{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:TP32NL3HUTPKNWIEUJJB7TWXBU","short_pith_number":"pith:TP32NL3H","schema_version":"1.0","canonical_sha256":"9bf7a6af67a4dea6d904a2521fced70d2bacc55cf0d1aa8d57daf4bd7d267962","source":{"kind":"arxiv","id":"2409.02037","version":1},"attestation_state":"computed","paper":{"title":"Compact binary coalescences: gravitational-wave astronomy with ground-based detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"F. Ohme, J. Veitch, K. Chatziioannou, M. Fishbach, M. P\\\"urrer, T. Dent, V. Raymond","submitted_at":"2024-09-03T16:36:23Z","abstract_excerpt":"The era of gravitational wave astronomy began in 2015 with the observation of the signal from the merger of two black holes by the LIGO detectors; by 2021, almost 100 more such transient signals from coalescences of compact binaries of black holes and neutron stars were catalogued. With improvements to the ground-based interferometer network consisting of LIGO, Virgo, and KAGRA now promising to bring the total number of detections into the hundreds, we review the observational signatures and analysis methods for the most prolific gravitational-wave source: the coalescence of compact binaries."},"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":"2409.02037","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-09-03T16:36:23Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"4289f09382f23b9d5ace0ae9eb3398e3bb161b07253241134f3028f79a106188","abstract_canon_sha256":"6dd4e62f40b93d1e7b7a06f71c3da419f61c6e7f7fb3242f383e88bc9d9e4557"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:02:37.779018Z","signature_b64":"TJ2zhy2DPOBRvm/SORw9cHcVA2lP0NPxIEuYk64/QTqlOFcWfdF1pVUf2+Ytk4Ts1Z2hC5lNikbpV/PZ2DMOCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9bf7a6af67a4dea6d904a2521fced70d2bacc55cf0d1aa8d57daf4bd7d267962","last_reissued_at":"2026-07-05T09:02:37.778524Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:02:37.778524Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Compact binary coalescences: gravitational-wave astronomy with ground-based detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"F. Ohme, J. Veitch, K. Chatziioannou, M. Fishbach, M. P\\\"urrer, T. Dent, V. Raymond","submitted_at":"2024-09-03T16:36:23Z","abstract_excerpt":"The era of gravitational wave astronomy began in 2015 with the observation of the signal from the merger of two black holes by the LIGO detectors; by 2021, almost 100 more such transient signals from coalescences of compact binaries of black holes and neutron stars were catalogued. With improvements to the ground-based interferometer network consisting of LIGO, Virgo, and KAGRA now promising to bring the total number of detections into the hundreds, we review the observational signatures and analysis methods for the most prolific gravitational-wave source: the coalescence of compact binaries."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2409.02037","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/2409.02037/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":"2409.02037","created_at":"2026-07-05T09:02:37.778588+00:00"},{"alias_kind":"arxiv_version","alias_value":"2409.02037v1","created_at":"2026-07-05T09:02:37.778588+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2409.02037","created_at":"2026-07-05T09:02:37.778588+00:00"},{"alias_kind":"pith_short_12","alias_value":"TP32NL3HUTPK","created_at":"2026-07-05T09:02:37.778588+00:00"},{"alias_kind":"pith_short_16","alias_value":"TP32NL3HUTPKNWIE","created_at":"2026-07-05T09:02:37.778588+00:00"},{"alias_kind":"pith_short_8","alias_value":"TP32NL3H","created_at":"2026-07-05T09:02:37.778588+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.27223","citing_title":"GWTC-5.0: An Introduction to Version 5.0 of the Gravitational-Wave Transient Catalog","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2509.03360","citing_title":"The Early Career Workshop of GR-Amaldi 2025","ref_index":57,"is_internal_anchor":false},{"citing_arxiv_id":"2507.08219","citing_title":"GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\\odot}$","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20768","citing_title":"Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition","ref_index":1,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15431","citing_title":"Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms","ref_index":108,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU","json":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU.json","graph_json":"https://pith.science/api/pith-number/TP32NL3HUTPKNWIEUJJB7TWXBU/graph.json","events_json":"https://pith.science/api/pith-number/TP32NL3HUTPKNWIEUJJB7TWXBU/events.json","paper":"https://pith.science/paper/TP32NL3H"},"agent_actions":{"view_html":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU","download_json":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU.json","view_paper":"https://pith.science/paper/TP32NL3H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2409.02037&json=true","fetch_graph":"https://pith.science/api/pith-number/TP32NL3HUTPKNWIEUJJB7TWXBU/graph.json","fetch_events":"https://pith.science/api/pith-number/TP32NL3HUTPKNWIEUJJB7TWXBU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU/action/storage_attestation","attest_author":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU/action/author_attestation","sign_citation":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU/action/citation_signature","submit_replication":"https://pith.science/pith/TP32NL3HUTPKNWIEUJJB7TWXBU/action/replication_record"}},"created_at":"2026-07-05T09:02:37.778588+00:00","updated_at":"2026-07-05T09:02:37.778588+00:00"}