Software for calibration and analysis of infrared images of solar system objects. Has been applied successfully to NIRC2, OSIRIS, and Lick ShARCS data.
I noticed that multi_reduce.py is using the same flat for every observation, i.e. the kp flat for h and hp filters.
I think the problem comes from on line 272 in multi_reduce.py:
wl_eff = float(tab[wl_kw].data[0])
When i print(tab[wl_kw].data), I get a table column with the effective wavelengths of all the data in my observation, and it always just uses the first value which is 2.1245 in my case.
I noticed that multi_reduce.py is using the same flat for every observation, i.e. the kp flat for h and hp filters.
I think the problem comes from on line 272 in multi_reduce.py:
wl_eff = float(tab[wl_kw].data[0])When i print(tab[wl_kw].data), I get a table column with the effective wavelengths of all the data in my observation, and it always just uses the first value which is 2.1245 in my case.