{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:XYGUNCBHFAWDCUQ4P3ZZMEZEDU","short_pith_number":"pith:XYGUNCBH","schema_version":"1.0","canonical_sha256":"be0d468827282c31521c7ef39613241d382b58f4dad5d83b861b3a237933c94c","source":{"kind":"arxiv","id":"2308.07348","version":1},"attestation_state":"computed","paper":{"title":"Observational prospects of double neutrons star mergers and their multi-messenger afterglows: LIGO discovery power, event rates and diversity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Lorenzo Amati, Maryam A. Abchouyeh, Maurice H.P.M. van Putten","submitted_at":"2023-08-14T05:37:04Z","abstract_excerpt":"The double neutron star (DNS) merger event GW170817 signifies the first multimessenger (MM) event with electromagnetic-gravitational (EM-GW) observations. LIGO-Virgo-KAGRA observational runs O4-5 promise to detect similar events and as yet unknown GW signals, which require confirmation in two or more detectors with comparable performance. To this end, we quantify duty cycles of comparable science quality of data in coincident H1L1-observations, further to seek consistent event rates of astrophysical transients in upcoming EM-GW surveys. Quite generally, discovery power scales with exposure tim"},"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":"2308.07348","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-08-14T05:37:04Z","cross_cats_sorted":[],"title_canon_sha256":"4c1e3556607c5c6686977ca2792ee19c54440f5d77c5ef5b12df59e25afc9a33","abstract_canon_sha256":"ad16c7e69be2bf2b96358e45c4bd89af07fee9e46b591513fdd9e40935eb07bd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:41:24.043546Z","signature_b64":"/nbZUtv+Q/XfM0soHxiUH5vqoAJzy2AW3HbKco+M14Npmo5vUFD+keIsh0Z2Z3iGIyH+Ox5JkugK0lb5R/FhAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"be0d468827282c31521c7ef39613241d382b58f4dad5d83b861b3a237933c94c","last_reissued_at":"2026-07-05T06:41:24.043152Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:41:24.043152Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Observational prospects of double neutrons star mergers and their multi-messenger afterglows: LIGO discovery power, event rates and diversity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Lorenzo Amati, Maryam A. Abchouyeh, Maurice H.P.M. van Putten","submitted_at":"2023-08-14T05:37:04Z","abstract_excerpt":"The double neutron star (DNS) merger event GW170817 signifies the first multimessenger (MM) event with electromagnetic-gravitational (EM-GW) observations. LIGO-Virgo-KAGRA observational runs O4-5 promise to detect similar events and as yet unknown GW signals, which require confirmation in two or more detectors with comparable performance. To this end, we quantify duty cycles of comparable science quality of data in coincident H1L1-observations, further to seek consistent event rates of astrophysical transients in upcoming EM-GW surveys. Quite generally, discovery power scales with exposure tim"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.07348","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/2308.07348/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":"2308.07348","created_at":"2026-07-05T06:41:24.043209+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.07348v1","created_at":"2026-07-05T06:41:24.043209+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.07348","created_at":"2026-07-05T06:41:24.043209+00:00"},{"alias_kind":"pith_short_12","alias_value":"XYGUNCBHFAWD","created_at":"2026-07-05T06:41:24.043209+00:00"},{"alias_kind":"pith_short_16","alias_value":"XYGUNCBHFAWDCUQ4","created_at":"2026-07-05T06:41:24.043209+00:00"},{"alias_kind":"pith_short_8","alias_value":"XYGUNCBH","created_at":"2026-07-05T06:41:24.043209+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.07871","citing_title":"Gravitational Waves from Accretion Disks: Turbulence, Mode Excitation and Prospects for Future Detectors","ref_index":82,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU","json":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU.json","graph_json":"https://pith.science/api/pith-number/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/graph.json","events_json":"https://pith.science/api/pith-number/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/events.json","paper":"https://pith.science/paper/XYGUNCBH"},"agent_actions":{"view_html":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU","download_json":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU.json","view_paper":"https://pith.science/paper/XYGUNCBH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.07348&json=true","fetch_graph":"https://pith.science/api/pith-number/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/graph.json","fetch_events":"https://pith.science/api/pith-number/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/action/storage_attestation","attest_author":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/action/author_attestation","sign_citation":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/action/citation_signature","submit_replication":"https://pith.science/pith/XYGUNCBHFAWDCUQ4P3ZZMEZEDU/action/replication_record"}},"created_at":"2026-07-05T06:41:24.043209+00:00","updated_at":"2026-07-05T06:41:24.043209+00:00"}