antaress.ANTARESS_corrections.ANTARESS_fringing module#
- corr_fring(inst, gen_dic, data_inst, plot_dic, data_dic)[source]#
Main fringing correction routine.
Determines and applies correction for near-infrared spectrograph fringes.
- Parameters:
TBD
- Returns:
TBD
- FIT_fring_mod(param, x, args=None)[source]#
Fringing fit function
Calls corresponding model function for optimization
- Parameters:
TBD
- Returns:
TBD
- fring_mod(param, x, args=None)[source]#
Fringing model function
Defined as the product of
nominal flux : should be close to 1 as we model the ratio between two overlapping orders
4th order polynomial function, function of wavelength: model low-frequency variations, such as the blaze if not removed
amplifying sinusoidal perturbation, function of wavenumber : periodic in wavenumber, amplitude is a gaussian increasing with wavenumber
- Parameters:
TBD
- Returns:
TBD