Cu Auger Line Curve Fitting CasaXPS 2.0.1

 

Problem: Given an unknown spectrum, determine the relative contributions from Cu2O, CuO and Metallic Cu to the unknown spectrum.

 

Four spectra are displayed in Figure 1, three of which are believed to contribute to the fourth spectrum. The three know spectra can be used to construct line-shapes forming the basis for a nonlinear optimisation, the results of which estimate the relative proportions on these know spectra to the unknown data.

 

Figure 1: Cu Auger lines. Data supplied by: Institute of Physics, Tampere University of Technology, Finland.

 

The following steps are required to perform the analysis:

 

Construct background subtracted line-shapes from the data.

 

 

For each of the spectra required by the peak-fit, add an appropriate background and create a new VAMAS block in the data file consisting of the background subtracted data.

 

  • Add a background using the Regions property page on the Quantification Parameters dialog window (Options menu “Quantify …”).
  • Subtract the background from the data using the Test Data property page on the Spectrum Processing dialog window (Options menu “Processing …”).
  • Copy the processed data to a new VAMAS block by right-clicking over the right-hand-side of the Experiment Frame and selecting the Data Only tick-box Figure 3.
  • Adjust the names of the new data using the Edit Info toolbar button  Figure 4. The Block Ids for the new line-shape VAMAS block must start with a % character (Figure 5).

 

 

Figure 2: Preprocess the basis data using the Background Subtract option.

 

Figure 3: Copy the processed line-shape to a new VAMAS block.

 

Figure 4: Edit the line-shape VAMAS block and ensure the Block Id starts with a % character.

 

Figure 5: Right-hand-side of the Experiment Frame following creation and renaming of the Block Id, Element and Experimental Variable fields in Figure 4

 

Define a peak model on the unknown spectrum in terms of the new line-shapes.

 

  • Using each of the original basis spectra fit the new line-shape derived from that data to the basis spectra. This provides initial starting points for the peak parameters ultimately used to create the model for the unknown spectrum. Create a component on the basis spectrum and enter the Block Id for the appropriate line-shape into the Line-Shape field on the Components property page (see Figure 6 for an example).
  • Fix the fwhm parameters derived from fitting to the original basis data and also limit the position parameters to a small interval around the value determined for the basis data. Note the fwhm parameter should be close to unity owing to the requirement that the line-shape from data should not be deformed away from the shape of the basis data.
  • Copy and Paste the components from the basis spectra onto the unknown spectrum. Manual adjust the components to guide the auto-fitting and press the Fit Components pushbutton on the Components property page.

 

Figure 6: Model defined from data. Note the Block Id of the line-shapes is entered into the Line-shape field.

 

Figure 7: A possible fit to the unknown spectrum using the line-shapes taken from known spectral forms.