{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:UUM23UVAPOTJXWQBJOSB2B5ILJ","short_pith_number":"pith:UUM23UVA","schema_version":"1.0","canonical_sha256":"a519add2a07ba69bda014ba41d07a85a621de0142f802ceeb12e0529472ff560","source":{"kind":"arxiv","id":"2402.02819","version":2},"attestation_state":"computed","paper":{"title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Eric Thrane, Jordan Moxon, Keefe Mitman, Kyle C. Nelli, Lawrence E. Kidder, Maximiliano Isi, Michael Boyle, Nils Deppe, Nils L. Vu, Paul D. Lasky, Teagan A. Clarke, William Throwe","submitted_at":"2024-02-05T09:03:45Z","abstract_excerpt":"The ringdown portion of a binary black hole merger consists of a sum of modes, each containing an infinite number of tones that are exponentially damped sinusoids. In principle, these can be measured as gravitational-waves with observatories like LIGO/Virgo/KAGRA, however in practice it is unclear how many tones can be meaningfully resolved. We investigate the consistency and resolvability of the overtones of the quadrupolar $\\ell = m = 2$ mode by starting at late times when the gravitational waveform is expected to be well-approximated by the $\\ell m n = 220$ tone alone. We present a Bayesian"},"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":"2402.02819","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-02-05T09:03:45Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"70e939b362f4e05f1c373c86b78fd4152714ad0eca36e48990b0d4856eb470b5","abstract_canon_sha256":"1adb9c9aa53fdb1c4a6668215bfab040b2414a2120958de6a03be6d05ebb8f95"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:30:31.546281Z","signature_b64":"zrO7vcqq92/OZoJyQDA9bsSmYGs2bBKBBJx+Tdredw2gaDNaK4PDsYmaYG4aZoJg478bzpbUNzRJobc6U5V7CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a519add2a07ba69bda014ba41d07a85a621de0142f802ceeb12e0529472ff560","last_reissued_at":"2026-07-05T08:30:31.545734Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:30:31.545734Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Striking the right tone: toward a self-consistent framework for measuring black hole ringdowns","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Eric Thrane, Jordan Moxon, Keefe Mitman, Kyle C. Nelli, Lawrence E. Kidder, Maximiliano Isi, Michael Boyle, Nils Deppe, Nils L. Vu, Paul D. Lasky, Teagan A. Clarke, William Throwe","submitted_at":"2024-02-05T09:03:45Z","abstract_excerpt":"The ringdown portion of a binary black hole merger consists of a sum of modes, each containing an infinite number of tones that are exponentially damped sinusoids. In principle, these can be measured as gravitational-waves with observatories like LIGO/Virgo/KAGRA, however in practice it is unclear how many tones can be meaningfully resolved. We investigate the consistency and resolvability of the overtones of the quadrupolar $\\ell = m = 2$ mode by starting at late times when the gravitational waveform is expected to be well-approximated by the $\\ell m n = 220$ tone alone. We present a Bayesian"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.02819","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/2402.02819/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":"2402.02819","created_at":"2026-07-05T08:30:31.545794+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.02819v2","created_at":"2026-07-05T08:30:31.545794+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.02819","created_at":"2026-07-05T08:30:31.545794+00:00"},{"alias_kind":"pith_short_12","alias_value":"UUM23UVAPOTJ","created_at":"2026-07-05T08:30:31.545794+00:00"},{"alias_kind":"pith_short_16","alias_value":"UUM23UVAPOTJXWQB","created_at":"2026-07-05T08:30:31.545794+00:00"},{"alias_kind":"pith_short_8","alias_value":"UUM23UVA","created_at":"2026-07-05T08:30:31.545794+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2512.08598","citing_title":"Horizon brightened acceleration radiation from massive vector fields","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03576","citing_title":"Ringdown Analysis of GW250114 with Orthonormal Modes","ref_index":51,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ","json":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ.json","graph_json":"https://pith.science/api/pith-number/UUM23UVAPOTJXWQBJOSB2B5ILJ/graph.json","events_json":"https://pith.science/api/pith-number/UUM23UVAPOTJXWQBJOSB2B5ILJ/events.json","paper":"https://pith.science/paper/UUM23UVA"},"agent_actions":{"view_html":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ","download_json":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ.json","view_paper":"https://pith.science/paper/UUM23UVA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.02819&json=true","fetch_graph":"https://pith.science/api/pith-number/UUM23UVAPOTJXWQBJOSB2B5ILJ/graph.json","fetch_events":"https://pith.science/api/pith-number/UUM23UVAPOTJXWQBJOSB2B5ILJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ/action/storage_attestation","attest_author":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ/action/author_attestation","sign_citation":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ/action/citation_signature","submit_replication":"https://pith.science/pith/UUM23UVAPOTJXWQBJOSB2B5ILJ/action/replication_record"}},"created_at":"2026-07-05T08:30:31.545794+00:00","updated_at":"2026-07-05T08:30:31.545794+00:00"}