CONAN.models.Planet_LC_Model.get_value
======================================

.. py:method:: CONAN.models.Planet_LC_Model.get_value(tarr, ss=None, grprs=0, vcont=0, Rstar=None, model_phasevar=False, custom_LCfunc=None, pc_model='cosine', approx_EA=False)

   computes the transit/occultation/phase curve model for a given set of parameters along with the baseline

   :param tarr: The timestamps of the lightcurve
   :type tarr: array-like
   :param ss: The configuration for the supersampling
   :type ss: SimpleNamespace
   :param grprs: when using fitting depth variation, the base RpRs value to which deviation of each filter is added
   :type grprs: float;
   :param vcont: contamination factor
   :type vcont: float;
   :param Rstar: Stellar radius in Rsun. used to calculate light travel time correction. Default: None to not perform light travel time correction
   :type Rstar: float
   :param model_phasevar: fit the phase variation in the model. Default: False, in which case even if occultation depth is given the transit and occ are joined by a straight line
   :type model_phasevar: bool;
   :param custom_LCfunc: object containing the custom light curve function to be combined to or to replace the lightcurve model. Default: None
   :type custom_LCfunc: SimpleNamespace
   :param pc_: the phase curve model to be used. Default: "cosine". Options: "cosine" or "lambert"
   :type pc_: str;
   :param model: the phase curve model to be used. Default: "cosine". Options: "cosine" or "lambert"
   :type model: str;
   :param approx_EA: use approximate calculation of the eccentric anomaly. Default: False
   :type approx_EA: bool;

   :returns: * **marr** (*array-like*) -- The lightcurve model for the given parameters
             * **model_components** (*dict*) -- The components of the model for each planet in a system