{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:TCN2XFORRFESNVEHADO5UTODDG","short_pith_number":"pith:TCN2XFOR","schema_version":"1.0","canonical_sha256":"989bab95d1894926d48700ddda4dc319860b819163bbe8b33b30a3f4f94e7aa0","source":{"kind":"arxiv","id":"1307.1628","version":1},"attestation_state":"computed","paper":{"title":"A Population of Fast Radio Bursts at Cosmological Distances","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"A. Jameson, A. Possenti, B. R. Barsdell, B. Stappers, C. Ng, D. J. Champion, D. Thornton, L. Levin, M. Bailes, M. Burgay, M. J. Keith, M. Kramer, N. d'Amico, N. D. R. Bhat, P. Coster, S. Burke-Spolaor, S. D. Bates, S. Johnston, S. Milia, W. van Straten","submitted_at":"2013-07-05T14:57:22Z","abstract_excerpt":"Searches for transient astrophysical sources often reveal unexpected classes of objects that are useful physical laboratories. In a recent survey for pulsars and fast transients we have uncovered four millisecond-duration radio transients all more than 40{\\deg} from the Galactic plane. The bursts' properties indicate that they are of celestial rather than terrestrial origin. Host galaxy and intergalactic medium models suggest that they have cosmological redshifts of 0.5 to 1, and distances of up to 3 gigaparsecs. No temporally coincident x- or gamma-ray signature was identified in association "},"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":"1307.1628","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-07-05T14:57:22Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"a00a3920d205ea41550908f434521abbe2b1d340a3780257345b39b2dcfb3a5b","abstract_canon_sha256":"62eeac35d801133d4082733f18c3e53e63abc0f30d6fdd5ef0bb2fe3ba97fde3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:19:12.356444Z","signature_b64":"wH12V1t07fYZmaDVO5MF8+eSuc1axxNS7AwitgVmQP2hWgyZjL1ZjKOQYpSdpU3cvJHiJXIuuN9xR2T6f6kBCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"989bab95d1894926d48700ddda4dc319860b819163bbe8b33b30a3f4f94e7aa0","last_reissued_at":"2026-05-18T03:19:12.355891Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:19:12.355891Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Population of Fast Radio Bursts at Cosmological Distances","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"A. Jameson, A. Possenti, B. R. Barsdell, B. Stappers, C. Ng, D. J. Champion, D. Thornton, L. Levin, M. Bailes, M. Burgay, M. J. Keith, M. Kramer, N. d'Amico, N. D. R. Bhat, P. Coster, S. Burke-Spolaor, S. D. Bates, S. Johnston, S. Milia, W. van Straten","submitted_at":"2013-07-05T14:57:22Z","abstract_excerpt":"Searches for transient astrophysical sources often reveal unexpected classes of objects that are useful physical laboratories. In a recent survey for pulsars and fast transients we have uncovered four millisecond-duration radio transients all more than 40{\\deg} from the Galactic plane. The bursts' properties indicate that they are of celestial rather than terrestrial origin. Host galaxy and intergalactic medium models suggest that they have cosmological redshifts of 0.5 to 1, and distances of up to 3 gigaparsecs. No temporally coincident x- or gamma-ray signature was identified in association "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.1628","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":""},"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":"1307.1628","created_at":"2026-05-18T03:19:12.355979+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.1628v1","created_at":"2026-05-18T03:19:12.355979+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.1628","created_at":"2026-05-18T03:19:12.355979+00:00"},{"alias_kind":"pith_short_12","alias_value":"TCN2XFORRFES","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"TCN2XFORRFESNVEH","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"TCN2XFOR","created_at":"2026-05-18T12:27:59.945178+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.04897","citing_title":"Fast Radio Burst Dispersion Measure--Timing Cross-Correlations: Bias Self-Calibration and Primordial Non-Gaussianity Constraints","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2604.12775","citing_title":"Gravitational Gertsenshtein-Zeldovich mechanism for the Association between GW190425 and FRB 20190425A","ref_index":2,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG","json":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG.json","graph_json":"https://pith.science/api/pith-number/TCN2XFORRFESNVEHADO5UTODDG/graph.json","events_json":"https://pith.science/api/pith-number/TCN2XFORRFESNVEHADO5UTODDG/events.json","paper":"https://pith.science/paper/TCN2XFOR"},"agent_actions":{"view_html":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG","download_json":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG.json","view_paper":"https://pith.science/paper/TCN2XFOR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.1628&json=true","fetch_graph":"https://pith.science/api/pith-number/TCN2XFORRFESNVEHADO5UTODDG/graph.json","fetch_events":"https://pith.science/api/pith-number/TCN2XFORRFESNVEHADO5UTODDG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG/action/storage_attestation","attest_author":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG/action/author_attestation","sign_citation":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG/action/citation_signature","submit_replication":"https://pith.science/pith/TCN2XFORRFESNVEHADO5UTODDG/action/replication_record"}},"created_at":"2026-05-18T03:19:12.355979+00:00","updated_at":"2026-05-18T03:19:12.355979+00:00"}