DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
Creators: name: Survey, Dark Energy
name: Collaboration, Kilo-Degree Survey
name: :
name: Abbott, T. M. C.
name: Aguena, M.
name: Alarcon, A.
name: Alves, O.
name: Amon, A.
name: Andrade-Oliveira, F.
name: Asgari, M.
name: Avila, S.
name: Bacon, D.
name: Bechtol, K.
name: Becker, M. R.
name: Bernstein, G. M.
name: Bertin, E.
name: Bilicki, M.
name: Blazek, J.
name: Bocquet, S.
name: Brooks, D.
name: Burger, P.
name: Burke, D. L.
name: Camacho, H.
name: Campos, A.
name: Rosell, A. Carnero
name: Kind, M. Carrasco
name: Carretero, J.
name: Castander, F. J.
name: Cawthon, R.
name: Chang, C.
name: Chen, R.
name: Choi, A.
name: Conselice, C.
name: Cordero, J.
name: Crocce, M.
name: da Costa, L. N.
name: Pereira, M. E. da Silva
name: Dalal, R.
name: Davis, C.
name: de Jong, J. T. A.
name: DeRose, J.
name: Desai, S.
name: Diehl, H. T.
name: Dodelson, S.
name: Doel, P.
name: Doux, C.
name: Drlica-Wagner, A.
name: Dvornik, A.
name: Eckert, K.
name: Eifler, T. F.
name: Elvin-Poole, J.
name: Everett, S.
name: Fang, X.
name: Ferrero, I.
name: Ferté, A.
name: Flaugher, B.
name: Friedrich, O.
name: Frieman, J.
name: García-Bellido, J.
name: Gatti, M.
name: Giannini, G.
name: Giblin, B.
name: Gruen, D.
name: Gruendl, R. A.
name: Gutierrez, G.
name: Harrison, I.
name: Hartley, W. G.
name: Herner, K.
name: Heymans, C.
name: Hildebrandt, H.
name: Hinton, S. R.
name: Hoekstra, H.
name: Hollowood, D. L.
name: Honscheid, K.
name: Huang, H.
name: Huff, E. M.
name: Huterer, D.
name: James, D. J.
name: Jarvis, M.
name: Jeffrey, N.
name: Jeltema, T.
name: Joachimi, B.
name: Joudaki, S.
name: Kannawadi, A.
name: Krause, E.
name: Kuehn, K.
name: Kuijken, K.
name: Kuropatkin, N.
name: Lahav, O.
name: Leget, P. -F.
name: Lemos, P.
name: Li, S. -S.
name: Li, X.
name: Liddle, A. R.
name: Lima, M.
name: Lin, C. -A
name: Lin, H.
name: MacCrann, N.
name: Mahony, C.
name: Marshall, J. L.
name: McCullough, J.
name: Mena-Fernández, J.
name: Menanteau, F.
name: Miquel, R.
name: Mohr, J. J.
name: Muir, J.
name: Myles, J.
name: Napolitano, N.
name: Navarro-Alsina, A.
name: Ogando, R. L. C.
name: Palmese, A.
name: Pandey, S.
name: Park, Y.
name: Paterno, M.
name: Peacock, J. A.
name: Petravick, D.
name: Pieres, A.
name: Malagón, A. A. Plazas
name: Porredon, A.
name: Prat, J.
name: Radovich, M.
name: Raveri, M.
name: Reischke, R.
name: Robertson, N. C.
name: Rollins, R. P.
name: Romer, A. K.
name: Roodman, A.
name: Rykoff, E. S.
name: Samuroff, S.
name: Sánchez, C.
name: Sanchez, E.
name: Sanchez, J.
name: Schneider, P.
name: Secco, L. F.
name: Sevilla-Noarbe, I.
name: Shan, H. -Y.
name: Sheldon, E.
name: Shin, T.
name: Sifón, C.
name: Smith, M.
name: Soares-Santos, M.
name: Stölzner, B.
name: Suchyta, E.
name: Swanson, M. E. C.
name: Tarle, G.
name: Thomas, D.
name: To, C.
name: Troxel, M. A.
name: Tröster, T.
name: Tutusaus, I.
name: Busch, J. L. van den
name: Varga, T. N.
name: Walker, A. R.
name: Weaverdyck, N.
name: Wechsler, R. H.
name: Weller, J.
name: Wiseman, P.
name: Wright, A. H.
name: Yanny, B.
name: Yin, B.
name: Yoon, M.
name: Zhang, Y.
name: Zuntz, J.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: We present a joint cosmic shear analysis of the Dark Energy Survey (DES Y3) and the Kilo-Degree Survey (KiDS-1000) in a collaborative effort between the two survey teams. We find consistent cosmological parameter constraints between DES Y3 and KiDS-1000 which, when combined in a joint-survey analysis, constrain the parameter $S_8 = σ_8 \sqrt{Ω_{\rm m}/0.3}$ with a mean value of $0.790^{+0.018}_{-0.014}$. The mean marginal is lower than the maximum a posteriori estimate, $S_8=0.801$, owing to skewness in the marginal distribution and projection effects in the multi-dimensional parameter space. Our results are consistent with $S_8$ constraints from observations of the cosmic microwave background by Planck, with agreement at the $1.7σ$ level. We use a Hybrid analysis pipeline, defined from a mock survey study quantifying the impact of the different analysis choices originally adopted by each survey team. We review intrinsic alignment models, baryon feedback mitigation strategies, priors, samplers and models of the non-linear matter power spectrum.
description: 40 pages, 21 figures, 15 tables, accepted Open Journal of Astrophysics. Download the chains from https://des.ncsa.illinois.edu/releases/y3a2/Y3key-joint-des-kids or create your own chains with CosmoSIS using https://github.com/joezuntz/cosmosis-standard-library/blob/main/examples/des-y3_and_kids-1000.ini Watch the core team discuss this analysis at https://cosmologytalks.com/2023/05/26/des-kids