| Xsight |


This user guide contains the following lessons:
Isomorphous replacement
Lesson 20:Richardson diagrams

> mkdir $HOME/crystal_info2. Copy the crystals and projects, and the cvccp files, from the $XSIGHTTUTORIAL directory to the $CRYSTALDATA directory:
> cp $XSIGHTTUTORIAL/crystals $HOME/crystal_info > cp $XSIGHTTUTORIAL/projects $HOME/crystal_info > cp $XSIGHTTUTORIAL/cvccp $HOME/crystal_info3. Make sure that your crystals and projects files are writeable.
> chmod +w $HOME/crystal_info/crystals > chmod +w $HOME/crystal_info/projects4. Edit your .cshrc file to include two environment variables:
setenv CRYSTALDATA $HOME/crystal_info5. Log out and log back in.
setenv CRYSTAL cvccp
Each time you start a new project or create a new crystal, the information will be updated in the $CRYSTALDATA directory. The cvccp crystal file is used for many of the tutorials. You will want to change your $CRYSTAL environment variable, depending on which crystal you most frequently use.
Do not do your work in the $CRYSTALDATA directory. This directory is only for storing information about crystals and projects. Define your working directory through the Utilities/Project command in the Xsight interface.

In Lesson 1:Merging native and derivative data, you learn to convert processed data into the .fin file format. You then merge and scale a native data set with an Au derivative. Finally, the lesson takes you through the different statistical plots that you can generate to evaluate the quality of the derivative.
In Lesson 2:Finding heavy atom sites for the first derivative, you calculate and contour a difference Patterson map for the Au derivative. You then locate the two major Au sites using an automated search method. You verify these positions against the difference Patterson map. Finally, you refine the Au sites and calculate SIR phases.
In Lesson 3:Adding a second derivative, you merge and scale an Ir derivative with the native data set. You then calculate a cross-Fourier using the SIR phases from the Au derivative and the isomorphous differences between the Ir data and the native data. From this map you locate an Ir site in the Ir derivative crystal. Finally, you refine the Ir site and calculate the MIR phases using the Au and Ir positions.
This lesson uses the following commands, accessed from the Xsight module:
Lesson 1: Merging native and derivative data
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Xsight module
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Utilities
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Data_Control
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MIR
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Project
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Import_Data
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Merge_Data
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Statistics
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The Scenario: You have just collected a putative derivative data set of C. vinosum Cytochrome c' (cvccp) and you want to merge it with an existing native data set. You then want to calculate statistics that will indicate whether you have been successful in producing a derivative.
In order to run this tutorial (and the other associated MIR tutorials), you must set up a directory which contains the ccp_raxis_au1.dat, ccp_raxis_ir1.dat, and ccp_raxis_n1.dat files, that is, two derivative data sets and a native data set.
Enter the following commands, in the order shown, at the command prompt:
> mkdir tutorial_mir > cd tutorial_mir > cp $XSIGHTTUTORIAL/*raxis* . |
The >> symbol allows you to append lines to an existing file. Once you type the cat command, all typed entries in the textport are appended to the crystals file. For this lesson, you simply want to add the cvccp crystal to the file and exit from the cat append mode. Be sure not to type anything else in the textport while you are in the cat command mode.
Invoke the Insight II software.
At the system prompt issue the command:
> insightIIand press <Enter>. |
Wait a few moments while Insight II loads.
The dialog box disappears automatically.
This lesson assumes that you have your processed reflection files in a format other than the .fin reflection format. In particular, it assumes you are starting with three reflection files in the standard R-AXIS II format. In this lesson, you use the native data set and one of the derivative data sets. The second derivative data set is used in Lesson 3:Adding a second derivative.
First, you will convert the native data set to the .fin file format.
5. Converting the Au derivative data set
Now you will convert the Au derivative data set to a .fin format.
6. Merging the native and Au derivative data files
This displays the Xmerge window
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In the Xmerge menu, set Scaling Type to Anisotropic. Click Scale to begin the merging procedure. |
After a few moments, two graphs are generated at the end of the merging procedure: merging R-factor versus resolution and the average |Fp-Fph| versus resolution. These two graphs help you evaluate your derivative data.
| Select Quit, then click Yes to confirm. |
This is an optional step in which you may replot the comparisons between the native and derivative data.
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Select the MIR/Statistics command. Set Input_File to ccp_n1.ccp_au1.fin. Select Execute. |
The Xfinstat window now appears.
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In the Xfinstat menu toggle on R-factor vs. resolution and |F1-F2| vs. resolution. Click Graph it. |
| Select Quit, then click Yes to confirm. |
| To quit Insight II, type quit on at the command line, and press <Enter>. |
This lesson uses the following commands, accessed from the Xsight module:
Lesson 2: Finding heavy atom sites for the first derivative
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Xsight module
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Utility
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MIR
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Project
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Calc_Fourier
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Contour_Map_3D
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Find_Heavy_Atoms
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Calc_Phases
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You need to have run lesson 1 before doing this tutorial lesson.
If you have just finished Lesson 1:Merging native and derivative data, and you are still running Insight II, you can skip to step 3.
If you have run Lesson 1:Merging native and derivative data, but need to restart Insight II carry out step 2.
At the system prompt issue the command:
> insightIIand press <Enter>. |
Insight II takes a few moments to load.
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Go to the Xsight pulldown by clicking the MSI logo and selecting Xsight from the list that appears. Select the Utilities/Project command and enter mir as the Project_Name parameter. Select Execute. |
3. Calculating a difference Patterson map
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Select the MIR/Calc_Fourier command. Enter ccp_n1.ccp_au1.fin for the Phase_File parameter. Make sure that ccp_n1.ccp_au1.map is entered as the Map_File parameter. Select Execute. |
Since you are calculating a Patterson map, you need to generate the Fourier coefficients from the observed differences between the native and derivative data sets. Your input file to the Fourier program therefore comes from a .fin file (structure factor amplitude file) rather than a .phs file (phase angle file).
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Set the following parameter values in the Xfft menu: Map Type: Fo*Fo (Patterson) Resolution filter: 999.999 to: 5.0 Outlier Filter: differences> 100 |
The label Patterson map from h,k,l,fp,s(fp),fm,s(fm) should now be loaded next to the Phase File Type button.
| Click Calculate to create the difference Patterson map. |
The calculation takes a few moments. The message FFT finished tells you when it is completed.
| Click Quit when you are finished, then click Yes to confirm. |
5. Display the difference Patterson map
After a few moments the three-dimensional representation of the Patterson map appears.
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Set Contour_Operation to Quit_Command. Select Execute. |
These input parameters set up a two-site heavy atom search using data to 5 Å resolution over a unique volume in the crystal cell. The Au sites that are located will be written to a solution file called ccp_n1.ccp_au1.sol.
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Make sure that Heavy_Operation is set to Run. MIR_Run_Mode should be set to Run_Now. Select Execute. |
| When the Notifier message appears to inform you that the background job is complete, select Continue. |
7. Checking the heavy atom solution
The graphical display of the difference Patterson map will appear. A table reports the positions of the two Au atoms that were located by the heavy atom search program. A pickable table will report the interatomic vectors that should correspond to peaks in the difference Patterson map.
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Set Contour_Operation to Quit_Command. Select Execute. |
8. Starting the heavy atom refinement and phase calculation program
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Select the MIR/Calc_Phases command. Select ccp_n1.ccp_au1.sol for the Solution_File parameter. Enter ccp_n1.ccp_au1.phs for the Phase_Output parameter. Select Execute. |
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Use MB1 to select the derivative AU. Click Edit. |
The Xheavy Derivative Editor will appear.
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In the Xheavy Derivative Editor menu change the high Resolution parameter from 1.0 to 5.0. Select Apply. |
| In the main Xheavy menu select Apply. |
The two Au sites are refined by the correlation method. This calculation takes about half a minute on an SGI R4400. When five refinement cycles are completed the correlation coefficient is reported as 0.8214.
| In the main Xheavy menu select Apply again |
After three refinement cycles the refinement converges with a correlation coefficient of 0.8386.
| Click the Save Derivative button, then click Overwrite at the prompt. |
You can now calculate SIR phases based on the refined heavy atom sites.
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Using MB3, click and hold the arrow button next to Method. Select Calculate Protein Phases and release MB3. Click Apply. |
The calculated phases are now stored in the Output Phases file (ccp_n1.ccp_au1.phs).
| Select Quit, then click Yes to confirm that you want to exit. |
| To quit Insight II, type quit on the command line, and press <Enter>. Press <Enter> again at the next prompt. |
This lesson uses the following commands, accessed from the Xsight modules:
Lesson 3: Adding a second derivative
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Xsight module
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Utilities
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Data_Control
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MIR
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Project
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Import_Data
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Merge_Data
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Calc_Fourier
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Contour_Map_3D
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Calc_Phases
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Merge_Phases
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You need to have run lessons 1 and 2 before doing this tutorial.
If you have just finished Lesson 1:Merging native and derivative data, and you are still running Insight II, you can skip to step 3.
If you have previously run Lesson 2:Finding heavy atom sites for the first derivative but have left Insight II go to step 2.
At the system prompt issue the command:
> insightIIand press <Enter>. |
Wait a few moments while Insight II loads.
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Go to the Xsight pulldown by clicking the MSI logo and selecting Xsight from the list that appears. Select the Utilities/Project command and enter mir as the Project_Name parameter. Select Execute. |
4. Merging the native and Ir derivative data files
This displays the Xmerge window.
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In the Xmerge menu, set Scaling Type to Anisotropic. Click Scale to begin the merging procedure. |
Two graphs are generated at the end of the merging procedure: one merging R factor versus resolution, and the other showing average |Fp-Fph| versus resolution. These two graphs help you evaluate your derivative data.
| Select Quit in the Xmerge menu, then click Yes to confirm. |
5. Merging the Au phases with the Ir and native .fin file
| Toggle on the Swap f1 and f2 (isomorphous Fourier) check box and click Merge. |
The creation of the new .phs file will only take a few seconds.
| Select Quit, then click Yes to confirm. |
6. Calculating a cross-Fourier map
7. Calculating the Fourier using the Xfft menu
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Set the following parameter values in the Xfft menu: Map Type: mFo-Fc Resolution filter: 999.999 to: 5.0 Outlier Filter: differences> 100 |
You switched the position of the native and Ir data when you created the .phs file in the last step. That is why an Fo-Fc map will generate a positive peak for an Ir site.
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Click the Calculate button to create the cross-Fourier map. Select Quit when you are finished, then click Yes to confirm. |
8. Display the cross-difference Fourier map
Now you want to use the cross-Fourier map to look for significant peaks that indicate Ir sites.
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Make sure the Site_Edit_Operation is set to Peak_Search. Use the value-aid to change the Scattering_Element to IR. Change the Site_Peak_Threshold value to 8.0. Select Execute. |
The unique Ir site will be identified by a yellow sphere and the sites related by the crystallographic symmetry are marked as purple spheres. The site co-ordinates are also be reported in a table.
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Set Site_Edit_Operation to Write_Solution_File. Enter ccp_n1.ccp_ir1.sol in the Out_Solution_File parameter block. Select Execute. Set Contour_Operation to Quit_Command. Select Execute. |
9. Starting the heavy atom refinement and phase calculation program
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Select the MIR/Calc_Phases command. Use the value-aid to enter ccp_n1.ccp_ir1.sol as the Solution_File parameter. Enter ccp_mir.phs as the Phase_File parameter. Select Execute. |
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Use MB1 to select the derivative IR. Click Edit. |
The Xheavy Derivative Editor appears.
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In the DataFile field enter ccp_n1.ccp_ir1.fin. Change the high Resolution parameter from 1.00 to 5.00. Select Apply. |
| Select Apply in the main Xheavy menu. |
The Ir site is refined by the correlation method.
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In the Xheavy Derivative Editor menu change the high Resolution parameter from 5.00 to 3.00. Select Apply. In the main Xheavy menu select Apply. |
You will now save the refined Ir parameters.
| Click the Save Derivative button, then click Overwrite at the prompt. |
10. Loading the Au derivative file and calculating MIR phases
Now you load the Au derivative.
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In the main Xheavy menu enter the filename, ccp_n1.ccp_au1.sol, in the Derivative File parameter field. Click the Load Derivative button. |
| Select the AU derivative from the derivative list in the main Xheavy menu using MB1, then click Edit. |
Now you will use the Xheavy Derivative Editor menu.
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In the Xheavy Derivative Editor menu change the high Resolution parameter from 5.00 to 3.00. Click Apply. |
| In the main Xheavy menu, click Apply. |
This step takes about a minute. At the end of the refinement the correlation coefficient is reported as 0.7742.
| Click the Save Derivative button, then click Overwrite at the prompt. |
You can now calculate MIR phases based on the refined heavy atom sites.
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Use MB3 to click and hold the Method arrow button. Select the Calculate Protein Phases button and release MB3. Click Apply. |
After about one minute, the calculation of the protein phases will be completed. Because of the limited amount of heavy atom derivative information this phase set is relatively poor, with a figure of merit of 0.497. The calculated phases are stored in the Output Phases file, ccp_mir.phs.
| Select Quit in the Xheavy menu, then click Yes to confirm that you want to exit. |
If you now wish to, quit Insight II.
| To quit Insight II, type quit on the command line, and press <Enter>. Press <Enter> again at the prompt. |