eman2:e3make3d_point
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| eman2:e3make3d_point [2026/03/20 13:55] – steveludtke | eman2:e3make3d_point [2026/03/20 17:45] (current) – steveludtke | ||
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| - | ===== Preview of e3_make3d_point | + | ===== Preview of e3make3d_point |
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| + | **THE METHOD DESCRIBED ON THIS PAGE IS NOT YET PUBLISHED, IT IS PROVIDED TO GIVE PEOPLE THE OPPORTUNITY TO TRY IT OUT AS WE MAKE FINAL IMPROVEMENTS** | ||
| + | If you have any difficulties (or successes) with this method, please let us know, and feel free to ask questions (sludtke@bcm.edu). | ||
| The under-development e3make3d_point.py can be used to produce reconstructions which: | The under-development e3make3d_point.py can be used to produce reconstructions which: | ||
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| ==== If you are starting with an EMAN2/3 project ==== | ==== If you are starting with an EMAN2/3 project ==== | ||
| - | * Run a standard e2spa_refine.py on your phase-flipped particle data | + | * Run a standard |
| - | * Run exactly the same command with the "--pointrecon 500" | + | * Run exactly the same command with the //--pointrecon 500// option added to the command-line, |
| * 500 is the number of first-stage points to use in the reconstruction as described above. | * 500 is the number of first-stage points to use in the reconstruction as described above. | ||
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| * cd <folder where your STAR file is> | * cd <folder where your STAR file is> | ||
| * e3relion_convert.py <star file> | * e3relion_convert.py <star file> | ||
| + | * This involves making a copy of your data (with compression). It is creating a complete EMAN2 project folder, so for a large project will take a little time. | ||
| * cd eman3 | * cd eman3 | ||
| - | * e3make3d_point.py sets/fromstar__ctf_flip.lst --volout fromstar.hdf: | + | * e3make3d_point.py sets/fromstar%%__%%ctf_flip.lst --volout fromstar.hdf: |
| - | * volfiltlp is the resolution in Å the final map will be (Gaussian) filtered to. | + | * volfiltlp is the resolution in Å the final map will be (Gaussian) filtered to. If you decide the map is over/under filtered the final volume can easily be recreated from the other output file. |
| + | * The output volume is fromstar.hdf, | ||
| + | * If you wish to generate even/odd maps for a GSFSC calculation, | ||
| + | * Alternatively you could run an EMAN2 style iterative refinement with point-based reconstruction, | ||
| + | * e2spa_refine.py --ptcl sets/ | ||
| + | * You may need to look at a full EMAN2 tutorial to pick specific options for your case. The only change is the addition of the --pointrecon option. | ||
| + | ==== If you are starting with a CryoSparc refinement ==== | ||
| + | You will need to export your metadata (as a .cs file) and corresponding particle stack from CryoSparc and have these stored together somewhere on your local computer. | ||
| + | * conda activate eman2 | ||
| + | * cd <folder where your .cs file is> | ||
| + | * e3cryosparc_convert.py < | ||
| + | * This involves making a copy of your data (with compression). It is creating a complete EMAN2 project folder, so for a large project will take a little time. | ||
| + | * cd eman3 | ||
| + | * e3make3d_point.py sets/ | ||
| + | * volfiltlp is the resolution in Å the final map will be (Gaussian) filtered to. If you decide the map is over/under filtered the final volume can easily be recreated from the other output file. | ||
| + | * The output volume is fromcs.hdf, which can be opened with e2display.py or Chimera | ||
| + | * You can also test a standard EMAN2 style iterative refinement with point-based reconstruction, | ||
| + | * e2spa_refine.py --ptcl sets/ | ||
| + | * You may need to look at a full EMAN2 tutorial to pick specific options for your case. The only change is the addition of the --pointrecon option. | ||
eman2/e3make3d_point.1774014940.txt.gz · Last modified: by steveludtke
