Source code for lenstronomy.LightModel.light_model

__author__ = "sibirrer"


from lenstronomy.LightModel.linear_basis import LinearBasis

__all__ = ["LightModel"]


[docs] class LightModel(LinearBasis): """Class to handle extended surface brightness profiles (for e.g. source and lens light) all profiles come with a surface_brightness parameterization (in units per square angle and independent of the pixel scale). The parameter 'amp' is the linear scaling parameter of surface brightness. Some functional forms come with a total_flux() definition that provide the integral of the surface brightness for a given set of parameters. The SimulationAPI module allows to use astronomical magnitudes to be used and translated into the surface brightness conventions of this module given a magnitude zero point. """
[docs] def __init__( self, light_model_list, deflection_scaling_list=None, source_redshift_list=None, smoothing=0.001, sersic_major_axis=None, ): """ :param light_model_list: list of light models :param deflection_scaling_list: list of floats indicating a relative scaling of the deflection angle from the reduced angles in the lens model definition (optional, only possible in single lens plane with multiple source planes) :param source_redshift_list: list of redshifts for the different light models (optional and only used in multi-plane lensing in conjunction with a cosmology model) :param smoothing: smoothing factor for certain models (deprecated) :param sersic_major_axis: boolean or None, if True, uses the semi-major axis as the definition of the Sersic half-light radius, if False, uses the product average of semi-major and semi-minor axis. If None, uses the convention in the lenstronomy yaml setting (which by default is =False) """ super(LightModel, self).__init__( light_model_list=light_model_list, smoothing=smoothing, sersic_major_axis=sersic_major_axis, ) self.deflection_scaling_list = deflection_scaling_list self.redshift_list = source_redshift_list