Reconstruction Parameters » History » Version 15
Amber Herold, 05/31/2011 02:18 PM
1 | 1 | Amber Herold | h1. Reconstruction Parameters |
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4 | 10 | Amber Herold | |_.Name|_.a.k.a.|_.Description|_.Used By|_.Required in interface?|_.Notes| |
5 | 15 | Amber Herold | |Outer Mask Radius|Outer Radius, mask|raduius of external map in pixels|xmipp, eman, imagic||| |
6 | |Inner Mask Radius|Inner Radius,Particle inner mask radius|inner radius for alignment in pixels|xmipp, frealign, spider||| |
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7 | 11 | Amber Herold | |imask||radius of internal mask (in pixels for eman and spider, Angstroms for frealign)|EMAN||| |
8 | 15 | Amber Herold | ||||xmipp||| |
9 | 10 | Amber Herold | |Particle outer mask radius (RO)|mask|radius from center of particle to outer edge (frealign in angstroms, spider in pixels)|frealign, spider||| |
10 | |amask||amask=[r],[threshold],[iter]|eman||| |
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11 | |Symmetry Group|sym|ex. c1, c2...|xmipp,eman,frealign,spider,imagic||| |
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12 | |Number of iterations|iteration number||xmipp||| |
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13 | |Mask Filename|||xmipp||| |
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14 | |Angular Sampling Rate|||xmipp||| |
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15 | |Max angular change|||xmipp||| |
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16 | |max change offset|||xmipp||| |
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17 | |Search range for 5d transitional search|||xmipp||| |
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18 | |Discard % of image with CCF below|||xmipp||| |
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19 | |Reconstruction Method|||xmipp||| |
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20 | |Values of lambda for ART|||xmipp||| |
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21 | |Initial max frequency used by reconstruct fourier|||xmipp||| |
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22 | |Compute resolution?|||xmipp||| |
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23 | |Low Pass Filter the reference?|||xmipp||| |
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24 | |Do not use estimated resolution for low-pass filtering?|||xmipp||| |
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25 | |Constant to add to the estimated resolution|||xmipp||| |
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26 | |ang||angular step for projections in degrees|EMAN||| |
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27 | |maxshift||max translation during image alignment in pixels|eman||| |
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28 | |hard||hard limit for make3d program|eman||| |
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29 | |clskeep||=[std dev multipier] how many raw particles discarded for each class average|eman||| |
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30 | |clsiter||iterative alignmnet to each other|eman||| |
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31 | |filt3d||applies gaussian low pass filter in pixels [rad]|eman||| |
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32 | |xfiles||=[mas in kD]|eman||| |
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33 | |shrink||scale down by a factor of [n] before classification|eman||| |
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34 | |euler2||=[oversample factor]|eman||| |
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35 | |median||use median value instead of average for each pixel|eman||| |
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36 | |phscls||use signal to noise ratio weighted phase residual|eman||| |
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37 | |refine||do subpixel alignment|eman||| |
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38 | |tree||decimate reference populatiuon|eman||| |
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39 | |coran||use coran algorithm|eman||| |
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40 | |eotest||use even odd test|eman||| |
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41 | |amplitude contrast (WGH)|||frealign||| |
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42 | |Standard deviation filtering|||fealign||| |
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43 | |Phase B-factor weighting constant (PBC) |||frealign||| |
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44 | |B-factor offset (BOFF) |||frealign||| |
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45 | |Number of randomized search trials (ITMAX) |||frealign||| |
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46 | |Number of potential matches to refine (IPMAX)|||frealign||| |
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47 | |Target phase residual (TARGET) |||frealign||| |
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48 | |Worst phase residual for inclusion (THRESH)|||frealign||| |
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49 | |Resolution limit of reconstruction (RREC) (in Ångstroms; default Nyquist) |||frealign||| |
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50 | |lp|filtering|low pass filter in angstroms|spider, imagic||| |
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51 | 1 | Amber Herold | |hp|filtering|high pass filter in angstroms|spider, imagic||| |
52 | 10 | Amber Herold | |Lower resolution limit or high-pass filter (RMAX1) (in Ångstroms) |||frealign||| |
53 | |Higher resolution limit or low-pass filter (RMAX2) (in Ångstroms; default 2*Nyquist) |||frealign||| |
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54 | |B-factor correction (RBFACT) (0 = off)|||frealign||| |
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55 | |Only use CTFFIND values|||frealign||| |
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56 | 1 | Amber Herold | |Last particle to use|||frealign||| |
57 | 13 | Amber Herold | ||||||| |
58 | 1 | Amber Herold | |MSA - num class averges to produce from raw images|||imagic||| |
59 | |MSA - num factors to use for classification|||imagic||| |
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60 | |MSA - percentage of worst class members to ignore after classification|||imagic||| |
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61 | |threed reconstruction||object size, low-pass filter 3d volume|imagic||| |
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62 | |Center stack prior to alignment |||imagic||| |
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63 | |Mirror references for alignment |||imagic||| |
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64 | 12 | Amber Herold | |MRA - min radius for rotational alignment in pixels|||imagic||| |
65 | |MRA - max radius for rotational alignment in pixels|||imagic||| |
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66 | 1 | Amber Herold | |MSA - fraction of final class averages to keep|||imagic||| |
67 | |MRA - angular increment of forward projections|||imagic||| |
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68 | |MRA - max radial shift compared to original images|||imagic||| |
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69 | |MRA - max radial shift during this iteration|||imagic||| |
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70 | |MSA - percentage of images to ignore when calculating eiganimages|||imagic||| |
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71 | |Angular reconstitution||angular increment of forward projections, ang inc of euler search, fraction of best ordered images to keep|imagic||| |
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72 | 13 | Amber Herold | |firstring||Any pixels this far away from center will not be used|spider||| |
73 | |lastring||Only pixels this far away will be used|spider||| |
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74 | |xysearch||translational search during projection matching will be limited to this many pixels from the center ofthe image|spider||| |
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75 | |angular increments||list of angular increments for projection mapping|spider||| |
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76 | |keep||determines which particles are kept for back-projection, -1 is one standard deviation worse than mean|spider||| |
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77 | 1 | Amber Herold | |xyshift||particles only allowed to shift this far from center|spider||| |
78 | 14 | Amber Herold | |Approximate mass in Kd |||imagic||| |