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For example, if background subtraction is applied to a line plot, the user could process the original data (re-binning or smoothing, for example) and then designate the resulting data to be used anywh…
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- Try the snip method that is in scikit-xray
- Try the thing that @CJ-Wright suggests lower down in this issue
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Hi @tischi,
how about creating an additional module for uneven illumination?
This is very similar to local background correction but you divide the images.
For instance for transmission this is qui…
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Sight-lines to watch:
- Direction of Orion nebula - known to be problematic with DR2 (i.e. fraction of known YSOs - e.g. classified as so by Spitzer). Appears to be a background subtraction issue i…
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Makefile:52: background_subtraction.d: No such file or directory
Makefile:52: floor_detector.d: No such file or directory
Makefile:52: foreground_extractor.d: No such file or directory
Makefile:52: lo…
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From Vassilis:
A researcher noticed that our L2 ESA data are not providing accurate moments. The reason is that the background subtraction needs to be changed to accommodate the increased radiation…
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Morphological reconstruction is super powerful, e.g., can be used for local maxima detection:
https://github.com/ijpb/MorphoLibJ/issues/47
- start from function f (-> the dark curve)
- consid…
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From Dec'22 quarterly update
- Investigate the viability of a second-order solution proposed by DM called "background matching" for possible use in full survey.
- this was a stretch goal for Phase …
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Hi! I'm trying to use the macro to quantify Huntington's aggregates. I have all my images stacked in a 3-channel TIFF. I can set the threshold for the aggregate channel, but in the next step I get an …