{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:J6Z2P7TCJQXRDBVFSQIYQTFO5E","short_pith_number":"pith:J6Z2P7TC","schema_version":"1.0","canonical_sha256":"4fb3a7fe624c2f1186a59411884caee93574e9bda723911d6fe8003916aa17c3","source":{"kind":"arxiv","id":"2607.03314","version":1},"attestation_state":"computed","paper":{"title":"Exploring the Magnetic Field Structure of the Milky Way with Pulsars in the SKA Era","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"J. L. Han, Jun Xu, WeiCong Jing","submitted_at":"2026-07-03T13:30:58Z","abstract_excerpt":"The magnetic field structure of the Milky Way can offer critical insights into the origin of galactic magnetic fields. Measurements of magnetic structures of the Milky Way are still sparse in far regions of the Galactic disk and halo. Pulsars are the best probes for the three-dimensional structure of the Galactic magnetic field, primarily owing to their highly polarized short-duration radio pulses, negligible intrinsic Faraday rotation compared to the contribution from the medium in front, and their widespread distribution throughout the Galaxy across the thin disk, spiral arms, and extended h"},"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":"2607.03314","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-07-03T13:30:58Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"0f6cf02c68fd22adfcf6ebc84726ae03484c63244ea01bdae75fd07de733478e","abstract_canon_sha256":"19e7ccdcbdc54d5b0378b42e602fd541edff1c1c5d435e5def342aeba24586e8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-07T02:17:36.905892Z","signature_b64":"FXYb4T2Ls9mzXvC3tHMBThg3qefZc48m2s9KWnUWukZ/KFlzGw89GvTB9TLhj4LncWwgf0ECQc89ZJOJxx4FBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4fb3a7fe624c2f1186a59411884caee93574e9bda723911d6fe8003916aa17c3","last_reissued_at":"2026-07-07T02:17:36.905148Z","signature_status":"signed_v1","first_computed_at":"2026-07-07T02:17:36.905148Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring the Magnetic Field Structure of the Milky Way with Pulsars in the SKA Era","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"J. L. Han, Jun Xu, WeiCong Jing","submitted_at":"2026-07-03T13:30:58Z","abstract_excerpt":"The magnetic field structure of the Milky Way can offer critical insights into the origin of galactic magnetic fields. Measurements of magnetic structures of the Milky Way are still sparse in far regions of the Galactic disk and halo. Pulsars are the best probes for the three-dimensional structure of the Galactic magnetic field, primarily owing to their highly polarized short-duration radio pulses, negligible intrinsic Faraday rotation compared to the contribution from the medium in front, and their widespread distribution throughout the Galaxy across the thin disk, spiral arms, and extended h"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.03314","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/2607.03314/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":"2607.03314","created_at":"2026-07-07T02:17:36.905248+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.03314v1","created_at":"2026-07-07T02:17:36.905248+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.03314","created_at":"2026-07-07T02:17:36.905248+00:00"},{"alias_kind":"pith_short_12","alias_value":"J6Z2P7TCJQXR","created_at":"2026-07-07T02:17:36.905248+00:00"},{"alias_kind":"pith_short_16","alias_value":"J6Z2P7TCJQXRDBVF","created_at":"2026-07-07T02:17:36.905248+00:00"},{"alias_kind":"pith_short_8","alias_value":"J6Z2P7TC","created_at":"2026-07-07T02:17:36.905248+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/J6Z2P7TCJQXRDBVFSQIYQTFO5E","json":"https://pith.science/pith/J6Z2P7TCJQXRDBVFSQIYQTFO5E.json","graph_json":"https://pith.science/api/pith-number/J6Z2P7TCJQXRDBVFSQIYQTFO5E/graph.json","events_json":"https://pith.science/api/pith-number/J6Z2P7TCJQXRDBVFSQIYQTFO5E/events.json","paper":"https://pith.science/paper/J6Z2P7TC"},"agent_actions":{"view_html":"https://pith.science/pith/J6Z2P7TCJQXRDBVFSQIYQTFO5E","download_json":"https://pith.science/pith/J6Z2P7TCJQXRDBVFSQIYQTFO5E.json","view_paper":"https://pith.science/paper/J6Z2P7TC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.03314&json=true","fetch_graph":"https://pith.science/api/pith-number/J6Z2P7TCJQXRDBVFSQIYQTFO5E/graph.json","fetch_events":"https://pith.science/api/pith-number/J6Z2P7TCJQXRDBVFSQIYQTFO5E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J6Z2P7TCJQXRDBVFSQIYQTFO5E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J6Z2P7TCJQXRDBVFSQIYQTFO5E/action/storage_attestation","attest_author":"https://pith.science/pith/J6Z2P7TCJQXRDBVFSQIYQTFO5E/action/author_attestation","sign_citation":"https://pith.science/pith/J6Z2P7TCJQXRDBVFSQIYQTFO5E/action/citation_signature","submit_replication":"https://pith.science/pith/J6Z2P7TCJQXRDBVFSQIYQTFO5E/action/replication_record"}},"created_at":"2026-07-07T02:17:36.905248+00:00","updated_at":"2026-07-07T02:17:36.905248+00:00"}