{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:XOA2VE3TYHCE7WEGQFDDMWTJ7S","short_pith_number":"pith:XOA2VE3T","schema_version":"1.0","canonical_sha256":"bb81aa9373c1c44fd8868146365a69fca30cb2a14637bb45b6a21864737f007f","source":{"kind":"arxiv","id":"2607.09964","version":1},"attestation_state":"computed","paper":{"title":"Faraday depth similarities across scales with LoTSS & DRAGONS","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alex S. Hill, Ana Erceg, Anna Ordog, Jo-Anne C. Brown, Marijke Haverkorn, Rebecca A. Booth, T.L. Landecker, Vibor Jeli\\'c","submitted_at":"2026-07-10T20:43:09Z","abstract_excerpt":"Faraday rotation of diffuse Galactic synchrotron emission is a powerful tracer of the complex, magnetised interstellar medium (ISM), whose structures span a wide range of spatial scales, requiring both interferometric and single-antenna broadband radio polarisation observations for full characterisation. We compare Faraday rotation in the interferometric LOw-Frequency ARray Two-Metre Sky Survey (LoTSS; 120-168 MHz) and the single-antenna Dominion Radio Astrophysical Observatory Global Magneto-Ionic Medium Survey of the Northern Sky (DRAGONS; 350-1030 MHz), which are complementary in their sens"},"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":"2607.09964","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2026-07-10T20:43:09Z","cross_cats_sorted":[],"title_canon_sha256":"7c0d99cfd9e2934cba53c2b3dc6ff5281325acb4ee2092d83d2b8c79d8378bfb","abstract_canon_sha256":"3fce2078fa01da669656c1e484eab5b9fbd7c9f6d58c8353a83912765cf0d4af"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-14T00:18:45.136667Z","signature_b64":"lwcxuC6CLA/tJ3fG+Ur9vVql2+7724LQ8MsMOK4sT0DBzXM8MXGbreFzkEz6C4aPcPIKHtLcy7ll56nNvH40AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bb81aa9373c1c44fd8868146365a69fca30cb2a14637bb45b6a21864737f007f","last_reissued_at":"2026-07-14T00:18:45.135809Z","signature_status":"signed_v1","first_computed_at":"2026-07-14T00:18:45.135809Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Faraday depth similarities across scales with LoTSS & DRAGONS","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alex S. Hill, Ana Erceg, Anna Ordog, Jo-Anne C. Brown, Marijke Haverkorn, Rebecca A. Booth, T.L. Landecker, Vibor Jeli\\'c","submitted_at":"2026-07-10T20:43:09Z","abstract_excerpt":"Faraday rotation of diffuse Galactic synchrotron emission is a powerful tracer of the complex, magnetised interstellar medium (ISM), whose structures span a wide range of spatial scales, requiring both interferometric and single-antenna broadband radio polarisation observations for full characterisation. We compare Faraday rotation in the interferometric LOw-Frequency ARray Two-Metre Sky Survey (LoTSS; 120-168 MHz) and the single-antenna Dominion Radio Astrophysical Observatory Global Magneto-Ionic Medium Survey of the Northern Sky (DRAGONS; 350-1030 MHz), which are complementary in their sens"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.09964","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/2607.09964/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":"2607.09964","created_at":"2026-07-14T00:18:45.136254+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.09964v1","created_at":"2026-07-14T00:18:45.136254+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.09964","created_at":"2026-07-14T00:18:45.136254+00:00"},{"alias_kind":"pith_short_12","alias_value":"XOA2VE3TYHCE","created_at":"2026-07-14T00:18:45.136254+00:00"},{"alias_kind":"pith_short_16","alias_value":"XOA2VE3TYHCE7WEG","created_at":"2026-07-14T00:18:45.136254+00:00"},{"alias_kind":"pith_short_8","alias_value":"XOA2VE3T","created_at":"2026-07-14T00:18:45.136254+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/XOA2VE3TYHCE7WEGQFDDMWTJ7S","json":"https://pith.science/pith/XOA2VE3TYHCE7WEGQFDDMWTJ7S.json","graph_json":"https://pith.science/api/pith-number/XOA2VE3TYHCE7WEGQFDDMWTJ7S/graph.json","events_json":"https://pith.science/api/pith-number/XOA2VE3TYHCE7WEGQFDDMWTJ7S/events.json","paper":"https://pith.science/paper/XOA2VE3T"},"agent_actions":{"view_html":"https://pith.science/pith/XOA2VE3TYHCE7WEGQFDDMWTJ7S","download_json":"https://pith.science/pith/XOA2VE3TYHCE7WEGQFDDMWTJ7S.json","view_paper":"https://pith.science/paper/XOA2VE3T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.09964&json=true","fetch_graph":"https://pith.science/api/pith-number/XOA2VE3TYHCE7WEGQFDDMWTJ7S/graph.json","fetch_events":"https://pith.science/api/pith-number/XOA2VE3TYHCE7WEGQFDDMWTJ7S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XOA2VE3TYHCE7WEGQFDDMWTJ7S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XOA2VE3TYHCE7WEGQFDDMWTJ7S/action/storage_attestation","attest_author":"https://pith.science/pith/XOA2VE3TYHCE7WEGQFDDMWTJ7S/action/author_attestation","sign_citation":"https://pith.science/pith/XOA2VE3TYHCE7WEGQFDDMWTJ7S/action/citation_signature","submit_replication":"https://pith.science/pith/XOA2VE3TYHCE7WEGQFDDMWTJ7S/action/replication_record"}},"created_at":"2026-07-14T00:18:45.136254+00:00","updated_at":"2026-07-14T00:18:45.136254+00:00"}