ISa: Difference between revisions

488 bytes added ,  29 May 2010
no edit summary
No edit summary
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 The variance of a reflection comes from random errors, and from systematic influences The values a and b appear in the formula v(I)=a*(v0(I)+b*I^2) which is used by CORRECT to adjust the variances of the intensities, to match their experimental spread. For strong and well-measured reflections, the variance is dominated by the systematic error that is introduced by any beam /spindle / detector /cryo or other instability or malfunction. For weak reflections, v0(I), the variance from counting statistics, dominates. The value for v(I) that the formula gives, will be higher than v'(I)=a*b*I^2 by an amount a*v0(I). Therefore, I/sigma(I) = I/sqrt(v(I)) will be lower than I/sqrt(v'(I)) = 1/sqrt(a*b) which is what the Unix command prints out.  
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.  


=== Versions of XDS before May 10, 2010 ===
=== Versions of XDS before May 10, 2010 ===
A Unix command to obtain it from CORRECT.LP is  
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
  awk '/a *b *I/{getline;print ($1*($2+4e-4))^-0.5}' CORRECT.LP


It 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)).  
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)).  


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.
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.
Line 19: Line 19:
=== Versions of XDS since May 10, 2010 ===
=== Versions of XDS since May 10, 2010 ===


Newer versions print out 1/sqrt(a*(b+0.0004)) as "ISa".  
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.
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.
Line 26: Line 26:


== Practical considerations ==
== Practical considerations ==
In practice, both crystal quality and beamline quality limit the value of the asymptotic I/SigmaI . A good crystal (even with elevated mosaicity and medium resolution) should give a high value of the asymptotic I/SigmaI on a good beamline.  
In practice, both crystal quality and beamline quality limit the value of <math>{I/Sigma(I)}^{asymptotic}</math> . A good crystal (even with elevated mosaicity and medium resolution) should give a high value on a good beamline.
I have seen values around 20 for good crystals that still allowed my to solve a MAD structure, but that required high multiplicity of observations. Values around 30 allowed me to solve a sulfur-SAD structure at medium resolution (diffraction to 2.3 A, anomalous signal to 3 A).  
I have seen values around 15-20 for good crystals that still allowed my to solve a MAD structure, but that required high multiplicity of observations. Values around 30 allowed me to solve a sulfur-SAD structure at medium resolution (diffraction to 2.3 A, anomalous signal to 3 A).  
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. 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>.
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!).
2,684

edits