Currently, the DRP creates data cubes of the delta wavelength map for arc and standard star observations.
For users that need to know the native resolution per pixel as a function of wavelength, it would be good to propagate the delta cube along with the intensity cube. Should be easy to implement, since it is already done for standard stars.
Currently, the DRP creates data cubes of the delta wavelength map for arc and standard star observations.
For users that need to know the native resolution per pixel as a function of wavelength, it would be good to propagate the delta cube along with the intensity cube. Should be easy to implement, since it is already done for standard stars.