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All of these sections are predefined strings that you can use in CosmoSIS modules. They are typically used as the names of "sections" - groups of parameters and data collected together.
For an entry on this list called "name", in code you would use these pre-defined constants for the strings:
Python: cosmosis.names.name
C: NAME_SECTION
C++: NAME_SECTION
Fortran: name_section
#Likelihoods likelihoods
Input parameters
cosmological_parameters
halo_model_parameters
intrinsic_alignment_parameters
baryon_parameters
shear_calibration_parameters
number_density_params
Source number density
wl_number_density
2-pt and related quantities
matter_power_nl
matter_power_lin
[[In development: matter_power_lin_cdm_baryon; only present when [camb]matter_power_lin_version indicates computation of no-neutrino spectra.]]
shear_xi
shear_cl
galaxy_cl
cmb_cl
lss_autocorrelation
gal_matter_power_lin
linear_cdm_transfer
sigma_r_lin
sigma_r_nl
Nuisance parameters
planck
intrinsic_alignment_field
shear_calibration
supernova_params
Galaxy bias
bias_field
Background quantities
distances
de_equation_of_state
Section for test likelihoods
test_parameters
Updated