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On the road to percent accuracy III: non-linear reaction of the matter power spectrum to massive neutrinos

, , , , and . (2019)cite arxiv:1909.02561Comment: 7 pages, 3 figures, submitted to MNRAS.

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Cosmology from large-scale structure: Constraining $Łambda$CDM with BOSS, , , , , , , , , and 2 other author(s). (2019)cite arxiv:1909.11006Comment: 8 pages, 7 figures. Submitted to A&A.Joint constraints on cosmology and the impact of baryon feedback: combining KiDS-1000 lensing with the thermal Sunyaev-Zeldovich effect from Planck and ACT, , , , , , , , , and 6 other author(s). (2021)cite arxiv:2109.04458Comment: 20 pages, 15 figures. Comments welcome. Code, data vectors, and covariances are available at https://github.com/tilmantroester/KiDS-1000xtSZ.Rubin-Euclid Derived Data Products: Initial Recommendations, , , , , , , , , and 110 other author(s). (2022)cite arxiv:2201.03862Comment: Report of the Rubin-Euclid Derived Data Products Working Group, 78 pages, 11 figures.An adapted filter function for density split statistics in weak lensing, , , , , , and . (2020)cite arxiv:2006.10778.The Dark Universe. Physics World Discovery IOP Publishing, (2016)KiDS-1000 catalogue: weak gravitational lensing shear measurements, , , , , , , , , and 12 other author(s). (2020)cite arxiv:2007.01845Comment: 24 pages, 11 figures, submitted to A&A. This paper is part of the KiDS-1000 series of papers, accompanying Joachimi et al. appearing on the arxiv today.On the road to percent accuracy III: non-linear reaction of the matter power spectrum to massive neutrinos, , , , and . (2019)cite arxiv:1909.02561Comment: 7 pages, 3 figures, submitted to MNRAS.KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies, , , , , , , , , and 6 other author(s). (2020)cite arxiv:2006.10777Comment: 10 pages, 10 figures, submitted to A&A, comments welcome.CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment, , , , , , , , , and 9 other author(s). Monthly Notices of the Royal Astronomical Society, 454 (2): 1432--1452 (Oct 20, 2015)The abundance of ultra-diffuse galaxies from groups to clusters: UDGs are relatively more common in more massive haloes, , , , , , , , , and 10 other author(s). (2017)cite arxiv:1706.02704Comment: 11 pages, 8 figures. Submitted for publication in A&A.