{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:NENHITADKF5UGZALYNZYE6Y6H2","short_pith_number":"pith:NENHITAD","schema_version":"1.0","canonical_sha256":"691a744c03517b43640bc373827b1e3e91e16082047f63e54e827b44035c0ba9","source":{"kind":"arxiv","id":"2106.15259","version":2},"attestation_state":"computed","paper":{"title":"Pre-merger localization of compact-binary mergers with third generation observatories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Alexander H. Nitz, Tito Dal Canton","submitted_at":"2021-06-29T11:31:01Z","abstract_excerpt":"We present the prospects for the pre-merger detection and localization of binary neutron star mergers with third generation gravitational-wave observatories. We consider a wide variety of gravitational-wave networks which may be operating in the 2030's and beyond; these networks include up to two Cosmic Explorer sites, the Einstein Telescope, and continued observation with the existing second generation ground-based detectors. For a fiducial local merger rate of 300 Gpc$^{-3}$yr$^{-1}$, we find that the Einstein Telescope on its own is able to detect 6 and 2 sources per year at 5 and 30 minute"},"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":"2106.15259","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2021-06-29T11:31:01Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"3325142340e63a3f0ed45e3aeade4eea06f3e28fb2f1e8e39ce432920f384a7c","abstract_canon_sha256":"faad1067fee74e20a11dff934088cfae8b835cdd48fbc0b4ed824582d86e2ca5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:11:31.361522Z","signature_b64":"9cNN4nqhiToli7u9ZT8zQM4eD/c+F1QmRUlkd+Mdk6+/y+HEnm3nkm0X/0Wd8adL7dQjD4u2ZOuT8JDM2V15BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"691a744c03517b43640bc373827b1e3e91e16082047f63e54e827b44035c0ba9","last_reissued_at":"2026-07-05T03:11:31.360975Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:11:31.360975Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pre-merger localization of compact-binary mergers with third generation observatories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Alexander H. Nitz, Tito Dal Canton","submitted_at":"2021-06-29T11:31:01Z","abstract_excerpt":"We present the prospects for the pre-merger detection and localization of binary neutron star mergers with third generation gravitational-wave observatories. We consider a wide variety of gravitational-wave networks which may be operating in the 2030's and beyond; these networks include up to two Cosmic Explorer sites, the Einstein Telescope, and continued observation with the existing second generation ground-based detectors. For a fiducial local merger rate of 300 Gpc$^{-3}$yr$^{-1}$, we find that the Einstein Telescope on its own is able to detect 6 and 2 sources per year at 5 and 30 minute"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2106.15259","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2106.15259/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":"2106.15259","created_at":"2026-07-05T03:11:31.361036+00:00"},{"alias_kind":"arxiv_version","alias_value":"2106.15259v2","created_at":"2026-07-05T03:11:31.361036+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2106.15259","created_at":"2026-07-05T03:11:31.361036+00:00"},{"alias_kind":"pith_short_12","alias_value":"NENHITADKF5U","created_at":"2026-07-05T03:11:31.361036+00:00"},{"alias_kind":"pith_short_16","alias_value":"NENHITADKF5UGZAL","created_at":"2026-07-05T03:11:31.361036+00:00"},{"alias_kind":"pith_short_8","alias_value":"NENHITAD","created_at":"2026-07-05T03:11:31.361036+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"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":72,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2","json":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2.json","graph_json":"https://pith.science/api/pith-number/NENHITADKF5UGZALYNZYE6Y6H2/graph.json","events_json":"https://pith.science/api/pith-number/NENHITADKF5UGZALYNZYE6Y6H2/events.json","paper":"https://pith.science/paper/NENHITAD"},"agent_actions":{"view_html":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2","download_json":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2.json","view_paper":"https://pith.science/paper/NENHITAD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2106.15259&json=true","fetch_graph":"https://pith.science/api/pith-number/NENHITADKF5UGZALYNZYE6Y6H2/graph.json","fetch_events":"https://pith.science/api/pith-number/NENHITADKF5UGZALYNZYE6Y6H2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2/action/storage_attestation","attest_author":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2/action/author_attestation","sign_citation":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2/action/citation_signature","submit_replication":"https://pith.science/pith/NENHITADKF5UGZALYNZYE6Y6H2/action/replication_record"}},"created_at":"2026-07-05T03:11:31.361036+00:00","updated_at":"2026-07-05T03:11:31.361036+00:00"}