{"paper":{"title":"Results from the first spectropolarimetric survey of $\\gamma$ Dor pulsators","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"2), (2) LIRA, (3) Department of Physics, 4), (4) School of Mathematics, (5) Nasa Ames Research Center, Astronomy, Bartol Research Institute, B. Mas Sanz (1), C. Neiner (2), CNRS, CY Cergy Paris Universit\\'e, Denmark, France, J. Labadie-Bartz (1, K. Thomson-Paressant (2, Newcastle University, Observatoire de Paris, O. D\\\"urfeldt Pedros (1), Physics, P. Stanley (3), R. Ouazzani (2), S. D. Chojnowski (5), Sorbonne Universit\\'e, Statistics, Technical University of Denmark, T. Natan (3), UK, Universit\\'e Paris Cit\\'e, Universit\\'e PSL, University of Delaware, USA, USA), V. Antoci (1), V. Petit (3) ((1) DTU Space","submitted_at":"2026-08-12T09:43:21Z","abstract_excerpt":"Context. Magnetic fields can have an important influence on stellar structure and evolution. In intermediate-mass (A- and F-type) stars, there are many known stars with directly measured strong, globally organized magnetic fields, as well as indications of weak and/or small-scale variable fields. However, among the intermediate-mass $\\gamma$ Dor pulsators, there are no known stars with strong surface magnetic fields.\n  Aims. The broad goal of this work is to search for evidence of strong, globally organized fields at the surface of $\\gamma$ Dor pulsators.\n  Methods. We identified objects consi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2608.11854","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/2608.11854/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"}