Juan Pablo Cordero
Juan Pablo Cordero
## Description #565 Does not include unit tests for EisensteinHuHalofit and has incomplete documentation for some of the class methods Unit tests can either compare to existing precomputed values obtained...
## Description Implements an achromatic model for dust obscured ellipticity distributions, from Padilla & Strauss 2008. This would close #341 The model follows a similar structure to `ryden04_ellipticity`. The `dust_extincted_ellipticity`...
## Description Absorption produced by dust affects flux measurements as galaxies seen edge-on can potentially have significant extinction and fall outside of selection cuts. This induces a selection bias that...
## Description Examples across different modules use different arbitrary input arrays and values. For instance, the Eisenstein & Hu module uses a log-spaced input for the wavenumbers `wavenumber = np.logspace(-3,...
## Description Specially relevant for galaxies in halos / clusters, this module should return peculiar line of sight velocities for galaxies. ## Inputs - Parent halo / cluster? ## Outputs...
Based on issue #117, we should add instructions on how to be consistent with units, tests, inputs etc. in the documentation and the code. Some of the modules are intrinsically...