Why are we still using 3D masses for cluster cosmology?

Author(s):
Debackere, S.N.B. (0000-0001-5412-2781); Hoekstra, H. (0000-0001-7463-2893); Schaye, J. (0000-0002-0668-5560); Heitmann, K.; Habib, S.
Published
2022
Publication type
Article / Letter to editor
Gravitational lensing: weakGalaxies: clusters: generalCosmological 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. 3, p. 3383-3405
hdl
1887/3514215
doi
10.1093/mnras/stac1687
URL
https://ui.adsabs.harvard.edu/abs/2022MNRAS.515.3383D