JiscMail Logo
Email discussion lists for the UK Education and Research communities

Help for CCP4BB Archives


CCP4BB Archives

CCP4BB Archives


CCP4BB@JISCMAIL.AC.UK


View:

Message:

[

First

|

Previous

|

Next

|

Last

]

By Topic:

[

First

|

Previous

|

Next

|

Last

]

By Author:

[

First

|

Previous

|

Next

|

Last

]

Font:

Proportional Font

LISTSERV Archives

LISTSERV Archives

CCP4BB Home

CCP4BB Home

CCP4BB  January 2013

CCP4BB January 2013

Options

Subscribe or Unsubscribe

Subscribe or Unsubscribe

Log In

Log In

Get Password

Get Password

Subject:

Re: a challenge

From:

"George M. Sheldrick" <[log in to unmask]>

Reply-To:

George M. Sheldrick

Date:

Tue, 15 Jan 2013 15:33:53 +0100

Content-Type:

text/plain

Parts/Attachments:

Parts/Attachments

text/plain (224 lines)

Dear Santosh,

I think that it is a bit more complicated. SIR generally provides a
stronger phasing signal than SAD, and can be better for phasing,
provided that:

(a) the native and derivative are sufficiently isomorphous, AND
(b) the heavy atom substructure is itself chiral.

For some space groups one site is enough to generate a chiral
substructure but for others, e.g.P21, more than one site is necessary.
Otherwise the first map will be a double image consisting of two
overlapping positive images, and density modification will not in
general be able to untangle them. SAD also gives a double image in such
cases, but then instead of two positive images we have one negative and
one positive image, and the simplest form of density modification -
setting negative density to zero - will break the pseudosymmetry. One
can also break such pseudosymmetry by using SIRAS or RIPAS instead of
SIR or RIP, even if the anomalous signal alone is not sufficient to
phase the structure.

If MAD doesn't work and one happens to have a native (Met) dataset as
well as SeMet, one should always consider analyzing the data as SIRAS.
Whether this is better than SAD on the SeMet data alone will depend
primarily on how isomorphous the two datasets are.

Best wishes, George


On 01/15/2013 11:06 AM, Santosh Panjikar wrote:
> Hi James,
> The datasets frac.80.mtz to frac.100.mtz are challenging to solve using SAD phasing. However these datasets can be  easily solved using
> other  experimental phasing method. Instead of using anomalous signal we could use isomorphous signal only. For example RIP or SIR
> phasing method, as there is a difference in intensity between the datasets due to scattering of S and Se. Since frac.80.mtz data contains
> 20% selenium that is sufficient to solve the structure against the frac.100.mtz. It seems the structure can be solved even as less as 10%
> selenium content (frac.90.mtz vs frac.100.mtz), and substructure can be solved easily. This is not surprising, the pair of the datasets is
> quite isomorphous, . We phase all  reflections (centric and non-centric) where as  anomalous phasing we could phase non-centric reflections
>  only. In fact, Single Isomorphous Replacement phasing method is the first phasing technique. This method has been further extended by
> Ravelli et al with some deviation by introduction of X-ray or UV RIP phasing.
>
> I  tried RIP (SIR)  phasing protocol of Auto-Rickshaw using frac.90.mtz  as "before" and frac.100.mtz as "after". Auto-Rickshaw used
> SHELXC/D/E and ARP/wARP/REFMAC5  to get the partially refined model (Rfree below 30%) .
>
> Cheers
> Santosh
>
> Santosh Panjikar, Ph.D.
> Scientist
> Australian Synchrotron
> 800 Blackburn Road
> Clayton VIC 3168
> Australia
> Ph: +61-4-67770851
> ________________________________________
> From: CCP4 bulletin board [[log in to unmask]] On Behalf Of James Holton [[log in to unmask]]
> Sent: Monday, January 14, 2013 8:12 PM
> To: [log in to unmask]
> Subject: Re: [ccp4bb] a challenge
>
> I am absolutely delighted at the response I have gotten to my little
> "John Henry Challenge"!  Three people already have managed to do the
> "impossible".  Congratulations to George Sheldrick, Pavol Skubak and Raj
> Pannu for finding ways to improve the phases over the ones I originally
> obtained (using the default settings of mlphare and dm) and build their
> way out of it.  This is quite useful information!  At least it is to me.
>
> Nevertheless, I do think Frances Reyes has a point.  This was meant to
> be a map interpretation challenge, and not a SAD-phasing challenge.  I
> appreciate that the two are linked, but the reason I did not initially
> provide the anomalous data is because I thought it would be too much to
> ask people to re-do all the phasing, etc. Yes, there do appear to be
> ways to improve the maps beyond the particular way I phased them, but no
> matter how good your phasing program is, there will always be a level of
> anomalous signal that will lead to phases that are "off" enough to make
> building the model "impossible".  Basically, once the map gets bad
> enough that just as many "wrong" atoms get built in as "right" atoms,
> then there is no escape.  However, I think human beings should still
> have an advantage when it comes to pattern recognition, and I remain
> curious to see if an insightful crystallographer can tip that balance in
> the right direction.  I am also still curious to see if tweaking some
> setting on some automated building program will do that too.  So, my
> original question remains: are automated building programs better than
> humans?  Any human?
>
> I therefore declare the John Henry Challenge still open.
>
>
> But yes, improving the phases can tip the balance too, and the accuracy
> of the anomalous differences will ultimately affect the accuracy of the
> phases, and so on.  This is a much broader challenge.  And I think the
> best way to frame it is with the question:
> "How low can the anomalous signal be before any conceivable approach fails?"
> and perhaps:
> "What is the best procedure to use for weak anomalous signal?"
>
>   For those who are interested in joining George, Pavol, Raj and others
> in this new challenge, the full spectrum of "difficulty" from trivial
> (100% Se incorporation) to a complete waste of time (0% Se, 100% S) is here:
> http://bl831.als.lbl.gov/~jamesh/challenge/occ_scan/
>
> The "impossible.mtz" for the John Henry Map Interpretation Challenge was
> derived from "frac0.79.mtz" and "possible.mtz" from "frac0.78.mtz".
> These simulated 31% and 32% Se incorporation into Met side chains
> (respectively).  It has now been shown that both of these can be solved
> automatically if you do the phasing right. But what about frac0.80.mtz?
> Or frac0.90.mtz ?  At least on this one "coordinate" of Se
> incorporation, the prowess of a particular approach can be given a
> "score".  For example, a "score" of 0.78 means that the indicated
> procedure could solve the frac0.78.mtz dataset, but not the frac0.79.mtz
> dataset.
>
> Based on the reports I have gotten back so far, the "difficulty score"
> lineup is:
>
> score  method
> 0.86   xds, xscale, right sites, crank2 (Pavol Skubak)
> 0.78   xds, xscale, right sites, mlphare, dm, phenix.autobuild using 20
> models (James Holton)
> 0.75   xds, xscale, right sites, mlphare, dm, buccaneer/refmac/dm (James
> Holton)
> 0.71   xds, xscale, right sites, mlphare, dm, ARP/wARP 7.3 (James Holton)
> 0.51   xds, xscale, right sites, mlphare, dm, ARP/wARP 6.1.1 (James Holton)
>
> Note that all of these attempts "cheated" on the sites.  Finding the
> sites seems to be harder than solving the structure once you've got
> them.  That lineup is:
>
> score  method
> 0.82   cheating: xds, xscale, right phases, anomalous difference Fourier
> (James Holton)
> 0.79   xds, xscale, shelxc/d/e 3.5A NTRY=10000 (George Sheldrick)
> 0.74   xds, autorickshaw (Santosh Panjikar)
> 0.65    xds, xscale, phenix.hyss --search=full (James Holton)
> 0.60   xds, xscale, shelxc/d with NTRY=100 (James Holton)
>
> Where again the "score" is the dataset where the heavy atom site
> constellation found is close enough to the "right" one to move forward.
> This transition, like the model-building one, is remarkably sharp,
> particularly if you let each step run for a lot of cycles.  The graph
> for model-building is here:
> http://bl831.als.lbl.gov/~jamesh/challenge/build_CC_vs_frac.png
> Note how the final map quality is pretty much independent of the initial
> map quality, up to the point where it all goes wrong.  I think this
> again is an example of the solution needing to be at least "half right"
> before it can be improved.  But perhaps someone can prove me wrong on
> that one?
>
> For those who want the unmerged data, I have all the XDS_ASCII.HKL files
> here:
> http://bl831.als.lbl.gov/~jamesh/challenge/occ_scan/XDS_ASCII.tgz
>
> If you'd like to go all the way back to the images, you can get them
> from here:
> http://bl831.als.lbl.gov/~jamesh/workshop2/
> the "badsignal" dataset is what produced frac1.00.mtz, and "goodsignal"
> produced frac0.00.mtz.  You can generate anything in between using the
> provided img_mix.com script.
>
>
> Oh, and when it comes to how useful it is to spend "weeks" building
> manually into a bad map, well I suppose that does indeed depend on what
> alternatives you have and on the science you are trying to do.  I agree
> that it is always better to have better data, but if you spend too much
> time trying to improve your crystals and waiting for your next beam
> time, then somebody else who IS willing to build into dodgy maps will
> probably do the science for you and publish it first.  So, I think in a
> world of competitive grant renewals it really is critically important to
> know at what point it actually is "impossible" to solve the structure,
> as opposed to a situation where trying some new procedure (or
> collaborator) might be the way to go.  I'd like to be able to answer
> that question for my users, and that's why I'm doing this.
>
> -James Holton
> MAD Scientist
>
>
> On 1/13/2013 12:11 PM, jens Preben Morth wrote:
>> I agree with Tassos, and btw think that this crystallographer, should
>> be able to go back into the lab and optimize the present crystal
>> conditions to get better crystals. In particularly, when he or she
>> realize that the scientific question they set out to investigate
>> cannot be answered, by analyzing the final structure, with the
>> available data quality.
>> Preben
>>
>>
>> On 1/13/13 8:52 PM, Anastassis Perrakis wrote:
>>>> I think the real challenge (and one that makes for an excellent
>>>> macromolecular crystallographer) is how well one can interpret a map
>>>> with poor phases.
>>> Let me disagree ... An excellent macromolecular crystallographer, is
>>> one that given some crystals can derive the best strategy to collect
>>> data,
>>> process the data optimally, derive phases using all available
>>> information, build a model and refine it in such a way that it best
>>> explains both data
>>> and geometrical expectations, and do these as efficiently as possible.
>>>
>>> Efficiency may suggest using one automated suite or another - or
>>> indeed may best be achieved by manual labor - be it in the map or in
>>> data
>>> collection strategy or refinement or another step: and here I am
>>> ignoring the art of transforming
>>> hair-needle-crystalline-like-dingbits to a diffracting crystal.
>>>
>>> One that can interpret a map with poor phases can be either a genius
>>> in 3d orientation - or a not necessarily too intelligent nor
>>> experienced but determined student
>>> that can drink and breathe this map for a few weeks in a row until a
>>> solution is in place. Neither would make an excellent macromolecular
>>> crystallographer by necessity.
>>>
>>> Tassos
>

--
Prof. George M. Sheldrick FRS
Dept. Structural Chemistry,
University of Goettingen,
Tammannstr. 4,
D37077 Goettingen, Germany
Tel. +49-551-39-3021 or -3068
Fax. +49-551-39-22582

Top of Message | Previous Page | Permalink

JiscMail Tools


RSS Feeds and Sharing


Advanced Options


Archives

April 2024
March 2024
February 2024
January 2024
December 2023
November 2023
October 2023
September 2023
August 2023
July 2023
June 2023
May 2023
April 2023
March 2023
February 2023
January 2023
December 2022
November 2022
October 2022
September 2022
August 2022
July 2022
June 2022
May 2022
April 2022
March 2022
February 2022
January 2022
December 2021
November 2021
October 2021
September 2021
August 2021
July 2021
June 2021
May 2021
April 2021
March 2021
February 2021
January 2021
December 2020
November 2020
October 2020
September 2020
August 2020
July 2020
June 2020
May 2020
April 2020
March 2020
February 2020
January 2020
December 2019
November 2019
October 2019
September 2019
August 2019
July 2019
June 2019
May 2019
April 2019
March 2019
February 2019
January 2019
December 2018
November 2018
October 2018
September 2018
August 2018
July 2018
June 2018
May 2018
April 2018
March 2018
February 2018
January 2018
December 2017
November 2017
October 2017
September 2017
August 2017
July 2017
June 2017
May 2017
April 2017
March 2017
February 2017
January 2017
December 2016
November 2016
October 2016
September 2016
August 2016
July 2016
June 2016
May 2016
April 2016
March 2016
February 2016
January 2016
December 2015
November 2015
October 2015
September 2015
August 2015
July 2015
June 2015
May 2015
April 2015
March 2015
February 2015
January 2015
December 2014
November 2014
October 2014
September 2014
August 2014
July 2014
June 2014
May 2014
April 2014
March 2014
February 2014
January 2014
December 2013
November 2013
October 2013
September 2013
August 2013
July 2013
June 2013
May 2013
April 2013
March 2013
February 2013
January 2013
December 2012
November 2012
October 2012
September 2012
August 2012
July 2012
June 2012
May 2012
April 2012
March 2012
February 2012
January 2012
December 2011
November 2011
October 2011
September 2011
August 2011
July 2011
June 2011
May 2011
April 2011
March 2011
February 2011
January 2011
December 2010
November 2010
October 2010
September 2010
August 2010
July 2010
June 2010
May 2010
April 2010
March 2010
February 2010
January 2010
December 2009
November 2009
October 2009
September 2009
August 2009
July 2009
June 2009
May 2009
April 2009
March 2009
February 2009
January 2009
December 2008
November 2008
October 2008
September 2008
August 2008
July 2008
June 2008
May 2008
April 2008
March 2008
February 2008
January 2008
December 2007
November 2007
October 2007
September 2007
August 2007
July 2007
June 2007
May 2007
April 2007
March 2007
February 2007
January 2007


JiscMail is a Jisc service.

View our service policies at https://www.jiscmail.ac.uk/policyandsecurity/ and Jisc's privacy policy at https://www.jisc.ac.uk/website/privacy-notice

For help and support help@jisc.ac.uk

Secured by F-Secure Anti-Virus CataList Email List Search Powered by the LISTSERV Email List Manager