TY  - RPRT
TI  - Why are we still using 3D masses for cluster cosmology?
AU  - Debackere, Stijn N. B. (ORCID:0000000154122781)
AU  - Hoekstra, Henk (ORCID:0000000206413231)
AU  - Schaye, Joop (ORCID:0000000206685560)
AU  - Heitmann, Katrin
AU  - Habib, Salman
PY  - 2022
DO  - 10.1093/mnras/stac1687
UR  - https://www.osti.gov/biblio/1880138
ID  - 1880138
ER  -