{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:KWVV2Z3ZSCTJCU4JVWMPLK4O7H","short_pith_number":"pith:KWVV2Z3Z","schema_version":"1.0","canonical_sha256":"55ab5d677990a6915389ad98f5ab8ef9d77b3a0e7b0d22f24fa2b49835720b99","source":{"kind":"arxiv","id":"2605.19482","version":1},"attestation_state":"computed","paper":{"title":"Methodological Synergies between Technosignature and UHE Neutrino Searches","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.data-an"],"primary_cat":"astro-ph.IM","authors_text":"Paramita Dasgupta","submitted_at":"2026-05-19T07:34:21Z","abstract_excerpt":"Radio technosignature searches and radio-based ultra-high energy (UHE) neutrino experiments address different scientific questions, but share a closely related data analysis problem: identifying rare signals of unknown morphology within large datasets dominated by thermal noise and anthropogenic radio-frequency interference (RFI). UHE neutrino radio experiments (including ARA, RNO-G, ANITA, and PUEO) have developed advanced methodologies for continuous-wave (CW) mitigation and background characterization. This invited contribution makes that connection concrete through three points. First, we "},"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":"2605.19482","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2026-05-19T07:34:21Z","cross_cats_sorted":["astro-ph.HE","physics.data-an"],"title_canon_sha256":"fe0e5c3688fc1a0c6b17dbbdae630f5eaed21e168977bfb16c808181871aff28","abstract_canon_sha256":"8b2ea8a50c0493a4eae99b8e3fd97ff8f34ffeba7ac67bf75f0776e208b86e2b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-20T01:05:47.946644Z","signature_b64":"0iH1Ej5X5JNn/8wHNKvAo/ruzF9S3Nl6++FKyyAXWgGVxEgdsqLV+BSanqlpwoSzx/8t588BrYQPvothqvUdDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"55ab5d677990a6915389ad98f5ab8ef9d77b3a0e7b0d22f24fa2b49835720b99","last_reissued_at":"2026-05-20T01:05:47.946098Z","signature_status":"signed_v1","first_computed_at":"2026-05-20T01:05:47.946098Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Methodological Synergies between Technosignature and UHE Neutrino Searches","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.data-an"],"primary_cat":"astro-ph.IM","authors_text":"Paramita Dasgupta","submitted_at":"2026-05-19T07:34:21Z","abstract_excerpt":"Radio technosignature searches and radio-based ultra-high energy (UHE) neutrino experiments address different scientific questions, but share a closely related data analysis problem: identifying rare signals of unknown morphology within large datasets dominated by thermal noise and anthropogenic radio-frequency interference (RFI). UHE neutrino radio experiments (including ARA, RNO-G, ANITA, and PUEO) have developed advanced methodologies for continuous-wave (CW) mitigation and background characterization. This invited contribution makes that connection concrete through three points. First, we "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.19482","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2605.19482/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":"2605.19482","created_at":"2026-05-20T01:05:47.946188+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.19482v1","created_at":"2026-05-20T01:05:47.946188+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.19482","created_at":"2026-05-20T01:05:47.946188+00:00"},{"alias_kind":"pith_short_12","alias_value":"KWVV2Z3ZSCTJ","created_at":"2026-05-20T01:05:47.946188+00:00"},{"alias_kind":"pith_short_16","alias_value":"KWVV2Z3ZSCTJCU4J","created_at":"2026-05-20T01:05:47.946188+00:00"},{"alias_kind":"pith_short_8","alias_value":"KWVV2Z3Z","created_at":"2026-05-20T01:05:47.946188+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/KWVV2Z3ZSCTJCU4JVWMPLK4O7H","json":"https://pith.science/pith/KWVV2Z3ZSCTJCU4JVWMPLK4O7H.json","graph_json":"https://pith.science/api/pith-number/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/graph.json","events_json":"https://pith.science/api/pith-number/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/events.json","paper":"https://pith.science/paper/KWVV2Z3Z"},"agent_actions":{"view_html":"https://pith.science/pith/KWVV2Z3ZSCTJCU4JVWMPLK4O7H","download_json":"https://pith.science/pith/KWVV2Z3ZSCTJCU4JVWMPLK4O7H.json","view_paper":"https://pith.science/paper/KWVV2Z3Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.19482&json=true","fetch_graph":"https://pith.science/api/pith-number/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/graph.json","fetch_events":"https://pith.science/api/pith-number/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/action/storage_attestation","attest_author":"https://pith.science/pith/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/action/author_attestation","sign_citation":"https://pith.science/pith/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/action/citation_signature","submit_replication":"https://pith.science/pith/KWVV2Z3ZSCTJCU4JVWMPLK4O7H/action/replication_record"}},"created_at":"2026-05-20T01:05:47.946188+00:00","updated_at":"2026-05-20T01:05:47.946188+00:00"}