{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:VHKMNNTYPZM3ZRCFC6XQUSO5D7","short_pith_number":"pith:VHKMNNTY","schema_version":"1.0","canonical_sha256":"a9d4c6b6787e59bcc44517af0a49dd1ff5365c8493abf0de001de11201e78ad2","source":{"kind":"arxiv","id":"2606.21334","version":1},"attestation_state":"computed","paper":{"title":"All-sky modeling of Galactic emission at radio and microwave frequencies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Angela C. Taylor, Clive Dickinson, Duncan J. Watts, Gabriel A. Hoerning, Gilles Weymann-Despres, Hans K. Eriksen, Ingunn K. Wehus, Jamie Leech, J. Patrick Leahy, Melis O. Irfan, Michael E. Jones, Michael W. Peel, Roke Cepeda-Arroita, Stuart E. Harper, Timothy J. Pearson, Vasundhara Shaw","submitted_at":"2026-06-19T11:28:26Z","abstract_excerpt":"We present a new all-sky model of low-frequency diffuse Galactic emission in the regime where synchrotron, free-free, and spinning dust dominate. The model extends the Planck 2015 diffuse component-separation analysis by incorporating recent radio and microwave surveys. We fit 35 full- and partial-sky maps at 1 degree resolution, including S-PASS at 2.30 GHz, C-BASS at 4.76 GHz, and QUIJOTE at 10-20 GHz, together with reprocessed WMAP and Planck LFI data from the Cosmoglobe collaboration and Planck HFI channels. Using a Bayesian parametric approach with Commander, we derive spatially varying a"},"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":"2606.21334","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2026-06-19T11:28:26Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"630bbbe75a1927c594dcba03fbfb1f5aa613e3848e358c21cee0cc8fa52eaaa2","abstract_canon_sha256":"f62c6db50a078e956c0b0231e065785ab5ed203b98fd27c5d7cc77a3418c3dcc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-23T01:12:37.602706Z","signature_b64":"t//b9DgTGo2DsBr7Ek2sn0iOEKcf+4J0WZc6gqJn4ToDOA9Se5DMl91YjbvZ1CyoJZSX2b19/WzOA4dfstCvBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9d4c6b6787e59bcc44517af0a49dd1ff5365c8493abf0de001de11201e78ad2","last_reissued_at":"2026-06-23T01:12:37.602045Z","signature_status":"signed_v1","first_computed_at":"2026-06-23T01:12:37.602045Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"All-sky modeling of Galactic emission at radio and microwave frequencies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Angela C. Taylor, Clive Dickinson, Duncan J. Watts, Gabriel A. Hoerning, Gilles Weymann-Despres, Hans K. Eriksen, Ingunn K. Wehus, Jamie Leech, J. Patrick Leahy, Melis O. Irfan, Michael E. Jones, Michael W. Peel, Roke Cepeda-Arroita, Stuart E. Harper, Timothy J. Pearson, Vasundhara Shaw","submitted_at":"2026-06-19T11:28:26Z","abstract_excerpt":"We present a new all-sky model of low-frequency diffuse Galactic emission in the regime where synchrotron, free-free, and spinning dust dominate. The model extends the Planck 2015 diffuse component-separation analysis by incorporating recent radio and microwave surveys. We fit 35 full- and partial-sky maps at 1 degree resolution, including S-PASS at 2.30 GHz, C-BASS at 4.76 GHz, and QUIJOTE at 10-20 GHz, together with reprocessed WMAP and Planck LFI data from the Cosmoglobe collaboration and Planck HFI channels. Using a Bayesian parametric approach with Commander, we derive spatially varying a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.21334","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/2606.21334/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":"2606.21334","created_at":"2026-06-23T01:12:37.602121+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.21334v1","created_at":"2026-06-23T01:12:37.602121+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.21334","created_at":"2026-06-23T01:12:37.602121+00:00"},{"alias_kind":"pith_short_12","alias_value":"VHKMNNTYPZM3","created_at":"2026-06-23T01:12:37.602121+00:00"},{"alias_kind":"pith_short_16","alias_value":"VHKMNNTYPZM3ZRCF","created_at":"2026-06-23T01:12:37.602121+00:00"},{"alias_kind":"pith_short_8","alias_value":"VHKMNNTY","created_at":"2026-06-23T01:12:37.602121+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/VHKMNNTYPZM3ZRCFC6XQUSO5D7","json":"https://pith.science/pith/VHKMNNTYPZM3ZRCFC6XQUSO5D7.json","graph_json":"https://pith.science/api/pith-number/VHKMNNTYPZM3ZRCFC6XQUSO5D7/graph.json","events_json":"https://pith.science/api/pith-number/VHKMNNTYPZM3ZRCFC6XQUSO5D7/events.json","paper":"https://pith.science/paper/VHKMNNTY"},"agent_actions":{"view_html":"https://pith.science/pith/VHKMNNTYPZM3ZRCFC6XQUSO5D7","download_json":"https://pith.science/pith/VHKMNNTYPZM3ZRCFC6XQUSO5D7.json","view_paper":"https://pith.science/paper/VHKMNNTY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.21334&json=true","fetch_graph":"https://pith.science/api/pith-number/VHKMNNTYPZM3ZRCFC6XQUSO5D7/graph.json","fetch_events":"https://pith.science/api/pith-number/VHKMNNTYPZM3ZRCFC6XQUSO5D7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VHKMNNTYPZM3ZRCFC6XQUSO5D7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VHKMNNTYPZM3ZRCFC6XQUSO5D7/action/storage_attestation","attest_author":"https://pith.science/pith/VHKMNNTYPZM3ZRCFC6XQUSO5D7/action/author_attestation","sign_citation":"https://pith.science/pith/VHKMNNTYPZM3ZRCFC6XQUSO5D7/action/citation_signature","submit_replication":"https://pith.science/pith/VHKMNNTYPZM3ZRCFC6XQUSO5D7/action/replication_record"}},"created_at":"2026-06-23T01:12:37.602121+00:00","updated_at":"2026-06-23T01:12:37.602121+00:00"}