Miguel de Val-Borro

flux calibration unstable at the edges

3

I have tried to run flux calibration in pydis using the standard star G191b2b. These data cover the optical and near-UV region starting around 3000 Å. The sensitivity function using...

Sometimes it is helpful to apply the sensitivity function from a standard target to a 2D spectrum with one axis being wavelength and the spatial direction to study extended sources.

This change is needed to be compatible with python 3.x