{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:X73N7FPCLUABLSRKW422KAOMUY","short_pith_number":"pith:X73N7FPC","schema_version":"1.0","canonical_sha256":"bff6df95e25d0015ca2ab735a501cca62030d89f1721bf314e22a69ee1ff75fd","source":{"kind":"arxiv","id":"astro-ph/0304364","version":3},"attestation_state":"computed","paper":{"title":"Searches for Fast Radio Transients","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"J. M. Cordes & M. A. McLaughlin","submitted_at":"2003-04-21T13:44:17Z","abstract_excerpt":"We discuss optimal detection of fast radio transients from astrophysical objects while taking into account the effects of propagation through intervening ionized media, including dispersion, scattering and scintillation.Our analysis applies to the giant-pulse phenomenon exhibited by some pulsars, for which we show examples, and to radio pulses from other astrophysical sources, such as prompt radio emission from gamma-ray burst sources and modulated signals from extra-terrestrial civilizations."},"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":"astro-ph/0304364","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-04-21T13:44:17Z","cross_cats_sorted":[],"title_canon_sha256":"0f383cd3fe290c1fe15532edde2d295f014c2710c6af393e671493381dc72537","abstract_canon_sha256":"9e59bdd4a7916f3ab4b7d20b6806b55ef471e6646d43007d1646f31a2931e477"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:36:53.636288Z","signature_b64":"UWeAwMlf5MFqGQIIW50jYoO4NGI6UHHXeaNyEPZB6V1VTiasv8NgIJZbGyvbgMVUo1MJ/AtIKfP8Oz1vFmKJAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bff6df95e25d0015ca2ab735a501cca62030d89f1721bf314e22a69ee1ff75fd","last_reissued_at":"2026-07-04T16:36:53.635833Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:36:53.635833Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Searches for Fast Radio Transients","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"J. M. Cordes & M. A. McLaughlin","submitted_at":"2003-04-21T13:44:17Z","abstract_excerpt":"We discuss optimal detection of fast radio transients from astrophysical objects while taking into account the effects of propagation through intervening ionized media, including dispersion, scattering and scintillation.Our analysis applies to the giant-pulse phenomenon exhibited by some pulsars, for which we show examples, and to radio pulses from other astrophysical sources, such as prompt radio emission from gamma-ray burst sources and modulated signals from extra-terrestrial civilizations."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0304364","kind":"arxiv","version":3},"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/astro-ph/0304364/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":"astro-ph/0304364","created_at":"2026-07-04T16:36:53.635918+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0304364v3","created_at":"2026-07-04T16:36:53.635918+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0304364","created_at":"2026-07-04T16:36:53.635918+00:00"},{"alias_kind":"pith_short_12","alias_value":"X73N7FPCLUAB","created_at":"2026-07-04T16:36:53.635918+00:00"},{"alias_kind":"pith_short_16","alias_value":"X73N7FPCLUABLSRK","created_at":"2026-07-04T16:36:53.635918+00:00"},{"alias_kind":"pith_short_8","alias_value":"X73N7FPC","created_at":"2026-07-04T16:36:53.635918+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2607.08106","citing_title":"The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars","ref_index":38,"is_internal_anchor":true},{"citing_arxiv_id":"2607.08657","citing_title":"VAPOLA -- A multi-year, multi-band polarization survey of AGN and Sgr A* at mm wavelengths with ALMA I. Survey Overview and Science-Ready Archival Products","ref_index":225,"is_internal_anchor":true},{"citing_arxiv_id":"2606.26334","citing_title":"Debiasing the Observed Fast Radio Burst Population with the CHIME/FRB Selection Function","ref_index":52,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21331","citing_title":"Searching for links between energetic millisecond pulsars and repeating fast radio bursts","ref_index":117,"is_internal_anchor":true},{"citing_arxiv_id":"2512.17214","citing_title":"Pulsed radio emission from a Central Compact Object","ref_index":53,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY","json":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY.json","graph_json":"https://pith.science/api/pith-number/X73N7FPCLUABLSRKW422KAOMUY/graph.json","events_json":"https://pith.science/api/pith-number/X73N7FPCLUABLSRKW422KAOMUY/events.json","paper":"https://pith.science/paper/X73N7FPC"},"agent_actions":{"view_html":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY","download_json":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY.json","view_paper":"https://pith.science/paper/X73N7FPC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0304364&json=true","fetch_graph":"https://pith.science/api/pith-number/X73N7FPCLUABLSRKW422KAOMUY/graph.json","fetch_events":"https://pith.science/api/pith-number/X73N7FPCLUABLSRKW422KAOMUY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY/action/storage_attestation","attest_author":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY/action/author_attestation","sign_citation":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY/action/citation_signature","submit_replication":"https://pith.science/pith/X73N7FPCLUABLSRKW422KAOMUY/action/replication_record"}},"created_at":"2026-07-04T16:36:53.635918+00:00","updated_at":"2026-07-04T16:36:53.635918+00:00"}