{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:WIF33TNQWX6OX6OEEVU67Z2IEB","short_pith_number":"pith:WIF33TNQ","schema_version":"1.0","canonical_sha256":"b20bbdcdb0b5fcebf9c42569efe7482072d33518ec8b8ef511f5d0305740d058","source":{"kind":"arxiv","id":"2408.01525","version":3},"attestation_state":"computed","paper":{"title":"Gravitational-Wave and Gravitational-Wave Memory Signatures of Core-Collapse Supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Adam Burrows, David Vartanyan, Lyla Choi","submitted_at":"2024-08-02T18:35:58Z","abstract_excerpt":"In this paper, we calculate the energy, signal-to-noise ratio, detection range, and angular anisotropy of the matter, matter memory, and neutrino memory gravitational wave (GW) signatures of 21 three-dimensional initially non-rotating core-collapse supernova (CCSN) models carried to late times. We find that inferred energy, signal-to-noise ratio, and detection range are angle-dependent quantities, and that the spread of possible energy, signal-to-noise, and detection ranges across all viewing angles generally increases with progenitor mass. When examining the low-frequency matter memory and ne"},"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":"2408.01525","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-08-02T18:35:58Z","cross_cats_sorted":["astro-ph.SR","gr-qc"],"title_canon_sha256":"55444f9b85d5a58a4b08feb89838adda008633eaf76daa448d872ef017b93e63","abstract_canon_sha256":"455db376304a887ea37f78a5f123b28eb77b87b8aee63aacda22588ff8c6694c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:59:01.353405Z","signature_b64":"CoZ/6oa1/fbI/1eAYflTHUhKmlu84apahFTTy4wfTYs5On9tkS2MlClEPQev+3Bjr13L66MCil1QUyndm84aDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b20bbdcdb0b5fcebf9c42569efe7482072d33518ec8b8ef511f5d0305740d058","last_reissued_at":"2026-07-05T10:59:01.352902Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:59:01.352902Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational-Wave and Gravitational-Wave Memory Signatures of Core-Collapse Supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Adam Burrows, David Vartanyan, Lyla Choi","submitted_at":"2024-08-02T18:35:58Z","abstract_excerpt":"In this paper, we calculate the energy, signal-to-noise ratio, detection range, and angular anisotropy of the matter, matter memory, and neutrino memory gravitational wave (GW) signatures of 21 three-dimensional initially non-rotating core-collapse supernova (CCSN) models carried to late times. We find that inferred energy, signal-to-noise ratio, and detection range are angle-dependent quantities, and that the spread of possible energy, signal-to-noise, and detection ranges across all viewing angles generally increases with progenitor mass. When examining the low-frequency matter memory and ne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.01525","kind":"arxiv","version":3},"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/2408.01525/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":"2408.01525","created_at":"2026-07-05T10:59:01.352964+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.01525v3","created_at":"2026-07-05T10:59:01.352964+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.01525","created_at":"2026-07-05T10:59:01.352964+00:00"},{"alias_kind":"pith_short_12","alias_value":"WIF33TNQWX6O","created_at":"2026-07-05T10:59:01.352964+00:00"},{"alias_kind":"pith_short_16","alias_value":"WIF33TNQWX6OX6OE","created_at":"2026-07-05T10:59:01.352964+00:00"},{"alias_kind":"pith_short_8","alias_value":"WIF33TNQ","created_at":"2026-07-05T10:59:01.352964+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.04896","citing_title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","ref_index":55,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB","json":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB.json","graph_json":"https://pith.science/api/pith-number/WIF33TNQWX6OX6OEEVU67Z2IEB/graph.json","events_json":"https://pith.science/api/pith-number/WIF33TNQWX6OX6OEEVU67Z2IEB/events.json","paper":"https://pith.science/paper/WIF33TNQ"},"agent_actions":{"view_html":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB","download_json":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB.json","view_paper":"https://pith.science/paper/WIF33TNQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.01525&json=true","fetch_graph":"https://pith.science/api/pith-number/WIF33TNQWX6OX6OEEVU67Z2IEB/graph.json","fetch_events":"https://pith.science/api/pith-number/WIF33TNQWX6OX6OEEVU67Z2IEB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB/action/storage_attestation","attest_author":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB/action/author_attestation","sign_citation":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB/action/citation_signature","submit_replication":"https://pith.science/pith/WIF33TNQWX6OX6OEEVU67Z2IEB/action/replication_record"}},"created_at":"2026-07-05T10:59:01.352964+00:00","updated_at":"2026-07-05T10:59:01.352964+00:00"}