Dear Auto,

with such crystals diffracting like rocks, it can be useful to collect two datasets. One at “low" resolution (up to 3A)  using low exposure time and/or low dose to avoid overloads and a second at higher resolution (1A in your case) using higher dose. Then, merge those two datasets into a single one using all reflections from the “low resolution” dataset and for instance data from 5 to 1A for the high resolution data (to exclude overloads). It may improve the Rmeas values at low resolution.

My two cents.

Marc


Marc GRAILLE, PhD
Directeur de recherche CNRS

Laboratoire de Biochimie
ECOLE POLYTECHNIQUE - UMR7654 CNRS
91128 PALAISEAU CEDEX
FRANCE



To unsubscribe from the CCP4BB list, click the following link:
https://www.jiscmail.ac.uk/cgi-bin/webadmin?SUBED1=CCP4BB&A=1



Phone : +33 (0)1 69 33 48 90 – Fax : +33 (0)1 69 33 49 09
Email: marc.grai...@polytechnique.edu

Team: Translation and degradation of eukaryotic mRNAs
https://portail.polytechnique.edu/bioc/recherche/couplage-entre-la-traduction-et-la-degradation-des-arnm-chez-les-eucaryotes
Team supported by the ATIP-Avenir CNRS program

Le 9 oct. 2018 à 19:12, Guto Rhys <guto.r...@bristol.ac.uk> a écrit :

Hi all,

I have a 1.05 Angstrom dataset that I was able to phase but the refined model only has an Rfree of approximately 0.25. The dataset includes 1800 images and, as the crystal did not suffer significantly from radiation damage, comprises all 360 deg. Auto-processing pipelines at diamond light source all suggest I222. I have also indexed the data in iMOSFLM, which has the highest-symmetry Laue group that is least penalised of I422. Subsequent scaling and merging in AIMLESS strongly indicates that I222 is the likely space group (see below). I have ran the refined model through ZANUDA, which has similar R values to lower symmetry space groups (see below). The output from Phenix Xtriage does not find any specific crystal pathologies and if twinning is present it is very low (2 to 4%, see below). The difference map suggests that the model accounts for nearly all the density. Any ideas or direction would be greatly appreciated.

Best,
Guto


AIMLESS Summary
  Overall  InnerShell  OuterShell
Low resolution limit                       27.75     27.75      1.07
High resolution limit                       1.05      5.75      1.05

Rmerge  (within I+/I-)                     0.050     0.078     0.466
Rmerge  (all I+ and I-)                    0.051     0.080     0.536
Rmeas (within I+/I-)                       0.055     0.086     0.591
Rmeas (all I+ & I-)                        0.054     0.085     0.613
Rpim (within I+/I-)                        0.023     0.034     0.359
Rpim (all I+ & I-)                         0.017     0.028     0.288
Rmerge in top intensity bin                0.049        -         -
Total number of observations              107950       779      1972
Total number unique                        11315        88       486
Mean((I)/sd(I))                             19.7      46.2       1.8
Mn(I) half-set correlation CC(1/2)         0.998     0.994     0.796
Completeness                                99.1      99.2      90.4
Multiplicity                                 9.5       8.9       4.1

Anomalous completeness                      98.1     100.0      79.1
Anomalous multiplicity                       5.0       6.4       2.2
DelAnom correlation between half-sets     -0.067     0.286     0.097
Mid-Slope of Anom Normal Probability       0.789       -         -  

Estimate of maximum resolution for significant anomalous signal =  1.14A, from CCanom >  0.15

Estimates of resolution limits: overall
  from half-dataset correlation CC(1/2) >  0.30: limit =  1.05A  == maximum resolution
  from Mn(I/sd) >  1.50:                         limit =  1.05A  == maximum resolution
  from Mn(I/sd) >  2.00:                         limit =  1.07A

Estimates of resolution limits in reciprocal lattice directions:
 Along h axis
  from half-dataset correlation CC(1/2) >  0.30: limit =  1.06A
  from Mn(I/sd) >  1.50:                         limit =  1.09A
 Along k axis
  from half-dataset correlation CC(1/2) >  0.30: limit =  1.11A
  from Mn(I/sd) >  1.50:                         limit =  1.13A
 Along l axis
  from half-dataset correlation CC(1/2) >  0.30: limit =  1.05A  == maximum resolution
  from Mn(I/sd) >  1.50:                         limit =  1.05A

Anisotropic deltaB (i.e. range of principal components), A^2:  6.40

Average unit cell:   29.12   29.26   55.50   90.00   90.00   90.00
Space group: I 2 2 2
Average mosaicity:   0.36

AIMLESS Laue Group prediction

  Laue Group        Lklhd   NetZc  Zc+   Zc-    CC    CC-  Rmeas   R-  Delta ReindexOperator

= 1    I m m m  ***  0.987   6.25  9.19  2.94   0.92  0.29   0.07  0.49   0.0 [h,k,l]
 2  I 1 2/m 1       0.004   4.36  9.32  4.96   0.93  0.50   0.07  0.30   0.0 [-h,-k,l]
 3  I 1 2/m 1       0.004   4.14  9.24  5.10   0.92  0.51   0.07  0.30   0.0 [k,-h,l]
 4  I 1 2/m 1       0.004   4.05  9.23  5.18   0.92  0.52   0.06  0.31   0.0 [h,-l,k]
 5  I 4/m m m       0.000   6.35  6.35  0.00   0.64  0.00   0.22  0.00   0.3 [h,k,l]
 6      I 4/m       0.000   0.90  6.83  5.93   0.68  0.59   0.17  0.26   0.3 [h,k,l]
 7       P -1       0.000   3.69  9.36  5.67   0.94  0.57   0.06  0.26   0.0 [-h,k,1/2h-1/2k-1/2l]
 8  I 1 2/m 1       0.000   0.08  6.40  6.33   0.64  0.63   0.23  0.22   0.3 [-1/2h+1/2k-1/2l,-h-k,-1/2h+1/2k+1/2l]
 9    F m m m       0.000  -0.43  6.17  6.60   0.62  0.66   0.24  0.20   0.3 [h+k,-h+k,l]
10  I 1 2/m 1       0.000   0.75  6.89  6.14   0.69  0.61   0.22  0.22   0.3 [-1/2h-1/2k-1/2l,h-k,-1/2h-1/2k+1/2l]


Xtriage Summary

Twinning and intensity statistics summary (acentric data):

Statistics independent of twin laws
 <I^2>/<I>^2 : 2.126  (untwinned: 2.0, perfect twin: 1.5)
 <F>^2/<F^2> : 0.774  (untwinned: 0.785, perfect twin: 0.885)
 <|E^2-1|>   : 0.761  (untwinned: 0.736, perfect twin: 0.541)
 <|L|>, <L^2>: 0.490, 0.323
 Multivariate Z score L-test: 1.303

The multivariate Z score is a quality measure of the given
spread in intensities. Good to reasonable data are expected
to have a Z score lower than 3.5.
Large values can indicate twinning, but small values do not
necessarily exclude it.



Statistics depending on twin laws
-----------------------------------------------------------------------------------
| Operator | type | R_abs obs. | R_abs calc. | Britton alpha | H alpha | ML alpha |
-----------------------------------------------------------------------------------
| k,h,-l   |  PM  | 0.469      | 0.478       | 0.016         | 0.041   | 0.022    |
-----------------------------------------------------------------------------------

Patterson analyses
 - Largest peak height   : 13.667
  (corresponding p value : 0.04780)


The largest off-origin peak in the Patterson function is 13.67% of the
height of the origin peak. No significant pseudotranslation is detected.

The results of the L-test indicate that the intensity statistics
behave as expected. No twinning is suspected.

Zanuda output

  Step 2.
  Refinements in subgroups.
  There are 5 subgroups to test.

  current time:                                        Jan 08 16:20 GMT
  expected end of job:                                 Jan 08 16:28 GMT

  ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
  | >>   5   | I 2 2 2    |  0.0005  |    --    |    --    |    --    |
  ---------------------------------------------------------------------
  |      1   | P 1        |  0.0731  |  0.3242  |  0.2842  |  0.2768  |
  |      2   | C 1 2 1    |  0.0755  |  0.3796  |  0.2899  |  0.2799  |
  |      3   | C 1 2 1    |  0.0727  |  0.3385  |  0.2909  |  0.2806  |
  |      4   | C 1 2 1    |  0.0729  |  0.3398  |  0.2900  |  0.2813  |
  |      5   | I 2 2 2    |  0.0707  |  0.3582  |  0.2976  |  0.2802  |
  ---------------------------------------------------------------------
  | <<   1   | P 1        |  0.0731  |  0.3242  |  0.2842  |  0.2768  |
  ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^

  Step 3.
  Refinement of the best model.
  Candidate symmetry elements are added one by one.

  current time:                                        Jan 08 16:25 GMT
  expected end of job:                                 Jan 08 16:28 GMT

  ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
  | >>   1   | P 1        |  0.0731  |  0.3242  |  0.2842  |  0.2768  |
  ---------------------------------------------------------------------
  |      1   | P 1        |  0.0730  |  0.3243  |  0.2842  |  0.2768  |
  |      4   | C 1 2 1    |  0.0751  |    --    |  0.2896  |  0.2826  |
  |      5   | I 2 2 2    |  0.0737  |    --    |  0.2970  |  0.2801  |
  ---------------------------------------------------------------------
  | <<   5   | I 2 2 2    |  0.0737  |    --    |  0.2970  |  0.2801  |
  ---------------------------------------------------------------------

  R-factor in the original subgroup is (almost) the best.
  The original spacegroup assignment seems to be correct.

########################################################################

To unsubscribe from the CCP4BB list, click the following link:
https://www.jiscmail.ac.uk/cgi-bin/webadmin?SUBED1=CCP4BB&A=1



To unsubscribe from the CCP4BB list, click the following link:
https://www.jiscmail.ac.uk/cgi-bin/webadmin?SUBED1=CCP4BB&A=1

Reply via email to