Reconstruction Parameters » History » Version 21
Amber Herold, 05/31/2011 02:55 PM
1 | 1 | Amber Herold | h1. Reconstruction Parameters |
---|---|---|---|
2 | |||
3 | |||
4 | 19 | Amber Herold | |_.Name|_.a.k.a.|_.Description|_.Used By|_.Make common to all?|_.Notes| |
5 | 18 | Amber Herold | |Outer Mask Radius|Outer Radius, mask|raduius of external map in pixels|xmipp, eman, imagic|y|| |
6 | 1 | Amber Herold | |Inner Mask Radius|Inner Radius,Particle inner mask radius|inner radius for alignment in pixels|xmipp, frealign, spider|y|| |
7 | 19 | Amber Herold | |Outer Alignment Radius|||xmipp, eman, imagic|y|| |
8 | |Inner Alignment Radius|||xmipp, eman, imagic|y|| |
||
9 | 21 | Amber Herold | |Symmetry Group|sym|ex. c1, c2...|xmipp,eman,frealign,spider,imagic|y|| |
10 | |Number of iterations|iteration number||xmipp|y|| |
||
11 | |Angular Sampling Rate|ang|angular step for projections in degrees|xmipp,EMAN|y|not frealign| |
||
12 | |Percentage of worst images to discard|||xmipp|y|not frealign| |
||
13 | 10 | Amber Herold | |imask||radius of internal mask (in pixels for eman and spider, Angstroms for frealign)|EMAN||| |
14 | 18 | Amber Herold | ||||||| |
15 | 1 | Amber Herold | |Particle outer mask radius (RO)|mask|radius from center of particle to outer edge (frealign in angstroms, spider in pixels)|frealign, spider||| |
16 | 10 | Amber Herold | |amask||amask=[r],[threshold],[iter]|eman||| |
17 | 1 | Amber Herold | |Mask Filename|||xmipp||| |
18 | 10 | Amber Herold | |Max angular change|||xmipp||| |
19 | |max change offset|||xmipp||| |
||
20 | 19 | Amber Herold | |Search range for 5d transitional search|||xmipp||| |
21 | 1 | Amber Herold | |Reconstruction Method|||xmipp||| |
22 | 10 | Amber Herold | |Values of lambda for ART|||xmipp||| |
23 | |Initial max frequency used by reconstruct fourier|||xmipp||| |
||
24 | |Compute resolution?|||xmipp||don't need this, should always be set to yes| |
||
25 | 21 | Amber Herold | |filt3d||applies gaussian low pass filter in pixels [rad]|eman||| |
26 | 10 | Amber Herold | |Low Pass Filter the reference?|||xmipp||| |
27 | |Do not use estimated resolution for low-pass filtering?|||xmipp||| |
||
28 | |Constant to add to the estimated resolution|||xmipp||| |
||
29 | |maxshift||max translation during image alignment in pixels|eman||| |
||
30 | |hard||hard limit for make3d program|eman||| |
||
31 | |clskeep||=[std dev multipier] how many raw particles discarded for each class average|eman||| |
||
32 | |clsiter||iterative alignmnet to each other|eman||| |
||
33 | |xfiles||=[mas in kD]|eman||| |
||
34 | |shrink||scale down by a factor of [n] before classification|eman||| |
||
35 | |euler2||=[oversample factor]|eman||| |
||
36 | |median||use median value instead of average for each pixel|eman||| |
||
37 | |phscls||use signal to noise ratio weighted phase residual|eman||| |
||
38 | |refine||do subpixel alignment|eman||| |
||
39 | |tree||decimate reference populatiuon|eman||| |
||
40 | |coran||use coran algorithm|eman||| |
||
41 | |eotest||use even odd test|eman||| |
||
42 | |amplitude contrast (WGH)|||frealign||| |
||
43 | |Standard deviation filtering|||fealign||| |
||
44 | |Phase B-factor weighting constant (PBC) |||frealign||| |
||
45 | |B-factor offset (BOFF) |||frealign||| |
||
46 | |Number of randomized search trials (ITMAX) |||frealign||| |
||
47 | |Number of potential matches to refine (IPMAX)|||frealign||| |
||
48 | |Target phase residual (TARGET) |||frealign||| |
||
49 | |Worst phase residual for inclusion (THRESH)|||frealign||| |
||
50 | |Resolution limit of reconstruction (RREC) (in Ångstroms; default Nyquist) |||frealign||| |
||
51 | |lp|filtering|low pass filter in angstroms|spider, imagic||| |
||
52 | 1 | Amber Herold | |hp|filtering|high pass filter in angstroms|spider, imagic||| |
53 | 10 | Amber Herold | |Lower resolution limit or high-pass filter (RMAX1) (in Ångstroms) |||frealign||| |
54 | |Higher resolution limit or low-pass filter (RMAX2) (in Ångstroms; default 2*Nyquist) |||frealign||| |
||
55 | |B-factor correction (RBFACT) (0 = off)|||frealign||| |
||
56 | |Only use CTFFIND values|||frealign||| |
||
57 | 1 | Amber Herold | |Last particle to use|||frealign||| |
58 | 13 | Amber Herold | ||||||| |
59 | 1 | Amber Herold | |MSA - num class averges to produce from raw images|||imagic||| |
60 | |MSA - num factors to use for classification|||imagic||| |
||
61 | |MSA - percentage of worst class members to ignore after classification|||imagic||| |
||
62 | |threed reconstruction||object size, low-pass filter 3d volume|imagic||| |
||
63 | |Center stack prior to alignment |||imagic||| |
||
64 | |Mirror references for alignment |||imagic||| |
||
65 | 12 | Amber Herold | |MRA - min radius for rotational alignment in pixels|||imagic||| |
66 | |MRA - max radius for rotational alignment in pixels|||imagic||| |
||
67 | 1 | Amber Herold | |MSA - fraction of final class averages to keep|||imagic||| |
68 | |MRA - angular increment of forward projections|||imagic||| |
||
69 | |MRA - max radial shift compared to original images|||imagic||| |
||
70 | |MRA - max radial shift during this iteration|||imagic||| |
||
71 | |MSA - percentage of images to ignore when calculating eiganimages|||imagic||| |
||
72 | |Angular reconstitution||angular increment of forward projections, ang inc of euler search, fraction of best ordered images to keep|imagic||| |
||
73 | 13 | Amber Herold | |firstring||Any pixels this far away from center will not be used|spider||| |
74 | |lastring||Only pixels this far away will be used|spider||| |
||
75 | |xysearch||translational search during projection matching will be limited to this many pixels from the center ofthe image|spider||| |
||
76 | |angular increments||list of angular increments for projection mapping|spider||| |
||
77 | |keep||determines which particles are kept for back-projection, -1 is one standard deviation worse than mean|spider||| |
||
78 | 1 | Amber Herold | |xyshift||particles only allowed to shift this far from center|spider||| |
79 | 14 | Amber Herold | |Approximate mass in Kd |||imagic||| |