Excellent point about R-factors. Indeed, at this resolution they should be
quite lower than what you have. Did you:
- model solvent?
- use anisotropic ADPs?
- add H (this alone can drop R by 1-2%)?
- model alternative conformations?
- How R-factors (Rwork) look in resolution?
Pavel


On Mon, Aug 26, 2013 at 10:47 PM, Emily Golden
<10417...@student.uwa.edu.au>wrote:

> Thanks Yuriy and Pavel,
>
> at this resolution one would expect R/Rfree to be ~ 10-11%/12-13% assuming
> you applied anisotropic B-factor refinement ( and probably having  a low
> symmetry SG).
> R merge of 80% may be OK if I/sig for high res shell is >2.
>
> Yes, I used anisotropic Bfactors and the space group is P1 21 1.  However,
> the I/sig is only 1.5 in the highest shell.   Cutting the data such that
> the I/sig is >2 has improved the R factors.  Thank you.
>
> Maps get worse.... Could it be when you use all resolution range you get
> 59% of missing reflections in highest resolution shell filled in with DFc
> for the purpose of map calculation?
>
> Yes! the map that I was looking at was filled.
>
> Emily
>
>
> On 27 August 2013 09:49, Emily Golden <10417...@student.uwa.edu.au> wrote:
>
>> Hi All,
>>
>> I have collected diffraction images to 1 Angstrom resolution to the edge
>> of the detector and 0.9A to the corner.    I collected two sets, one for
>> low resolution reflections and one for high resolution reflections.
>> I get 100% completeness above 1A and 41% completeness in the 0.9A-0.95A
>> shell.
>>
>> However, my Rmerge in the highest shelll is not good, ~80%.
>>
>> The Rfree is 0.17 and Rwork is 0.16 but the maps look very good.   If I
>> cut the data to 1 Angstrom the R factors improve but I feel the maps are
>> not as good and I'm not sure if I can justify cutting data.
>>
>> So my question is,  should I cut the data to 1Angstrom or should I keep
>> the data I have?
>>
>> Also, taking geometric restraints off during refinement the Rfactors
>> improve marginally, am I justified in doing this at this resolution?
>>
>> Thank you,
>>
>> Emily
>>
>
>

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