Parameter file¶
This identifier is the most important one, and determine what the program will do.
It defines some parameters such has the number of potential mode, the total
number of potential mode that are going to be test, the grid mode, and the
number of rows and columns in the grid.
It allows to enter the information on the potential.
Under this identifier are defined the priors on the potential parameters. It is advised to put the limit identifier just after the potentiel identifier. As the potential identifier, it is allowed to put comments after the identifier limit on the same line.
Under this identifier are defined the default parameters for all the galaxy scale mass
components that account for perturbations to the cluster potential by the
galaxies. By default, the mass distribution model for the galaxies is PIEMD.
Under this identifier are defined the parameters to constrain the mass profile using dynamical data.
Under this identifier are defined the the parameters that define a source shape.
Under this identifier are defined the priors on the parameters that define a source shape.
Under this identifier are defined the parameters to compute the critical and the caustic lines.
Under this identifier is defined the way to represent the computed deformation of objects.
Under this identifier is defined the different noise that can be added to a gravitational image, such as seeing or Poisson Noise. All these constants are used when the image mode grande iso or runmode pixel representation is set.
Under this identifier are defined the cosmological parameters 0mega, λ and H0.
Under this identifier are defined the limits on the cosmological parameters that you want to optimise during the Bayesian optimisation.
Under this identifier is defined the size of the field used in some calculations such as the dimension of the grid for the inversion of the lens equation.
Under this identifier are defined some parameters to retrieve the shape of the source knowing a pixel-frame of the image.
Under this identifier are defined some characteristics of images, multiple
images or arclets.
Under this identifier are defined some characteristics of the source.
To put at the end of the .par file.