{"paper":{"title":"First Constraints on the Epoch of Reionization Using the non-Gaussianity of the Kinematic Sunyaev-Zel{'}dovich Effect from the South Pole Telescope and {\\it Herschel}-SPIRE Observations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Stark, A. Coerver, A. Cukierman, A. Doussot, A. E. Gambrel, A. E. Lowitz, A. Foster, A. Hryciuk, A. J. Anderson, A. Maniyar, A. N. Bender, A. Rahlin, A. R. Khalife, A. Suzuki, A. T. Crites, A. T. Lee, B. A. Benson, B. Ansarinejad, B. R. Saliwanchik, B. Thorne, C. Corbett Moran, C. Daley, C. Feng, C. L. Chang, C.-L. Kuo, C. L. Reichardt, C. Lu, C. Pryke, C. Sievers, C. Tandoi, C. Trendafilova, C. Tucker, C. Umilta, D. Dutcher, D. Li, E. Camphuis, E. Hivon, E. M. George, E. Schiappucci, E. S. Martsen, F. Bianchini, F. Ge, F. Guidi, F. K\\'eruzor\\'e, F. Menanteau, F. R. Bouchet, G. I. Noble, G. P. Holder, G. Smecher, G. Wang, H. C. Chiang, J. A. Beall, J. A. Sobrin, J. A. Zebrowski, J. Bock, J. C. Hood, J. D. Hrubes, J. D. Vieira, J. E. Austermann, J. E. Carlstrom, J. E. Ruhl, J. Gallicchio, J. Hubmayr, J. J. McMahon, J. Montgomery, J. P. Nibarger, J. Stephen, K. A. Phadke, K. Benabed, K. D. Irwin, K. Fichman, K. Kornoelje, K. K. Schaffer, K. Levy, K. L. Thompson, K. Prabhu, K. R. Dibert, K. R. Ferguson, L. Balkenhol, L. Bryant, L. E. Bleem, L. Knox, M. A. Dobbs, M. Archipley, M. Korman, M. Millea, M. P. Viero, M. Rahimi, M. Rouble, M. R. Young, M. Zemcov, N. Goeckner-Wald, N. Gupta, N. Huang, N. W. Halverson, N. Whitehorn, P. A. R. Ade, P. Chaubal, P. M. Chichura, P. Paschos, R. Citron, R. Gualtieri, R. W. Gardner, S. Galli, S. Guns, S. Padin, S. Patil, S. Raghunathan, T. de Haan, T.-L. Chou, T. M. Crawford, T. Natoli, T. Veach, T. W. Cecil, V. Novosad, V. Yefremenko, W. Everett, W. L. Holzapfel, W. L. K. Wu, W. Quan, Y. Nakato, Y. Omori, Y. Wan, Z. Pan","submitted_at":"2024-03-04T18:59:07Z","abstract_excerpt":"We report results from an analysis aimed at detecting the trispectrum of the kinematic Sunyaev-Zel{'}dovich (kSZ) effect by combining data from the South Pole Telescope (SPT) and {\\it Herschel}-SPIRE experiments over a 100 ${\\rm deg}^{2}$ field. The SPT observations combine data from the previous and current surveys, namely SPTpol and SPT-3G, to achieve depths of 4.5, 3, and 16 $\\mu {\\rm K-arcmin}$ in bands centered at 95, 150, and 220 GHz. For SPIRE, we include data from the 600 and 857 GHz bands. We reconstruct the velocity-induced large-scale correlation of the small-scale kSZ signal with a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.02337","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/2403.02337/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"}