Persistent URL of this record https://hdl.handle.net/1887/3514215
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- MNRAS_515_2022_3383
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Why are we still using 3D masses for cluster cosmology?
- All authors
- Debackere, S.N.B.; Hoekstra, H.; Schaye, J.; Heitmann, K.; Habib, S.
- Date
- 2022
- Volume
- 515
- Issue
- 3
- Pages
- 3383 - 3405