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Last modified by flenners on 2026-02-04 17:25
From version 16.3
edited by flenners
on 2026-02-04 17:16
Change comment: There is no comment for this version
To version 17.1
edited by flenners
on 2026-02-04 17:17
Change comment: There is no comment for this version

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76 76  
77 77  You do not need to load any additional dark images.
78 78  
79 -Skip "Normalize, Minus Log, Rotate" in the Preperation Tab. The optional steps, eg.  are still optional. (see below)
79 +Skip "Normalize, Minus Log, Rotate" in the Preperation Tab. The optional steps, eg. padding are still optional. (see below)
80 80  
81 81  In principle, you can directly proceed to the third tab "Reconstruction". 
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102 102  
103 103  **Binning:** You can bin your data before reconstruction. Since the detector has a point spread function of 2-3 pixels, it is save to bin by a factor of 2 without loosing spatial resolution. This reduces computation time and storage space needed.
104 104  
105 -**Padding:** RECOMENDED FOR ROI scans! If your samples are significantly __larger__ than the field of view, you can pad your data to prevent artifacts at the outer field of view. Example: 100
105 +**Padding:** **//RECOMENDED FOR ROI scans//**! If your samples are significantly __larger__ than the field of view, you can pad your data to prevent artifacts at the outer field of view. Example: 100
106 106  
107 107  **Filter Projections before reconstruction:** You can filter the data before reconstruction. This reduces the noise, but also can induce blurring in the data. Only recommended for very noisy data. Filtering after reconstruction is usually better.
108 108