diff --git a/sphere/IFS.py b/sphere/IFS.py index 9d26302..a4cace2 100644 --- a/sphere/IFS.py +++ b/sphere/IFS.py @@ -2905,13 +2905,12 @@ def sph_ifs_combine_data(self, cpix=True, psf_dim=80, science_dim=290, correct_a - *_cube: the (x,y,time,lambda) cube - - *_parang: the parallactic angle vector - - *_derot: the derotation angles vector. This vector takes - into account the parallactic angle and any - instrumental pupil offset. This is the values - that need to be used for aligning the images with - North up and East left. + into account the parallactic angle, the default + -1.75° true North offset, and any instrumental + pupil offset. This is the values that need to be + used for aligning the images with North up and + East left. - *_frames: a csv file with all the information for every frames. There is one line by time step in the diff --git a/sphere/IRDIS/ImagingReduction.py b/sphere/IRDIS/ImagingReduction.py index cd62d91..9ad6918 100644 --- a/sphere/IRDIS/ImagingReduction.py +++ b/sphere/IRDIS/ImagingReduction.py @@ -1515,13 +1515,12 @@ def sph_ird_combine_data(self, cpix=True, psf_dim=80, science_dim=290, correct_a - *_cube: the (x,y,time,lambda) cube - - *_parang: the parallactic angle vector - - *_derot: the derotation angles vector. This vector takes - into account the parallactic angle and any - instrumental pupil offset. This is the values - that need to be used for aligning the images with - North up and East left. + into account the parallactic angle, the default + -1.75° true North offset, and any instrumental + pupil offset. This is the values that need to be + used for aligning the images with North up and + East left. - *_frames: a csv file with all the information for every frames. There is one line by time step in the