{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:Z5SSMB7GSS3TA4P7VSUOSEECC7","short_pith_number":"pith:Z5SSMB7G","schema_version":"1.0","canonical_sha256":"cf652607e694b73071ffaca8e9108217d626c996ee0f1b2db828b3334db4e8cb","source":{"kind":"arxiv","id":"2311.12120","version":4},"attestation_state":"computed","paper":{"title":"The Coherent Magnetic Field of the Milky Way","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Glennys R. Farrar, Michael Unger","submitted_at":"2023-11-20T19:02:15Z","abstract_excerpt":"We present a suite of models of the coherent magnetic field of the Galaxy (GMF) based on new divergence-free parametric functions describing the global structure of the field. The model parameters are fit to the latest full-sky Faraday rotation measures of extragalactic sources (RMs) and polarized synchrotron intensity (PI) maps from WMAP and Planck. We employ multiple models for the density of thermal and cosmic-ray electrons in the Galaxy, needed to predict the skymaps of RMs and PI for a given GMF model. The robustness of the inferred properties of the GMF is gauged by studying many combina"},"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":"2311.12120","kind":"arxiv","version":4},"metadata":{"license":"http://creativecommons.org/licenses/by-sa/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-11-20T19:02:15Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"70ceaa27bdf1f27443b1fc287c61926156daa2e7c7f4b11486409accd0b6737c","abstract_canon_sha256":"a996b717db01ace955e76c0290104c6db23a5aef8bc3bd01bc4b6030799da4d7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:54:45.105168Z","signature_b64":"+tKwWg44anUCXQId+Efh9uIS9EfkKxS4ClFvoXDLOwalA+KbIxModfkFGgX9adtL+I/BlkF7tKzl2wyZtInADQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cf652607e694b73071ffaca8e9108217d626c996ee0f1b2db828b3334db4e8cb","last_reissued_at":"2026-07-05T08:54:45.104742Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:54:45.104742Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Coherent Magnetic Field of the Milky Way","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Glennys R. Farrar, Michael Unger","submitted_at":"2023-11-20T19:02:15Z","abstract_excerpt":"We present a suite of models of the coherent magnetic field of the Galaxy (GMF) based on new divergence-free parametric functions describing the global structure of the field. The model parameters are fit to the latest full-sky Faraday rotation measures of extragalactic sources (RMs) and polarized synchrotron intensity (PI) maps from WMAP and Planck. We employ multiple models for the density of thermal and cosmic-ray electrons in the Galaxy, needed to predict the skymaps of RMs and PI for a given GMF model. The robustness of the inferred properties of the GMF is gauged by studying many combina"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.12120","kind":"arxiv","version":4},"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/2311.12120/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":"2311.12120","created_at":"2026-07-05T08:54:45.104798+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.12120v4","created_at":"2026-07-05T08:54:45.104798+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.12120","created_at":"2026-07-05T08:54:45.104798+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z5SSMB7GSS3T","created_at":"2026-07-05T08:54:45.104798+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z5SSMB7GSS3TA4P7","created_at":"2026-07-05T08:54:45.104798+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z5SSMB7G","created_at":"2026-07-05T08:54:45.104798+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":10,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07158","citing_title":"Weakly supervised machine learning for model-agnostic searches of new phenomena in the $\\gamma$-ray sky","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2606.15269","citing_title":"Line-of-sight magnetic-field propagation effects on axion-like particle constraints from GRB 221009A","ref_index":40,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28141","citing_title":"Transition from Diffusion to Drift-Dominated Cosmic Ray Transport and the Origin of the Knee","ref_index":56,"is_internal_anchor":false},{"citing_arxiv_id":"2504.02030","citing_title":"Neutron Star Eclipses as Axion Laboratories","ref_index":34,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15261","citing_title":"Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion","ref_index":67,"is_internal_anchor":false},{"citing_arxiv_id":"2505.21042","citing_title":"What exactly did the Transformer learn from our physics data?","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2509.13322","citing_title":"Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities","ref_index":30,"is_internal_anchor":false},{"citing_arxiv_id":"2510.08025","citing_title":"On the contribution of galaxies to the magnetic field in cosmic voids","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2604.01277","citing_title":"Lights, Camera, Axion: Tracing Axions from Supernovae in the Diffuse $\\gamma$-ray Sky","ref_index":128,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24446","citing_title":"Energy spectrum of magnetic fields from electroweak symmetry breaking","ref_index":6,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7","json":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7.json","graph_json":"https://pith.science/api/pith-number/Z5SSMB7GSS3TA4P7VSUOSEECC7/graph.json","events_json":"https://pith.science/api/pith-number/Z5SSMB7GSS3TA4P7VSUOSEECC7/events.json","paper":"https://pith.science/paper/Z5SSMB7G"},"agent_actions":{"view_html":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7","download_json":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7.json","view_paper":"https://pith.science/paper/Z5SSMB7G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.12120&json=true","fetch_graph":"https://pith.science/api/pith-number/Z5SSMB7GSS3TA4P7VSUOSEECC7/graph.json","fetch_events":"https://pith.science/api/pith-number/Z5SSMB7GSS3TA4P7VSUOSEECC7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7/action/storage_attestation","attest_author":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7/action/author_attestation","sign_citation":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7/action/citation_signature","submit_replication":"https://pith.science/pith/Z5SSMB7GSS3TA4P7VSUOSEECC7/action/replication_record"}},"created_at":"2026-07-05T08:54:45.104798+00:00","updated_at":"2026-07-05T08:54:45.104798+00:00"}