{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:CM6NLLB6JEJOVFNX4VWLI37G4A","short_pith_number":"pith:CM6NLLB6","schema_version":"1.0","canonical_sha256":"133cd5ac3e4912ea95b7e56cb46fe6e00ceb2dd1314f7bc5802dbe42f6deb373","source":{"kind":"arxiv","id":"2303.04109","version":2},"attestation_state":"computed","paper":{"title":"Deep Einstein@Home all-sky search for continuous gravitational waves in LIGO O3 public data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"B. Allen, B. Machenschalk, B. Steltner, H.-B. Eggenstein, M. A. Papa, M. Bensch, R. Prix","submitted_at":"2023-03-07T18:19:06Z","abstract_excerpt":"We present the results of an all-sky search for continuous gravitational waves in the public LIGO O3 data. The search covers signal frequencies $20$ Hz $\\leq f \\leq 800$ Hz and a spin-down range down to $-2.6\\times 10^{-9}$ Hz s$^{-1}$1, motivated by detectability studies on synthetic populations of Galactic neutron stars. This search is the most sensitive all-sky search to date in this frequency/spin-down region. The initial search was performed using the first half of the public LIGO O3 data (O3a), utilizing Graphical Processing Units provided in equal parts by the volunteers of the Einstein"},"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":"2303.04109","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-03-07T18:19:06Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"401d40cebf15173f493424b9e697106cb47142348e4ac970005be41a16703579","abstract_canon_sha256":"3e06f1b4643eb710cb83993d4161504b499a55de62f3f99b6f3a6282e1348e66"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:33:04.281853Z","signature_b64":"xYXTWido4/vF6xwvq+F6nir11rS1E3NGceUe4V+DPi2Okt7yMJRqaVRKAwbeRSF/9UELZ6mtv8QyV8MB7xHDBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"133cd5ac3e4912ea95b7e56cb46fe6e00ceb2dd1314f7bc5802dbe42f6deb373","last_reissued_at":"2026-07-05T06:33:04.281393Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:33:04.281393Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Deep Einstein@Home all-sky search for continuous gravitational waves in LIGO O3 public data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"B. Allen, B. Machenschalk, B. Steltner, H.-B. Eggenstein, M. A. Papa, M. Bensch, R. Prix","submitted_at":"2023-03-07T18:19:06Z","abstract_excerpt":"We present the results of an all-sky search for continuous gravitational waves in the public LIGO O3 data. The search covers signal frequencies $20$ Hz $\\leq f \\leq 800$ Hz and a spin-down range down to $-2.6\\times 10^{-9}$ Hz s$^{-1}$1, motivated by detectability studies on synthetic populations of Galactic neutron stars. This search is the most sensitive all-sky search to date in this frequency/spin-down region. The initial search was performed using the first half of the public LIGO O3 data (O3a), utilizing Graphical Processing Units provided in equal parts by the volunteers of the Einstein"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.04109","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/2303.04109/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":"2303.04109","created_at":"2026-07-05T06:33:04.281451+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.04109v2","created_at":"2026-07-05T06:33:04.281451+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.04109","created_at":"2026-07-05T06:33:04.281451+00:00"},{"alias_kind":"pith_short_12","alias_value":"CM6NLLB6JEJO","created_at":"2026-07-05T06:33:04.281451+00:00"},{"alias_kind":"pith_short_16","alias_value":"CM6NLLB6JEJOVFNX","created_at":"2026-07-05T06:33:04.281451+00:00"},{"alias_kind":"pith_short_8","alias_value":"CM6NLLB6","created_at":"2026-07-05T06:33:04.281451+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.05082","citing_title":"First Constraints on the Ellipticities of Self-Interacting Fermionic Dark Matter Admixed Neutron Stars from Continuous Gravitational-Wave Searches","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A","json":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A.json","graph_json":"https://pith.science/api/pith-number/CM6NLLB6JEJOVFNX4VWLI37G4A/graph.json","events_json":"https://pith.science/api/pith-number/CM6NLLB6JEJOVFNX4VWLI37G4A/events.json","paper":"https://pith.science/paper/CM6NLLB6"},"agent_actions":{"view_html":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A","download_json":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A.json","view_paper":"https://pith.science/paper/CM6NLLB6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.04109&json=true","fetch_graph":"https://pith.science/api/pith-number/CM6NLLB6JEJOVFNX4VWLI37G4A/graph.json","fetch_events":"https://pith.science/api/pith-number/CM6NLLB6JEJOVFNX4VWLI37G4A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A/action/storage_attestation","attest_author":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A/action/author_attestation","sign_citation":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A/action/citation_signature","submit_replication":"https://pith.science/pith/CM6NLLB6JEJOVFNX4VWLI37G4A/action/replication_record"}},"created_at":"2026-07-05T06:33:04.281451+00:00","updated_at":"2026-07-05T06:33:04.281451+00:00"}