Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses

Author(s):
Debackere, S.N.B. (0000-0001-5412-2781); Hoekstra, H. (0000-0001-7463-2893); Schaye, J. (0000-0002-0668-5560)
Published
2022
Publication type
Article / Letter to editor
Gravitational lensing: weakGalaxies: ClustersgeneralCosmological parametersCosmology: ObservationsCosmology: theoryLarge-scale structure of UniverseAstrophysics - Cosmology and Nongalactic Astrophysics
Date issued
2022
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2022), Vol. 515, no. 4, p. 6023-6031
hdl
1887/3514213
doi
10.1093/mnras/stac2077
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.515.6023D