{"paper":{"title":"Constraints on the redshift evolution of astrophysical feedback with Sunyaev-Zeldovich effect cross-correlations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas, A. Carnero Rosell, A. E. Evrard, A. Lidz, A. Roodman, B. Flaugher, B. Jain, D. Brooks, D. J. James, D. L. Hollowood, D. W. Gerdes, E. Bertin, E. Buckley-Geer, E. J. Baxter, E. Krause, E. Sanchez, E. Suchyta, F. J. Castander, F. Menanteau, F. Sobreira, G. Tarle, H. T. Diehl, I. Sevilla-Noarbe, J. Aguirre, J. Carretero, J. C. Hill, J. DeRose, J. De Vicente, J. Frieman, J. Garc\\'ia-Bellido, J. Gschwend, J. L. Marshall, J. Orlowski-Scherer, J. P. Dietrich, K. Kuehn, L. N. da Costa, M. A. G. Maia, M. Carrasco Kind, M. Devlin, M. E. C. Swanson, M. Smith, M. Soares-Santos, N. Kuropatkin, N. Zhu, P. Doel, P. Fosalba, P. Melchior, R. A. Gruendl, R. Cawthon, R. H. Wechsler (DES Collaboration), R. K. Sheth, R. Miquel, S. Avila, S. Desai, S. Pandey, S. Serrano, T. Giannantonio, W. G. Hartley, Z. Xu","submitted_at":"2019-04-30T16:21:05Z","abstract_excerpt":"An understanding of astrophysical feedback is important for constraining models of galaxy formation and for extracting cosmological information from current and future weak lensing surveys. The thermal Sunyaev-Zel'dovich effect, quantified via the Compton-$y$ parameter, is a powerful tool for studying feedback, because it directly probes the pressure of the hot, ionized gas residing in dark matter halos. Cross-correlations between galaxies and maps of Compton-$y$ obtained from cosmic microwave background surveys are sensitive to the redshift evolution of the gas pressure, and its dependence on"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.13347","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/1904.13347/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"}