{"paper":{"title":"KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Amara, A. Cimatti, A. Cuceu, A. Da Silva, A. Dvornik, A. Grazian, A. H. Wright, A. Kiessling, A. Loureiro, A. N. Taylor, A. Secroun, A. Spurio Mancini, B. Garilli, B. Giblin, B. Gillis, B. Joachimi, B. Morin, B. St\\\"olzner, C. A. J. Duncan, C. Bodendorf, C. Carbone, C. Giocoli, C. Heymans, C. Padilla, C. Sirignano, D. Bonino, E. A. Valentijn, E. Branchini, E. Franceschi, E. Munari, F. Dubath, F. Grupp, F. Hormuth, F. Marulli, F. Pasian, F. Raison, F. Torradeflot, G. Congedo, G. Meylan, G. Polenta, G. Sirri, G. Zamorani, H. Hildebrandt, H. Kurki-Suonio, H. Rix, H. Shan, I. Lloro, I. Tereno, J. Carretero, J. L. Starck, J. Rhodes, J. Weller, J. Zoubian, K. Jahnke, K. Kuijken, K. Markovic, K. Pedersen, L. Conversi, L. Corcione, L. Moscardini, L. Popa, L. Stanco, L. Whittaker, M. Asgari, M. Baldi, M. Bilicki, M. Brescia, M. Castellano, M. Cropper, M. Douspis, M. Frailis, M. Fumana, M. Kilbinger, M. K\\\"ummel, M. Kunz, M. Meneghetti, M. Moresco, M. Poncet, M. Roncarelli, N. Auricchio, N. Tessore, N. Welikala, O. Mansutti, O. Marggraf, P. B. Lilje, P. Fosalba, P. Schneider, P. Tallada-Cresp\\'i, R. Cledassou, R. Farinelli, R. Massey, R. Saglia, R. Toledo-Moreo, S. Andreon, S. Camera, S. Cavuoti, S. Dusini, S. Farrens, S. Ferriol, S. Kermiche, S. Ligori, S. M. Niemi, S. Paltani, S. Pires, S. Serrano, S. V. H. Haugan, T. Kitching, T. Tr\\\"oster, V. Capobianco, V. Pettorino, W. Holmes, X. Dupac, Y. Copin, Y. Wang","submitted_at":"2021-10-13T18:00:03Z","abstract_excerpt":"We present a tomographic weak lensing analysis of the Kilo Degree Survey Data Release 4 (KiDS-1000), using a new pseudo angular power spectrum estimator (pseudo-$C_{\\ell}$) under development for the ESA Euclid mission. Over 21 million galaxies with shape information are divided into five tomographic redshift bins, ranging from 0.1 to 1.2 in photometric redshift. We measured pseudo-$C_{\\ell}$ using eight bands in the multipole range $76<\\ell<1500$ for auto- and cross-power spectra between the tomographic bins. A series of tests were carried out to check for systematic contamination from a varie"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2110.06947","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/2110.06947/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"}