Reconstruction Parameters » History » Version 3
Amber Herold, 05/31/2011 12:07 PM
1 | 1 | Amber Herold | h1. Reconstruction Parameters |
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4 | |_.Name|_.a.k.a.|_.Description|_.Used By|_.Required in interface?| |
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5 | 3 | Amber Herold | |Mask Radius|mask|raduius of external map in pixels|xmipp, eman|| |
6 | |Inner Radius||inner radius for alignment in pixels|xmipp|| |
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7 | |imask|Particle inner mask raduius|radius of internal mask (in pixels for eman and spider, Angstroms for frealign)|EMAN, frealign, spider|| |
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8 | 1 | Amber Herold | |Outer Radius|||xmipp|| |
9 | 3 | 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|| |
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12 | |Number of iterations|iteration number||xmipp|| |
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13 | 1 | Amber Herold | |Mask Filename|||xmipp|| |
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 | 3 | Amber Herold | |ang||angular step for projections in degrees|EMAN|| |
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 | |Lower resolution limit or high-pass filter (RMAX1) (in Ångstroms) |||frealign|| |
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51 | |Higher resolution limit or low-pass filter (RMAX2) (in Ångstroms; default 2*Nyquist) |||frealign|| |
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52 | |B-factor correction (RBFACT) (0 = off)|||frealign|| |
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53 | |Only use CTFFIND values|||frealign|| |
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54 | |Last particle to use|||frealign|| |
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55 | |firstring||Any pixels this far away from center will not be used|spider|| |
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56 | |lastring||Only pixels this far away will be used|spider|| |
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57 | |xysearch|||spider|| |
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58 | |lp||low pass filter in angstroms|spider|| |
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59 | |hp||high pass filter in angstroms|spider|| |
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60 | |xyshift||particles only allowed to shift this far from center|spider|| |
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61 | |keep||determines which particles are kept for back-projection, -1 is one standard deviation worse than mean|spider|| |
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62 | |angular increments||list of angular increments for projection mapping|spider|| |