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Add spin_mass_dependence option to dark_matter_halo group
The option defaults to false, and indicates whether the lognormal distribution used to draw lambda values should use a fix value of 0.03, or a dynamic value based on the halo spin distribution following Kim et al. (2015), as its m parameter (the natural logarithm of the distribution's mean). The Lagos et al. (2023) paper used this dependency, and therefore we're also updating the sample configuration file that reflects that paper to ensure reproducibility. Signed-off-by: Rodrigo Tobar <[email protected]>
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