Gerard, of course you are right and I was confused. Twinning causes too few 
weak intensities and too few strong ones, ie reduced variance of the 
distribution. 

But this distribution is certainly wrong!

Phil

> On 29 May 2025, at 18:06, Gerard Bricogne 
> <0000ead34ec923cf-dmarc-requ...@jiscmail.ac.uk> wrote:
> 
> CAUTION: This email originated from outside of the LMB:
> .-owner-ccp...@jiscmail.ac.uk-.
> Do not click links or open attachments unless you recognize the sender and 
> know the content is safe.
> If you think this is a phishing email, please forward it to 
> phish...@mrc-lmb.cam.ac.uk
> --
> 
> Dear Phil,
> 
>     I am not sure that I follow you there: perfectly twinned acentric
> intensities will follow a Chi-squared distribution with four degrees
> of freedom, while untwinned ones have only two degrees of freedom. The
> higher the number of degrees of freedom, the more the Chi-squared
> distribution will peak around its mean value (Central Limit Theorem).
> This trend is clearly visible in going from the red to the blue curve.
> 
>     The green curve shows an even stronger trend towards a peaked
> distribution, so actually the data coming our of 20240712 are, so to
> speak, "hyper-twinned". This shift away from low values is consistent
> with Gleb Bourenkov's findings, obtained by integrating images with
> very low signal created with our image simulator, that integrated
> intensities produced by the six successive buggy versions of XDS since
> July last year (20240712, 20240723, 20241002, 20250119, 20250224 and
> 20250320) were affected by biases, mostly positive and causing a
> depletion of the weak intensity population (hence spurious twinning
> diagnostics), plus an overestimation of I/sig(I) and even Wilson plots
> curving upwards (!) at high resolution.
> 
>     Please peruse the autoPROC Wiki page for which I sent a link
> earlier and take a look at the plots it contains: it is all described
> in there.
> 
> 
>     With best wishes,
> 
>          Gerard.
> 
> --
> On Thu, May 29, 2025 at 05:30:54PM +0100, Phil Evans wrote:
>> Dear Kay
>> 
>> This is a plot I sent to Eleanor yesterday, from her log file. The 
>> cumulative intensity plot shows I think that there are too few weak 
>> intensities, the opposite of twinning. I don;t know where it comes from but 
>> it’s not right!
>> Best
>> Phil
>> 
>> ########################################################################
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>> 
>> 
>> 
>>> On 29 May 2025, at 12:03, Kay Diederichs <kay.diederi...@uni-konstanz.de> 
>>> wrote:
>>> 
>>> CAUTION: This email originated from outside of the LMB:
>>> .-owner-ccp...@jiscmail.ac.uk-.
>>> Do not click links or open attachments unless you recognize the sender and 
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>>> If you think this is a phishing email, please forward it to 
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>>> --
>>> 
>>> Dear Gerard,
>>> 
>>> part of the problem was probably indeed due to the use of XDS 
>>> BUILT=20240712 (that version was used for CORRECT.LP that Janani Ganesh 
>>> sent to me). I obtained the raw data from Janani Ganesh and processed with 
>>> both the current XDS (BUILT=20250430), and the bad version from July last 
>>> year. My findings:
>>> - with the bad version the data appear twinned, whereas with the current 
>>> version the data appear untwinned
>>> - Wilson B is 34 A^2 with the current version, and significantly (and 
>>> unrealistically) lower with the bad version
>>> 
>>> The structure can be satisfactorily solved and refined with data from the 
>>> current XDS version. With data from the bad version, average B goes down to 
>>> 19 and the R-values stall at high values.
>>> 
>>> This does not explain the weird B-values that were reported, though. So I 
>>> suspect another problem.
>>> 
>>> Best,
>>> Kay
>>> 
>>> 
>>> 
>>> On Thu, 29 May 2025 11:37:14 +0100, Gerard Bricogne 
>>> <g...@globalphasing.com> wrote:
>>> 
>>>> Dear all,
>>>> 
>>>>   I wrote yesterday a contribution to this thread, but mistakenly
>>>> used a simple Reply instead of a Group Reply, so that my message did
>>>> not reach the BB while it intended to, as shown by the introductory
>>>> "Dear all". 
>>>> 
>>>>   I am including it below, as it contains a link to some material
>>>> that is of general interest but that we had not yet found a way of
>>>> disseminating to the whole community. Users of XDS, or of XDS-based
>>>> pipelines, please take notice and do take a close look at this link,
>>>> and ultimately at the BUILT= information about the exact XDS version
>>>> used in producing your results - it can make a lot of difference.
>>>> 
>>>> 
>>>>   With best wishes,
>>>> 
>>>>        Gerard.
>>>> 
>>>> --
>>>> Date: Wed, 28 May 2025 16:18:25 +0100
>>>> From: Gerard Bricogne <gb10>
>>>> Subject: Re: [ccp4bb] Requesting help with twin refinement
>>>> To: Eleanor Dodson <eleanor.dod...@york.ac.uk>
>>>> 
>>>> Dear all,
>>>> 
>>>>   These kinds of anomalies (overoptimistic estimates of resolution,
>>>> unphysical persistence of signal at high resolution, spurious twinning
>>>> diagnostics) are reminiscent of what we observed with some of the
>>>> recent versions of XDS, as documented at
>>>> 
>>>> https://www.globalphasing.com/autoproc/wiki/index.cgi?ComparisonProcessing202504
>>>> 
>>>> and three predecessor pages referenced from within this one.
>>>> 
>>>>   Only one version is currently available from the XDS download
>>>> page (that we consider as being OK) but there was a succession of many
>>>> problematic ones going back to July 2024. Perhaps the version used to
>>>> process this dataset was one of the unlucky ones.
>>>> 
>>>>   Apologies if this is a red herring, but that check is worth
>>>> making.
>>>> 
>>>> 
>>>>   Best wishes,
>>>> 
>>>>      Gerard
>>>> 
>>>> --
>>>> On Thu, May 29, 2025 at 11:05:52AM +0100, Eleanor Dodson wrote:
>>>>> After inspecting the log files it is obvious the problem is in the data
>>>>> integration. (Wilson B negative! highest resolution shell stronger than 
>>>>> low
>>>>> res, etc..)
>>>>> I think you used XDS for that? Do you have an alternative set of 
>>>>> integrated
>>>>> unmerged data, eg done with DIALS?
>>>>> If so I would use that, or download a new version of XDS and try again..
>>>>> 
>>>>> On Wed, 28 May 2025 at 07:56, Janani Ganesh <jganesh3...@gmail.com> wrote:
>>>>> 
>>>>>> Dear Martin,
>>>>>> 
>>>>>> Thank you for your suggestion. I will try it out and let you know.
>>>>>> 
>>>>>> Regards,
>>>>>> Janani Ganesh
>>>>>> 
>>>>>> On Tue, 27 May 2025 09:01:06 +0100, Martin Mal� <martin.maly...@email.cz>
>>>>>> wrote:
>>>>>> 
>>>>>>> Dear Janani,
>>>>>>> 
>>>>>>> There has been recently a significant development in twin refinement
>>>>>>> algorithms in Servalcat. Could you try this program and let us know if
>>>>>>> it helps?
>>>>>>> You can find Servalcat in i2 in the most recent version of CCP4. You can
>>>>>>> also run it in terminal/CCP4Console:
>>>>>>> servalcat refine_xtal_norefmac --hklin data.mtz --model model.pdb -s
>>>>>>> xray --labin I,IMEAN,FreeR_flag --twin
>>>>>>> (Assuming your MTZ data file has columns I,IMEAN,FreeR_flag.)
>>>>>>> 
>>>>>>> Full list of options:
>>>>>>> servalcat refine_xtal_norefmac -h
>>>>>>> 
>>>>>>> Please feel free to ask if anything was not clear.
>>>>>>> Cheers,
>>>>>>> Martin
>>>>>>> 
>>>>>>> 
>>>>>>> On 27/05/2025 07:00, Janani Ganesh wrote:
>>>>>>>> Hello,
>>>>>>>> 
>>>>>>>> I recently collected diffraction data and I was able to do the data
>>>>>> processing upto 1.88 �. I observed the R-merge remained the same 
>>>>>> throughout
>>>>>> the resolution bins. I could solve the structure using Phaser in the 
>>>>>> space
>>>>>> group P32 2 1 (no. 154). But when I refined the structure the R-factors
>>>>>> remained ~ 35 % even after several cycles of refinement and model 
>>>>>> building.
>>>>>>>> 
>>>>>>>> Then I looked for twinning in my data using Xtriage, Detwin, Pointless,
>>>>>> etc which indicated twining. Subsequently, I started twin refinement with
>>>>>> Refmac using twin law (-h, -k, l). The R-factors came down to ~25%.
>>>>>> However, the B-factors refined to 0.5 for all the atoms.  I tried redoing
>>>>>> the data processing at lower symmetry space groups, P3, P31, P32, 
>>>>>> followed
>>>>>> by twin refinement but the issue with the B-factors persisted.
>>>>>>>> 
>>>>>>>> I would appreciate any suggestions and advice towards resolving this
>>>>>> problem.
>>>>>>>> 
>>>>>>>> Regards,
>>>>>>>> Janani Ganesh
>>>>>>>> 
>>>>>>>> ########################################################################
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