"How baryons can significantly bias cluster count cosmology" by Debackere et al. dataset

Dataset of the Maximum A-Posteriori Probabilities for the stage III and stage IV-like cluster count cosmology surveys. The datasets are saved as asdf files ending in _maps.asdf. These behave similarly to Python dictionaries. They can be generated with the code at https://github.com/StijnDebackere/lensing_haloes/

The dictionary keys contain the true cosmological parameters for each dataset ('omega_m', 'omega_b', 'h', 'n_s', 'w0', 'sigma_8'), the minimum and maximum redshifts ('z_min' and 'z_max') and masses ('log10_m_min' and 'log10_m_max') for the halo sample that was used to fit the cosmology, the survey area, 'A_survey'.

The MAPs are saved for the 'WL' (masses inferred from NFW profile with fixed concentration-mass relation fits to reduced shear), 'WL_c' (masses inferred from NFW profile with free concentration fits to reduced shear) and 'true' (unbiased halo masses) fitting methods. Each fitting method has the results for the mass cuts 14.0, 14.25 and 14.5 in m_200m.

For the stage III-like dataset, we also include all of the cluster samples. The halo sample dataset for the stage IV-like survey can be requested from Stijn Debackere (see arXiv:2101.07800 for contact information), since it exceeds the 50GB file limit.