Currently, we are assuming in our halo biasing module that we have fit a bias model for every exact cosmology that we want to generate simulations for.
However, we would like to be able to run our pipeline at any cosmology, including ones for which we don't have a Quijote calibration simulation.
We can do this by:
Nearest neighbor matching new cosmologies to Quijote cosmologies
Linear or kNN interpolation of the bias parameters (if they're smooth enough)
Deriving a global fit to bias parameters across all cosmologies (could break at extreme cosmologies
Currently, we are assuming in our halo biasing module that we have fit a bias model for every exact cosmology that we want to generate simulations for.
However, we would like to be able to run our pipeline at any cosmology, including ones for which we don't have a Quijote calibration simulation.
We can do this by: