A new non-parametric method to infer galaxy cluster masses from weak lensing
We introduce a new, non-parametric method to infer deprojected 3D mass profiles $M(r)$ of galaxy clusters from weak gravitational lensing observations. The method assumes spherical symmetry and a moderately small convergence, $\kappa \lesssim 1$. The assumption of spherical symmetry is an important...
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| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Maynooth Academic Publishing
2024-12-01
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| Series: | The Open Journal of Astrophysics |
| Online Access: | https://doi.org/10.33232/001c.127612 |
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