{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:B3GTXIOCFA4I742R2C6NCUZZD4","short_pith_number":"pith:B3GTXIOC","schema_version":"1.0","canonical_sha256":"0ecd3ba1c228388ff351d0bcd153391f05c0de89a45128afdcfb310f06e8f1f4","source":{"kind":"arxiv","id":"1502.06825","version":2},"attestation_state":"computed","paper":{"title":"Localising fast radio bursts and other transients using interferometric arrays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Benjamin Stappers, Monika Obrocka, Peter Wilkinson","submitted_at":"2015-02-24T14:47:12Z","abstract_excerpt":"A new population of sources emitting fast and bright transient radio bursts has recently been identified. The observed large dispersion measure values of FRBs suggests an extragalactic origin and an accurate determination of their positions and distances will provide an unique opportunity to study the magneto-ionic properties of the IGM. So far, FRBs have all been found using large dishes equipped with multi-pixel arrays. While large single dishes are well-suited for the discovery of transient sources they are poor at providing accurate localisations. A 2D snapshot image of the sky, made with "},"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":"1502.06825","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-02-24T14:47:12Z","cross_cats_sorted":[],"title_canon_sha256":"a121f76368b05961972d6e4d7e066099ec9abb3f175f01dd30ec648c5d62b699","abstract_canon_sha256":"6a4efd495c0b03805c58d4c315e39f9a3081a6e522ed3687fa1d3ba6d08dbd6f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:37:35.046309Z","signature_b64":"4C2obsGJdhIeoxK73xumTFCD6Whb2zdR1Xv925n0FaLN3rZylkiJfi4nNA4VdkUIDWkCnY65yJMYceSgudDeCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0ecd3ba1c228388ff351d0bcd153391f05c0de89a45128afdcfb310f06e8f1f4","last_reissued_at":"2026-05-18T01:37:35.045610Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:37:35.045610Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Localising fast radio bursts and other transients using interferometric arrays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Benjamin Stappers, Monika Obrocka, Peter Wilkinson","submitted_at":"2015-02-24T14:47:12Z","abstract_excerpt":"A new population of sources emitting fast and bright transient radio bursts has recently been identified. The observed large dispersion measure values of FRBs suggests an extragalactic origin and an accurate determination of their positions and distances will provide an unique opportunity to study the magneto-ionic properties of the IGM. So far, FRBs have all been found using large dishes equipped with multi-pixel arrays. While large single dishes are well-suited for the discovery of transient sources they are poor at providing accurate localisations. A 2D snapshot image of the sky, made with "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.06825","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":""},"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":"1502.06825","created_at":"2026-05-18T01:37:35.045718+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.06825v2","created_at":"2026-05-18T01:37:35.045718+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.06825","created_at":"2026-05-18T01:37:35.045718+00:00"},{"alias_kind":"pith_short_12","alias_value":"B3GTXIOCFA4I","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_16","alias_value":"B3GTXIOCFA4I742R","created_at":"2026-05-18T12:29:14.074870+00:00"},{"alias_kind":"pith_short_8","alias_value":"B3GTXIOC","created_at":"2026-05-18T12:29:14.074870+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/B3GTXIOCFA4I742R2C6NCUZZD4","json":"https://pith.science/pith/B3GTXIOCFA4I742R2C6NCUZZD4.json","graph_json":"https://pith.science/api/pith-number/B3GTXIOCFA4I742R2C6NCUZZD4/graph.json","events_json":"https://pith.science/api/pith-number/B3GTXIOCFA4I742R2C6NCUZZD4/events.json","paper":"https://pith.science/paper/B3GTXIOC"},"agent_actions":{"view_html":"https://pith.science/pith/B3GTXIOCFA4I742R2C6NCUZZD4","download_json":"https://pith.science/pith/B3GTXIOCFA4I742R2C6NCUZZD4.json","view_paper":"https://pith.science/paper/B3GTXIOC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.06825&json=true","fetch_graph":"https://pith.science/api/pith-number/B3GTXIOCFA4I742R2C6NCUZZD4/graph.json","fetch_events":"https://pith.science/api/pith-number/B3GTXIOCFA4I742R2C6NCUZZD4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/B3GTXIOCFA4I742R2C6NCUZZD4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/B3GTXIOCFA4I742R2C6NCUZZD4/action/storage_attestation","attest_author":"https://pith.science/pith/B3GTXIOCFA4I742R2C6NCUZZD4/action/author_attestation","sign_citation":"https://pith.science/pith/B3GTXIOCFA4I742R2C6NCUZZD4/action/citation_signature","submit_replication":"https://pith.science/pith/B3GTXIOCFA4I742R2C6NCUZZD4/action/replication_record"}},"created_at":"2026-05-18T01:37:35.045718+00:00","updated_at":"2026-05-18T01:37:35.045718+00:00"}