Added LightCurve.set_exptime(), allowing the user to reset the exposure time;
Allowing the user to add the distance, velocity, and star diameter as the LightCurve is instantiated;
Added the object distance information in the print(LightCurve).
On EphemKernel and EphemJPL:
Added Ephem.to_file(), allowing the user to create an ASCII file that can be used as input on EphemPlanete.
On Occultation:
Added the name of the points (f, g) in Occultation.chi2_params as ['choord_name'];
Now, Occultation.chi2_params['radial_dispersion'] has all the values for each individual point, and not only the mean value and its standard deviation;
Occultation.chi2_params['mean_error'] was replaced by Occultation.chi2_params['radial_error'] and also has all the individual values, instead of only the mean value and its standard deviation.
On
LightCurve:LightCurve.set_dist();LightCurve.set_exptime(), allowing the user to reset the exposure time;LightCurveis instantiated;print(LightCurve).On
EphemKernelandEphemJPL:Ephem.to_file(), allowing the user to create an ASCII file that can be used as input onEphemPlanete.On
Occultation:Occultation.chi2_paramsas['choord_name'];Occultation.chi2_params['radial_dispersion']has all the values for each individual point, and not only the mean value and its standard deviation;Occultation.chi2_params['mean_error']was replaced byOccultation.chi2_params['radial_error']and also has all the individual values, instead of only the mean value and its standard deviation.