{"paper":{"title":"Summary of the First Year of the Space Weather Around Young Suns Program: 900 Hours of Low-frequency Radio and Optical Data Dedicated to Young, Solar-type Stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Akshatha K. Vydula, Andrea Isella, Andres Rizo, Andrew Romero-Wolf, Bin Chen, Brian O'Donnell, Carolyn Heffner, Casey Law, Charlie Harnach, Corey Posner, Curt Corcoran, Dale Gary, Daniel C. Jacobs, David Hodge, David Woody, Ghislain Kemby, Gregg Hallinan, Greg Hellbourg, Greg Taylor, Ivey Davis, Jack Hickish, James Lamb, Jayce Dowell, Jeffry Zolkower, John Baker, John T. Klinefelter, Jordan Trim, Judd D. Bowman, Jun Shi, Katherine Elder, Kathryn Plant, Larry D'Addario, Marin M. Anderson, Mark Hodges, Matthew Kolopanis, Mike Virgin, Morgan Catha, Navtej Saini, Nikita Kosogorov, Nivedita Mahesh, Peijin Zhang, Rick Burruss, Rick Hobbs, Ruby Byrne, Sandy Weinreb, Scott White, Sherry Chhabra, Sijie Yu, Surajit Mondal, Thomas Zentmeyer, Travis Powell, Vinand Prayag, Xingyao Chen, Yuping Huang","submitted_at":"2026-06-09T22:24:58Z","abstract_excerpt":"The Space Weather Around Young Suns (SWAYS) program was introduced in \\citet{Davis2025} as a multi-wavelength monitoring program for studying the activity and particle environments of nearby, young, solar-type stars. The SWAYS program currently includes the Owens Valley Radio Observatory Long Wavelength Array (OVRO-LWA) operating between 13--87\\,MHz to search for stellar equivalents of solar type~II and III bursts, which are associated with bulk plasma motion in the corona and interplanetary medium. These observations are accompanied by simultaneous photometric data from the high-precision, op"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.11492","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/2606.11492/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"}