{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:Q62UZ65CWHZEWHUUMIMYV2YAB7","short_pith_number":"pith:Q62UZ65C","schema_version":"1.0","canonical_sha256":"87b54cfba2b1f24b1e9462198aeb000fcd46caf38514178689f7b3c74e0fba62","source":{"kind":"arxiv","id":"1605.06074","version":1},"attestation_state":"computed","paper":{"title":"A Search for Highly Dispersed Fast Radio Bursts in Three Parkes Multibeam Surveys","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. Rane, D. R. Lorimer, F. Crawford, J. P. Ridley, K. Rolph, L. Tran","submitted_at":"2016-05-19T18:27:07Z","abstract_excerpt":"We have searched three Parkes multibeam 1.4 GHz surveys for the presence of fast radio bursts (FRBs) out to a dispersion measure (DM) of 5000 pc cm$^{-3}$. These surveys originally targeted the Magellanic Clouds (in two cases) and unidentified gamma-ray sources at mid-Galactic latitudes (in the third case) for new radio pulsars. In previous processing, none of these surveys were searched to such a high DM limit. The surveys had a combined total of 719 hr of Parkes multibeam on-sky time. One known FRB, 010724, was present in our data and was detected in our analysis but no new FRBs were found. "},"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":"1605.06074","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-05-19T18:27:07Z","cross_cats_sorted":["astro-ph.IM","astro-ph.SR"],"title_canon_sha256":"d391c663784d0c5befd25617458513cc4baec30728f929ac9bbf5aed438a6735","abstract_canon_sha256":"093b9b466e599e2464b2e14e6da73b777135a427ef33af7e4efd4bda9eb4734f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:10.895110Z","signature_b64":"XH5tM1I/Pb1hFeM5LnyPqiWM2MKidb/5hc0n+/Y0YmB96o1yWYre/IBekP9xdzONDzKph9dwjYNK8Flnh6u8DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"87b54cfba2b1f24b1e9462198aeb000fcd46caf38514178689f7b3c74e0fba62","last_reissued_at":"2026-05-18T01:13:10.894717Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:10.894717Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Search for Highly Dispersed Fast Radio Bursts in Three Parkes Multibeam Surveys","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. Rane, D. R. Lorimer, F. Crawford, J. P. Ridley, K. Rolph, L. Tran","submitted_at":"2016-05-19T18:27:07Z","abstract_excerpt":"We have searched three Parkes multibeam 1.4 GHz surveys for the presence of fast radio bursts (FRBs) out to a dispersion measure (DM) of 5000 pc cm$^{-3}$. These surveys originally targeted the Magellanic Clouds (in two cases) and unidentified gamma-ray sources at mid-Galactic latitudes (in the third case) for new radio pulsars. In previous processing, none of these surveys were searched to such a high DM limit. The surveys had a combined total of 719 hr of Parkes multibeam on-sky time. One known FRB, 010724, was present in our data and was detected in our analysis but no new FRBs were found. "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.06074","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":"1605.06074","created_at":"2026-05-18T01:13:10.894782+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.06074v1","created_at":"2026-05-18T01:13:10.894782+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.06074","created_at":"2026-05-18T01:13:10.894782+00:00"},{"alias_kind":"pith_short_12","alias_value":"Q62UZ65CWHZE","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"Q62UZ65CWHZEWHUU","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"Q62UZ65C","created_at":"2026-05-18T12:30:39.010887+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/Q62UZ65CWHZEWHUUMIMYV2YAB7","json":"https://pith.science/pith/Q62UZ65CWHZEWHUUMIMYV2YAB7.json","graph_json":"https://pith.science/api/pith-number/Q62UZ65CWHZEWHUUMIMYV2YAB7/graph.json","events_json":"https://pith.science/api/pith-number/Q62UZ65CWHZEWHUUMIMYV2YAB7/events.json","paper":"https://pith.science/paper/Q62UZ65C"},"agent_actions":{"view_html":"https://pith.science/pith/Q62UZ65CWHZEWHUUMIMYV2YAB7","download_json":"https://pith.science/pith/Q62UZ65CWHZEWHUUMIMYV2YAB7.json","view_paper":"https://pith.science/paper/Q62UZ65C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.06074&json=true","fetch_graph":"https://pith.science/api/pith-number/Q62UZ65CWHZEWHUUMIMYV2YAB7/graph.json","fetch_events":"https://pith.science/api/pith-number/Q62UZ65CWHZEWHUUMIMYV2YAB7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Q62UZ65CWHZEWHUUMIMYV2YAB7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Q62UZ65CWHZEWHUUMIMYV2YAB7/action/storage_attestation","attest_author":"https://pith.science/pith/Q62UZ65CWHZEWHUUMIMYV2YAB7/action/author_attestation","sign_citation":"https://pith.science/pith/Q62UZ65CWHZEWHUUMIMYV2YAB7/action/citation_signature","submit_replication":"https://pith.science/pith/Q62UZ65CWHZEWHUUMIMYV2YAB7/action/replication_record"}},"created_at":"2026-05-18T01:13:10.894782+00:00","updated_at":"2026-05-18T01:13:10.894782+00:00"}