWw7vSXJ8d3/iSut7ASeVumoKhVmay/wNT8hiD2pQNnYg7yxFkXOvxGHthgMIW14jxCH//AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b5b1dca32df186d455ffce11dc76db7aa69079b07362c35b974f6f56888afdc","last_reissued_at":"2026-07-04T16:58:42.530230Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:58:42.530230Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The LISA verification binaries","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph","authors_text":"A. Stroeer, A. Vecchio","submitted_at":"2006-05-09T11:32:02Z","abstract_excerpt":"The Laser Interferometer Space Antenna (LISA) guarantees the detection of gravitational waves by monitoring a handful of known nearby galactic binary systems, the so-called ``verification binaries''. We consider the most updated information on the source parameters for the thirty more promising verification binaries. We investigate which of them are indeed guaranteed sources for LISA and estimate the accuracy of the additional information that can be extracted during the mission. Our analysis considers the two independent Michelson outputs that can be synthesised from the LISA constellation, a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0605227","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/astro-ph/0605227/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":"astro-ph/0605227","created_at":"2026-07-04T16:58:42.530294+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0605227v1","created_at":"2026-07-04T16:58:42.530294+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0605227","created_at":"2026-07-04T16:58:42.530294+00:00"},{"alias_kind":"pith_short_12","alias_value":"LNNR3SRS34MG","created_at":"2026-07-04T16:58:42.530294+00:00"},{"alias_kind":"pith_short_16","alias_value":"LNNR3SRS34MG2RK7","created_at":"2026-07-04T16:58:42.530294+00:00"},{"alias_kind":"pith_short_8","alias_value":"LNNR3SRS","created_at":"2026-07-04T16:58:42.530294+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":149,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6","json":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6.json","graph_json":"https://pith.science/api/pith-number/LNNR3SRS34MG2RK77TQR3R3NW6/graph.json","events_json":"https://pith.science/api/pith-number/LNNR3SRS34MG2RK77TQR3R3NW6/events.json","paper":"https://pith.science/paper/LNNR3SRS"},"agent_actions":{"view_html":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6","download_json":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6.json","view_paper":"https://pith.science/paper/LNNR3SRS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0605227&json=true","fetch_graph":"https://pith.science/api/pith-number/LNNR3SRS34MG2RK77TQR3R3NW6/graph.json","fetch_events":"https://pith.science/api/pith-number/LNNR3SRS34MG2RK77TQR3R3NW6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6/action/storage_attestation","attest_author":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6/action/author_attestation","sign_citation":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6/action/citation_signature","submit_replication":"https://pith.science/pith/LNNR3SRS34MG2RK77TQR3R3NW6/action/replication_record"}},"created_at":"2026-07-04T16:58:42.530294+00:00","updated_at":"2026-07-04T16:58:42.530294+00:00"}