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Codecov Report✅ All modified and coverable lines are covered by tests. Additional details and impacted files@@ Coverage Diff @@
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vitenti
approved these changes
Feb 10, 2026
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Description
This is an implementation of the mass-dependent NLA model for intrinsic alignments as a weak lensing systematic. It adds a simple NLA systematic to each weak lensing tracer where the intrinsic alignment bias amplitude for the NLA model is given by:
where$A_\mathrm{IA,0},\beta$ are the amplitude and mass scaling of the model (as shared parameters, with the same values used for all tracers at each likelihood evaluation) while $f_r^{(i)}$ , $\langle M_\mathrm{h} \rangle^{(i)}$ are the fraction of red galaxies and average halo mass of tracer $(i)$ . The default pivot halo mass $M_\mathrm{h,piv}=10^{13.5}$ $\mathrm{M_{sun}}/h$ .
Type of change
Checklist:
The following checklist will make sure that you are following the code style and
guidelines of the project as described in the
contributing page.
bash pre-commit-checkand fixed any issues