{"paper":{"title":"The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy Clusters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Alarcon, A. Amon, A. A. Plazas Malag\\'on, A. Campos, A. Carnero Rosell, A. Choi, A. Drlica-Wagner, A. Ferte, A. J. Ross, A. K. Romer, A. Liu, A. Merloni, A. Navarro-Alsina, A. Pieres, A. Roodman, B. Flaugher, B. Yanny, B. Yin, C. Chang, C. Davis, C. Doux, C. Garrel, C. Sanchez, D. Brooks, D. Friedel, D. Gruen, D. J. James, D. L. Burke, D. L. Hollowood, E. Artis, E. Bulbul, E. M. Huf, E. Sanchez, E. Sheldon, E. S. Rykoff, E. Suchyta, F. Balzer, F. Kleinebreil, F. Menanteau, F. Pacaud, G. Bernstein, G. Giannini, G. Gutierrez, G. Tarle, H. T. Diehl, H. Wu, I. Chiu, I. Ferrero, I. Harrison, I. Sevilla-Noarbe, I. Tutusaus, J. Carretero, J. Comparat, J. Cordero, J. DeRose, J. De Vicente, J. Elvin-Poole, J. Frieman, J. Garc\\'ia-Bellido, J. J. Mohr, J. L. Marshall, J. McCullough, J. Myles, J. Prat, J. Sanders, J. Weller, K. Bechtol, K. Eckert, K. Herner, K. Honscheid, K. Nandra, L. F. Secco, L. Kimmig, L. N. da Costa, M. Carrasco Kind, M. Costanzi, M. E. C. Swanson, M. E. S. Pereira, M. Gatt, M. Kluge, M. Ramos, M. Raveri, M. R. Becker, M. Schubnell, M. Smith, M. Troxel, N. Clerc, N. Jeffrey, N. Kuropatkin, N. MacCrann, N. Okabe, N. Weaverdyck, O. Alves, O. Lahav, P. Doel, P. F. Leget, P. Giles, P. Predehl, R. A. Gruendl, R. Cawthon, R. Chen, R. L. C. Ogando, R. P. Rollins, R. Seppi, S. Bhargava, S. Bocquet, S. Desai, S. Dodelson, S. Everett, S. Grandis, S. Lee, S. Pandey, S. R. Hinton, (The Dark Energy Survey Collaboration, the eROSITA-DE Consortium), T. H. Reiprich, T. N. Varga, T. Schrabback, T. Shin, V. Ghirardini, W. G. Hartley, X. Zhang, Y. E. Bahar, Y. Zhang","submitted_at":"2024-02-13T13:39:40Z","abstract_excerpt":"Number counts of galaxy clusters across redshift are a powerful cosmological probe, if a precise and accurate reconstruction of the underlying mass distribution is performed -- a challenge called mass calibration. With the advent of wide and deep photometric surveys, weak gravitational lensing by clusters has become the method of choice to perform this measurement. We measure and validate the weak gravitational lensing (WL) signature in the shape of galaxies observed in the first 3 years of the DES Y3 caused by galaxy clusters selected in the first all-sky survey performed by SRG/eROSITA. Thes"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.08455","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/2402.08455/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"}