CLMM
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LSSTDESC
A Python library for performing galaxy cluster mass reconstruction from weak lensing observables
Pylint was failing on astropy v6.0, with errors of type: ``` clmm/support/mock_data.py:418:33: E1101: Module 'astropy.units' has no 'deg' member; maybe 'dex'? (no-member) ``` This is a known error, and a...
#615 needs to be merged first in order not to make changes to the CI script.
Fix how max supported CCL version is checked to prepare for the new release.
The current method for checking max supported CCL version in the theory module will fail after CCL > 3.0.0 is released.
Notebooks in `examples/NumCosmo/` are outdated and need to be either fixed or removed. Also fix `examples/Paper_v1.0/mcmc.ipynb`.
https://github.com/LSSTDESC/CLMM/blob/d9de5a38ea3d0708695ae900f1e0d539051a257f/clmm/utils/statistic.py#L214 `cumulative_trapezoid` requires Scipy >= 1.6.0. `simps` was also renamed to `simpson` in that version.
I found a possible inconsistency in how azimuthal angles (phi) are computed in clmm.dataops (e.g. by _compute_lensing_angles_astropy). I would compute phi as (sk0 and sk1 being the coordinates of lens...
As we discussed writing a v2.0 note we need to list the developments that took part since the first CLMM paper. See discussion here : https://github.com/LSSTDESC/CLMM/issues/474 for desired additions.
Add code to calculate the covariance contribution from uncorrelated large scale structures in the field of galaxy clusters. The expression is given in equation 17 of Mclintock: https://arxiv.org/pdf/1805.00039.pdf although it...
