{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:LSU62OM5RNZJZ2ZJ2VMAPMVQNP","short_pith_number":"pith:LSU62OM5","schema_version":"1.0","canonical_sha256":"5ca9ed399d8b729ceb29d55807b2b06bd409728fe3dcf639ad29b8806bd9f1b1","source":{"kind":"arxiv","id":"1501.00966","version":2},"attestation_state":"computed","paper":{"title":"Coherent Network Analysis of Gravitational Waves from Three-Dimensional Core-Collapse Supernova Models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Kazuhiro Hayama, Kei Kotake, Takami Kuroda, Tomoya Takiwaki","submitted_at":"2015-01-02T12:11:56Z","abstract_excerpt":"Using predictions from three-dimensional (3D) hydrodynamics simulations of core-collapse supernovae (CCSNe), we present a coherent network analysis to detection, reconstruction, and the source localization of the gravitational-wave (GW) signals. We use the {\\tt RIDGE} pipeline for the analysis, in which the network of LIGO Hanford, LIGO Livingston, VIRGO, and KAGRA is considered. By combining with a GW spectrogram analysis, we show that several important hydrodynamics features in the original waveforms persist in the waveforms of the reconstructed signals. The characteristic excess in the spec"},"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":"1501.00966","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-01-02T12:11:56Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"26ee6789a21a2ed1c21f81bd7850c98aafc9d4650a3ed7d4a8efe56e1f4ee12d","abstract_canon_sha256":"c3e9f70e95fe48faf4ca15874f32abcd90573b3c85e485428ab8ab6457a5c540"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:23:38.587308Z","signature_b64":"LXt7w6lO+um8vYJyWu3CNJcgcEdFmNfH3De5fa560TQw2isYZxEZVTc+Pw9J5mLIprv2gqKabBcxTUaaB+88Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5ca9ed399d8b729ceb29d55807b2b06bd409728fe3dcf639ad29b8806bd9f1b1","last_reissued_at":"2026-05-18T01:23:38.586634Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:23:38.586634Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Coherent Network Analysis of Gravitational Waves from Three-Dimensional Core-Collapse Supernova Models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Kazuhiro Hayama, Kei Kotake, Takami Kuroda, Tomoya Takiwaki","submitted_at":"2015-01-02T12:11:56Z","abstract_excerpt":"Using predictions from three-dimensional (3D) hydrodynamics simulations of core-collapse supernovae (CCSNe), we present a coherent network analysis to detection, reconstruction, and the source localization of the gravitational-wave (GW) signals. We use the {\\tt RIDGE} pipeline for the analysis, in which the network of LIGO Hanford, LIGO Livingston, VIRGO, and KAGRA is considered. By combining with a GW spectrogram analysis, we show that several important hydrodynamics features in the original waveforms persist in the waveforms of the reconstructed signals. The characteristic excess in the spec"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.00966","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":"1501.00966","created_at":"2026-05-18T01:23:38.586765+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.00966v2","created_at":"2026-05-18T01:23:38.586765+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.00966","created_at":"2026-05-18T01:23:38.586765+00:00"},{"alias_kind":"pith_short_12","alias_value":"LSU62OM5RNZJ","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_16","alias_value":"LSU62OM5RNZJZ2ZJ","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_8","alias_value":"LSU62OM5","created_at":"2026-05-18T12:29:29.992203+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/LSU62OM5RNZJZ2ZJ2VMAPMVQNP","json":"https://pith.science/pith/LSU62OM5RNZJZ2ZJ2VMAPMVQNP.json","graph_json":"https://pith.science/api/pith-number/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/graph.json","events_json":"https://pith.science/api/pith-number/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/events.json","paper":"https://pith.science/paper/LSU62OM5"},"agent_actions":{"view_html":"https://pith.science/pith/LSU62OM5RNZJZ2ZJ2VMAPMVQNP","download_json":"https://pith.science/pith/LSU62OM5RNZJZ2ZJ2VMAPMVQNP.json","view_paper":"https://pith.science/paper/LSU62OM5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.00966&json=true","fetch_graph":"https://pith.science/api/pith-number/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/graph.json","fetch_events":"https://pith.science/api/pith-number/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/action/storage_attestation","attest_author":"https://pith.science/pith/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/action/author_attestation","sign_citation":"https://pith.science/pith/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/action/citation_signature","submit_replication":"https://pith.science/pith/LSU62OM5RNZJZ2ZJ2VMAPMVQNP/action/replication_record"}},"created_at":"2026-05-18T01:23:38.586765+00:00","updated_at":"2026-05-18T01:23:38.586765+00:00"}