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At this moment, we implement the following tasks in this second half part:
- measure the flux calibration vector of each flux standard,
- simply calculate an average of the flux calibration vectors across the field of view, instead of smart modeling,
- apply the averaged flux calibration vector to science targets,
- finally, output the flux-calibrated spectra of the science targets (pfsSingle) and the flux calibration parameters (fluxCal).
After commissioning observations, we will work on modeling flux calibration vectors across the FoV and studying it.
`fluxCal` will be a subclass of FocalPlaneFunction according to the current fluxCalibrateTask.
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