Dear Sir,

 image1.osc
<https://drive.google.com/file/d/1K5hhoMymVyidOjZyR5Hbfb8ny-KkMIm6/view?usp=drive_web>
 image2.osc
<https://drive.google.com/file/d/16TsGwBPtrkVxOYN7M5PxvJyS0pvMljVZ/view?usp=drive_web>
The detector-to-crystal distance was 190 mm. The Oscillation range was 1.0
degree. Please find attached two diffraction images.
With best regards,
Sayan Saha.

On Thu, Jul 28, 2022 at 9:41 PM Sayan Saha <ssaha43...@gmail.com> wrote:

> Dear Sir,
>
> The detector-to-crystal distance was 190 mm. The Oscillation range was 1.0
> degree. Please find attached two diffraction images.
> With best regards,
> Sayan Saha.
>
>
> On Thu, Jul 28, 2022 at 7:31 PM Kay Diederichs <
> kay.diederi...@uni-konstanz.de> wrote:
>
>> Dear Sayan,
>>
>> On Thu, 28 Jul 2022 15:12:30 +0530, Sayan Saha <ssaha43...@gmail.com>
>> wrote:
>>
>> >Dear Sir,
>> >
>> >1. There are no ice-rings. However, diffraction spots seem to be
>> >overlapping. This can be seen during the data processing, as the space
>> >group (C2 or P222) varies even in the consecutive frames.
>>
>> spot overlap results in inaccurate intensity values. Inaccurate
>> intensities result in high Rwork/Rfree.
>>
>> Why do the spots overlap? High mosaicity? Detector distance too small?
>> Oscillation range too high (0.1° is typically adequate)?
>>
>> It would be good to see the data, otherwise we can only speculate.
>>
>> Space group does not change from one frame to the next. If you use XDS, a
>> good guide to decide between higher and lower-symmetry space groups is to
>> compare their ISa values.
>>
>> best,
>> Kay
>>
>> >
>> >2. Crystal packing of C2 and P22121 seem to be similar (please see the
>> >attached images).
>> >
>> >3. Forgot to mention in my previous email that we have already processed
>> >the data in P1 and MR solution could be found only in P1 (Phaser was used
>> >with an option in all possible space groups of that point group).
>> >
>> >Please let me know if any other information is required.
>> >
>> >With best regards,
>> >Sayan Saha.
>> >
>> >
>> >On Thu, Jul 28, 2022 at 1:26 PM Schreuder, Herman /DE <
>> >herman.schreu...@sanofi.com> wrote:
>> >
>> >> Dear Sayan,
>> >>
>> >>
>> >>
>> >> If a subunit is correctly oriented, but the translation is incorrect,
>> >> density for a ligand may still show up in the binding site of the
>> protein.
>> >> It might be that one of the 2-fold axes, you think is
>> crystallographic, is
>> >> in fact non crystallographic and a few Angstroms away from the
>> >> crystallographic position.
>> >>
>> >>
>> >>
>> >> What I would do:
>> >>
>> >>    1. Check the images: are there ice-rings or other artifacts that
>> could
>> >>    cause scaling problems that would lead to high Rw/Rf values? In
>> that case,
>> >>    there is not much you can do.
>> >>    2. Compare the C2 and P22121 solutions: do they have the same
>> overall
>> >>    crystal packing (CS+NCS), or are they different? Do they have the
>> same
>> >>    Rw/Rf values? Can we learn anything from the differences in overall
>> crystal
>> >>    packing?
>> >>    3. Process, run MR and refine in P1. Do you get lower R-factors? If
>> >>    so, then run Zanuda to find out the real space group.
>> >>
>> >>
>> >>
>> >> Best,
>> >>
>> >> Herman
>> >>
>> >>
>> >>
>> >> *Von:* CCP4 bulletin board <CCP4BB@JISCMAIL.AC.UK> *Im Auftrag von
>> *Sayan
>> >> Saha
>> >> *Gesendet:* Donnerstag, 28. Juli 2022 08:15
>> >> *An:* CCP4BB@JISCMAIL.AC.UK
>> >> *Betreff:* [ccp4bb] Regarding the correct space group identification
>> >>
>> >>
>> >>
>> >> Dear All,
>> >>
>> >>
>> >>
>> >> We have collected home-source X-ray intensity data for a protein at 2.6
>> >> Angstrom. The data can be processed in either C2 (a=120, b=80, c=85 and
>> >> beta=115) or P222 (P22121, a=80, b=85, c=110). MR solution can be
>> obtained
>> >> in both the space groups. However, the solution can be refined with an
>> >> Rw/Rf of 29/32% only. The protein is bound to a ligand
>> (co-crystallization)
>> >> for which a clear density can be observed.
>> >>
>> >>
>> >>
>> >> Any help and suggestion in this regard would be very helpful.
>> >>
>> >>
>> >>
>> >> With best regards,
>> >>
>> >> Sayan Saha.
>> >>
>> >>
>> >>
>> >>
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