The Code

jwstobsim

class jwstobsim.utils.AncillaryData(params)

Note

• Units for the orbital period and ephemeris can be anything as long as they are consistent (e.g. both in days).
• The orbital path is calculated based on t0 for primary transits and t_secondary for secondary eclipses.

jwstobsim.utils.bins_new(x, y, y_err, n_bins)

Calculate maximum error for transit light curve calculation.

Parameters:plot (bool) – If True, plots the error in the light curve model as a function of separation of centers. Returns:Truncation error (parts per million) Return type:float