{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:SSAUSDJLSAL22RBX6OFEJ44H7T","short_pith_number":"pith:SSAUSDJL","schema_version":"1.0","canonical_sha256":"9481490d2b9017ad4437f38a44f387fcfbe794a59a3ce5b3dd6e045359d53eed","source":{"kind":"arxiv","id":"1405.5945","version":1},"attestation_state":"computed","paper":{"title":"An absence of fast radio bursts at intermediate galactic latitudes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Possenti, B. W. Stappers, C. Flynn, C. Ng, C. Tiburzi, D. Champion, D. Thornton, E. D. Barr, E. F. Keane, E. Petroff, L. Levin, M. Bailes, M. Burgay, M. J. Keith, M. Kramer, N. D. R. Bhat, P. Coster, S. Burke-Spolaor, S. D. Bates, S. Johnston, W. van Straten","submitted_at":"2014-05-23T01:41:22Z","abstract_excerpt":"Fast radio bursts (FRBs) are an emerging class of bright, highly dispersed radio pulses. Recent work by Thornton et al. (2013) has revealed a population of FRBs in the High Time Resolution Universe (HTRU) survey at high Galactic latitudes. A variety of progenitors have been proposed including cataclysmic events at cosmological distances, Galactic flare stars, and terrestrial radio frequency interference. Here we report on a search for FRBs at intermediate Galactic latitudes ($-15^{\\circ}$ $< b <$ 15$^{\\circ}$) in data taken as part of the HTRU survey. No FRBs were discovered in this region. Se"},"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":"1405.5945","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-05-23T01:41:22Z","cross_cats_sorted":[],"title_canon_sha256":"850604bd0bdda99a11da79ff5223e70045e2de899d58a9982187321155820879","abstract_canon_sha256":"9c595ddb23051931fa32f2b4dc1cef93fcbf9e5e2383618edf0536ec7832d465"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:07.202404Z","signature_b64":"h7NwZNLwCqPVe/vVKgTzimvdfZN8Ris1+FgcZYVkD4hNOsUjekCGKxfcwN8Cvqa07XiuHClAlthG+ILAmM2qBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9481490d2b9017ad4437f38a44f387fcfbe794a59a3ce5b3dd6e045359d53eed","last_reissued_at":"2026-05-18T01:43:07.201731Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:07.201731Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An absence of fast radio bursts at intermediate galactic latitudes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Possenti, B. W. Stappers, C. Flynn, C. Ng, C. Tiburzi, D. Champion, D. Thornton, E. D. Barr, E. F. Keane, E. Petroff, L. Levin, M. Bailes, M. Burgay, M. J. Keith, M. Kramer, N. D. R. Bhat, P. Coster, S. Burke-Spolaor, S. D. Bates, S. Johnston, W. van Straten","submitted_at":"2014-05-23T01:41:22Z","abstract_excerpt":"Fast radio bursts (FRBs) are an emerging class of bright, highly dispersed radio pulses. Recent work by Thornton et al. (2013) has revealed a population of FRBs in the High Time Resolution Universe (HTRU) survey at high Galactic latitudes. A variety of progenitors have been proposed including cataclysmic events at cosmological distances, Galactic flare stars, and terrestrial radio frequency interference. Here we report on a search for FRBs at intermediate Galactic latitudes ($-15^{\\circ}$ $< b <$ 15$^{\\circ}$) in data taken as part of the HTRU survey. No FRBs were discovered in this region. Se"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.5945","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":"1405.5945","created_at":"2026-05-18T01:43:07.201815+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.5945v1","created_at":"2026-05-18T01:43:07.201815+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.5945","created_at":"2026-05-18T01:43:07.201815+00:00"},{"alias_kind":"pith_short_12","alias_value":"SSAUSDJLSAL2","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"SSAUSDJLSAL22RBX","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"SSAUSDJL","created_at":"2026-05-18T12:28:49.207871+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/SSAUSDJLSAL22RBX6OFEJ44H7T","json":"https://pith.science/pith/SSAUSDJLSAL22RBX6OFEJ44H7T.json","graph_json":"https://pith.science/api/pith-number/SSAUSDJLSAL22RBX6OFEJ44H7T/graph.json","events_json":"https://pith.science/api/pith-number/SSAUSDJLSAL22RBX6OFEJ44H7T/events.json","paper":"https://pith.science/paper/SSAUSDJL"},"agent_actions":{"view_html":"https://pith.science/pith/SSAUSDJLSAL22RBX6OFEJ44H7T","download_json":"https://pith.science/pith/SSAUSDJLSAL22RBX6OFEJ44H7T.json","view_paper":"https://pith.science/paper/SSAUSDJL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.5945&json=true","fetch_graph":"https://pith.science/api/pith-number/SSAUSDJLSAL22RBX6OFEJ44H7T/graph.json","fetch_events":"https://pith.science/api/pith-number/SSAUSDJLSAL22RBX6OFEJ44H7T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SSAUSDJLSAL22RBX6OFEJ44H7T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SSAUSDJLSAL22RBX6OFEJ44H7T/action/storage_attestation","attest_author":"https://pith.science/pith/SSAUSDJLSAL22RBX6OFEJ44H7T/action/author_attestation","sign_citation":"https://pith.science/pith/SSAUSDJLSAL22RBX6OFEJ44H7T/action/citation_signature","submit_replication":"https://pith.science/pith/SSAUSDJLSAL22RBX6OFEJ44H7T/action/replication_record"}},"created_at":"2026-05-18T01:43:07.201815+00:00","updated_at":"2026-05-18T01:43:07.201815+00:00"}