Preprocess images: Difference between revisions
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* '''Uncorrected for CTF''' (this is done internally) | * '''Uncorrected for CTF''' (this is done internally) | ||
** If your data have previously been phase-flipped, that's OK: just tell RELION about it | ** If your data have previously been phase-flipped, that's OK: just tell RELION about it | ||
** Actually, if you are not planning to correct for CTFs inside RELION (e.g. for negative stain data), phase-flipping is recommended. | |||
** If your data have previously been pre-Wiener filtered, that's a ''very bad thing to do in general'': go back to the original data. | ** If your data have previously been pre-Wiener filtered, that's a ''very bad thing to do in general'': go back to the original data. | ||
* '''Normalised''' (the exact procedure does not matter too much, as errors in the normalisation are corrected internally) | * '''Normalised''' (the exact procedure does not matter too much, as errors in the normalisation are corrected internally) |
Revision as of 20:59, 27 September 2011
RELION will work best if your data are
- Clean from false particles (no images are discarded during refinement).
- Xmipp implements an image sorting utility called
xmipp_sort_by_statistics
that is very handy in the cleaning of a data set.
- Xmipp implements an image sorting utility called
- Unmasked (masking is performed internally)
- Non-interpolated (prevent any prior rotations/translations: use the originally scanned pixel values)
- If downscaling is necessary because of memory issues: use a window-operation in Fourier-space, not a convolution in real-space (e.g. with rectangle/B-spline).
- Xmipp implements the Fourier-space downscaling in the
xmipp_scale
program with the-fourier
option.
- Uncorrected for CTF (this is done internally)
- If your data have previously been phase-flipped, that's OK: just tell RELION about it
- Actually, if you are not planning to correct for CTFs inside RELION (e.g. for negative stain data), phase-flipping is recommended.
- If your data have previously been pre-Wiener filtered, that's a very bad thing to do in general: go back to the original data.
- Normalised (the exact procedure does not matter too much, as errors in the normalisation are corrected internally)
- In one or more MRC stacks (with extension
.mrcs
; but also SPIDER and IMAGIC files may be read)
And then, just like with any other refinement program, you might save yourself lots of trouble if your data have:
- high signal-to-noise ratios (take great care in sample preparation and data collection)