{"paper":{"title":"BeyondPlanck XVI. Limits on Large-Scale Polarized Anomalous Microwave Emission from Planck LFI and WMAP","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Karakci, A.-S. Suur-Uski, A. Zacchei, B. Hensley, B. Partridge, C. Franceschet, D. Herman, D. J. Watts, D. Maino, D. Tavagnacco, E. Gjerl{\\o}w, E. Keih\\\"anen, G. Maggio, H. K. Eriksen, H. Thommesen, H. T. Ihle, I. K. Wehus, J. B. Jewell, K. J. Andersen, L. P. L. Colombo, M. Bersanelli, M. Brilenkov, M. Carbone, M. Galloway, M. Iacobellis, M. Ieronymaki, M. K. Foss, M. Maris, M. Reinecke, R. Aurlien, R. Banerji, R. Keskitalo, S. Bertocco, S. Galeotta, S. Gerakakis, S. Paradiso, T. L. Svalheim, U. Fuskeland","submitted_at":"2022-01-10T18:41:29Z","abstract_excerpt":"We constrain the level of polarized anomalous microwave emission (AME) on large angular scales using $\\textit{Planck}$ LFI and $\\textit{WMAP}$ polarization data within a Bayesian CMB analysis framework. We model synchrotron emission with a power-law spectral energy distribution, and the sum of AME and thermal dust emission through linear regression with the $\\textit{Planck}$ HFI 353 GHz data. This template-based dust emission model allows us to constrain the level of polarized AME while making minimal assumptions on its frequency dependence. We neglect cosmic microwave background fluctuations,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2201.03530","kind":"arxiv","version":2},"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/2201.03530/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"}