ISa: Difference between revisions

Jump to navigation Jump to search
284 bytes added ,  9 January 2013
no edit summary
m (moved CORRECT to ISa: seems more appropriate)
No edit summary
Line 7: Line 7:
This number is called <math>{I/Sigma(I)}^{asymptotic}</math> ([Diederichs, Acta Cryst. (2010). D66, 733-740 http://dx.doi.org/10.1107/S0907444910014836])
This number is called <math>{I/Sigma(I)}^{asymptotic}</math> ([Diederichs, Acta Cryst. (2010). D66, 733-740 http://dx.doi.org/10.1107/S0907444910014836])


What is that number? Scaling procedures (like the ones used in XDS, SCALA, SCALEPACK and DSCALEAVERAGE) scale (or rather, inflate) the variances of individual observations such that they match the experimental spread of symmetry-related observations. To this end, two contributions to the variance of a reflection are added: the first component is random error, and the other component is systematic error. The two values a and b appearing in the formula v(I)=a*(v0(I)+b*I^2) are printed out by CORRECT. a scales the random error component, a*b scales the systematic error component. For strong and well-measured reflections, the variance is dominated by the systematic error a*b*I^2 that is introduced by any beam /spindle / detector /cryo or other instability or malfunction. For weak reflections, a*v0(I), the variance from counting statistics, dominates.  
What is that number? Scaling procedures (like the ones used in XDS, SCALA, SCALEPACK and DSCALEAVERAGE) scale (or rather, inflate) the variances of individual observations such that they match the experimental spread of symmetry-related observations. To this end, two contributions to the variance v(I) of a reflection are considered: the first component is random error, and the other component is systematic error. The two values a and b appearing in the variance-scaling formula v(I)=a*(v0(I)+b* <math>{I}^2</math>) are printed out by CORRECT. a scales the random error component, a*b scales the systematic error component. For strong and well-measured reflections, the variance is dominated by the systematic error a*b* <math>{I}^2</math> that is introduced by any beam /spindle / detector /cryo or other instability or malfunction. For weak reflections, a*v0(I), the variance from counting statistics, dominates.  


=== Versions of XDS before May 10, 2010 ===
Versions of XDS since May 10, 2010 print out <math>{I/Sigma(I)}^{asymptotic}</math> = <math>I/\sqrt(a*b)</math> as "ISa". ISa is the I/sigma of an infinitely strong reflection. If there were no systematic error, ISa would be infinite. In the presence of systematic error, ISa is finite and is the upper limit of I/sigma of any observation in your dataset.  
A Unix command to obtain <math>{I/Sigma(I)}^{asymptotic}</math> from CORRECT.LP is
awk '/a *b *I/{getline;print ($1*($2+4e-4))^-0.5}' CORRECT.LP


The command just finds the line " a         b             INPUT DATA SET" in [[CORRECT.LP]], grabs the values of "a" and "b" from the next line, and prints out 1/sqrt(a*(b+0.0004)).  
As you can see from the formula, low values of a and b are ''good'' in the sense that a high upper limit of I/sigma(I) results. If e.g. the crystal is badly split or broken, or reflections are too close on the detector, or the data reduction is not good (wrong parameters), then the values of a and b are elevated.


The 0.0004 stems from the fact that the INTEGRATE step does its own adjustment of the variances, and the two adjustments (in INTEGRATE and CORRECT) have to be combined.
If your crystal is good, then a and b will reflect the quality of the other components of the experimental setup (e.g. beamline stability).  
 
=== Versions of XDS since May 10, 2010 ===
 
Newer versions print out <math>{I/Sigma(I)}^{asymptotic}</math>  as "ISa".
 
As you can see from the formula, low values of a and b are ''good'' in the sense that a high upper limit of I/sigma(I) results. If e.g. the crystal is badly split or broken, or reflections are too close on the detector, or the data reduction is not good (wrong parameters), then the values of a and b are elevated.


If your crystal is good (and no matter ''how'' good your crystal is!), then a and b will reflect the quality of the other components of the experimental setup (e.g. beamline stability).  
ISa is well suited to judge the quality of the experimental setup, because its value does not depend on random error, whereas the low-resolution <math>R_{meas}</math> does, and is thus influenced by crystal size and exposure. If you see a high value of the the low-resolution <math>R_{meas}</math>, you don't know if it is high because the crystal diffracted weakly, or because the beamline was broken. Conversely, a low value of ISa indicates that something is broken, no matter how small the crystal is or how weakly it was exposed.


== Practical considerations ==
== Practical considerations ==
Line 31: Line 23:
I have also seen a value around 40 for Z. Dauter's 0.98A Proteinase K (2ID8) sulfur-SAD data from J. Holton's APS/22-ID beamline, and recently even higher values were obtained at the SLS, beamline X06SA, with a Pilatus detector.
I have also seen a value around 40 for Z. Dauter's 0.98A Proteinase K (2ID8) sulfur-SAD data from J. Holton's APS/22-ID beamline, and recently even higher values were obtained at the SLS, beamline X06SA, with a Pilatus detector.


On the other hand, I have sometimes obtained values less than 10 with good test crystals. It is always good to discuss this with the people who are responsible for the beamline. They might know what is broken, or might be able to find out what went wrong.
On the other hand, I have sometimes obtained values less than 10 with good test crystals, clearly indicating strong systematic errors. It is always good to discuss this with the people who are responsible for the beamline. They might know what is broken, or might be able to find out what went wrong.


A low <math>{I/Sigma(I)}^{asymptotic}</math> may be compensated by high multiplicity, at the expense of radiation damage. Conversely, high multiplicity is not needed to solve a structure, if the data have a high <math>{I/Sigma(I)}^{asymptotic}</math>.  
A low <math>{I/Sigma(I)}^{asymptotic}</math> may be compensated by high multiplicity, at the expense of radiation damage. Conversely, high multiplicity is not needed to solve a structure, if the data have a high <math>{I/Sigma(I)}^{asymptotic}</math>.  
For molecular replacement and refinement, a high value of <math>{I/Sigma(I)}^{asymptotic}</math> is not strictly needed (but the maps are better with better data!).
For molecular replacement and refinement, a high value of <math>{I/Sigma(I)}^{asymptotic}</math> is not strictly needed (but the maps are better with better data!).
2,652

edits

Cookies help us deliver our services. By using our services, you agree to our use of cookies.

Navigation menu