{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:3DJXYOSYEG5HRE3BV4IIWKSCUM","short_pith_number":"pith:3DJXYOSY","schema_version":"1.0","canonical_sha256":"d8d37c3a5821ba789361af108b2a42a31dd8a3d889aae5fe91e2d87a8c426ddb","source":{"kind":"arxiv","id":"2301.05116","version":1},"attestation_state":"computed","paper":{"title":"QUIJOTE Scientific Results -- VII. Galactic AME sources in the QUIJOTE-MFI Northern Hemisphere Wide-Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. N. Lasenby, B. Ruiz-Granados, C. H. L\\'opez-Caraballo, D. Herranz, D. Tramonte, E. Artal, E. de la Hoz, E. Martinez-Gonzalez, F. Guidi, F. J. Casas, F. Poidevin, F. Vansyngel, J. A. Rubi\\~no-Mart\\'in, L. Piccirillo, M. Ashdown, M. Fern\\'andez-Torreiro, M. W. Peel, P. Vielva, R. A. Watson, R. B. Barreiro, R. J. Hoyland, R. Rebolo, R. T. G\\'enova-Santos","submitted_at":"2023-01-12T16:17:35Z","abstract_excerpt":"The QUIJOTE-MFI Northern Hemisphere Wide-Survey has provided maps of the sky above declinations $-30^\\circ$ at 11, 13, 17 and 19$\\,$GHz. These data are combined with ancillary data to produce Spectral Energy Distributions in intensity in the frequency range 0.4--3\\,000$\\,$GHz on a sample of 52 candidate compact sources harbouring anomalous microwave emission (AME). We apply a component separation analysis at 1$^\\circ$ scale on the full sample from which we identify 44 sources with high AME significance. We explore correlations between different fitted parameters on this last sample. QUIJOTE-MF"},"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":"2301.05116","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-01-12T16:17:35Z","cross_cats_sorted":[],"title_canon_sha256":"8b5c119335e0cd243ff7c78f693b55d278bb9f5d265095e02398e3049b1da096","abstract_canon_sha256":"b0b6375f9b26081e357ab7ff46de324fe3f99cc96645950c50e60e7070147dc4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:32:40.571469Z","signature_b64":"r+ZGOX0tac9V/6qvTp1aLK+v2ay3crWf+c2SHWWtNreb/RPpGnf5AujfR1YhJ5rOqniZQbTfUatLWJFowrdtBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d8d37c3a5821ba789361af108b2a42a31dd8a3d889aae5fe91e2d87a8c426ddb","last_reissued_at":"2026-07-05T05:32:40.570975Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:32:40.570975Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"QUIJOTE Scientific Results -- VII. Galactic AME sources in the QUIJOTE-MFI Northern Hemisphere Wide-Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. N. Lasenby, B. Ruiz-Granados, C. H. L\\'opez-Caraballo, D. Herranz, D. Tramonte, E. Artal, E. de la Hoz, E. Martinez-Gonzalez, F. Guidi, F. J. Casas, F. Poidevin, F. Vansyngel, J. A. Rubi\\~no-Mart\\'in, L. Piccirillo, M. Ashdown, M. Fern\\'andez-Torreiro, M. W. Peel, P. Vielva, R. A. Watson, R. B. Barreiro, R. J. Hoyland, R. Rebolo, R. T. G\\'enova-Santos","submitted_at":"2023-01-12T16:17:35Z","abstract_excerpt":"The QUIJOTE-MFI Northern Hemisphere Wide-Survey has provided maps of the sky above declinations $-30^\\circ$ at 11, 13, 17 and 19$\\,$GHz. These data are combined with ancillary data to produce Spectral Energy Distributions in intensity in the frequency range 0.4--3\\,000$\\,$GHz on a sample of 52 candidate compact sources harbouring anomalous microwave emission (AME). We apply a component separation analysis at 1$^\\circ$ scale on the full sample from which we identify 44 sources with high AME significance. We explore correlations between different fitted parameters on this last sample. QUIJOTE-MF"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2301.05116","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/2301.05116/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":"2301.05116","created_at":"2026-07-05T05:32:40.571032+00:00"},{"alias_kind":"arxiv_version","alias_value":"2301.05116v1","created_at":"2026-07-05T05:32:40.571032+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2301.05116","created_at":"2026-07-05T05:32:40.571032+00:00"},{"alias_kind":"pith_short_12","alias_value":"3DJXYOSYEG5H","created_at":"2026-07-05T05:32:40.571032+00:00"},{"alias_kind":"pith_short_16","alias_value":"3DJXYOSYEG5HRE3B","created_at":"2026-07-05T05:32:40.571032+00:00"},{"alias_kind":"pith_short_8","alias_value":"3DJXYOSY","created_at":"2026-07-05T05:32:40.571032+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/3DJXYOSYEG5HRE3BV4IIWKSCUM","json":"https://pith.science/pith/3DJXYOSYEG5HRE3BV4IIWKSCUM.json","graph_json":"https://pith.science/api/pith-number/3DJXYOSYEG5HRE3BV4IIWKSCUM/graph.json","events_json":"https://pith.science/api/pith-number/3DJXYOSYEG5HRE3BV4IIWKSCUM/events.json","paper":"https://pith.science/paper/3DJXYOSY"},"agent_actions":{"view_html":"https://pith.science/pith/3DJXYOSYEG5HRE3BV4IIWKSCUM","download_json":"https://pith.science/pith/3DJXYOSYEG5HRE3BV4IIWKSCUM.json","view_paper":"https://pith.science/paper/3DJXYOSY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2301.05116&json=true","fetch_graph":"https://pith.science/api/pith-number/3DJXYOSYEG5HRE3BV4IIWKSCUM/graph.json","fetch_events":"https://pith.science/api/pith-number/3DJXYOSYEG5HRE3BV4IIWKSCUM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3DJXYOSYEG5HRE3BV4IIWKSCUM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3DJXYOSYEG5HRE3BV4IIWKSCUM/action/storage_attestation","attest_author":"https://pith.science/pith/3DJXYOSYEG5HRE3BV4IIWKSCUM/action/author_attestation","sign_citation":"https://pith.science/pith/3DJXYOSYEG5HRE3BV4IIWKSCUM/action/citation_signature","submit_replication":"https://pith.science/pith/3DJXYOSYEG5HRE3BV4IIWKSCUM/action/replication_record"}},"created_at":"2026-07-05T05:32:40.571032+00:00","updated_at":"2026-07-05T05:32:40.571032+00:00"}