DOI: 10.48436/mvrkc-dz146
title: Transformer Network trained on Simulated X-ray photoelectron spectroscopy data for organic and inorganic compounds

description: Dataset Description

This data repository provides the underlying data and neural network training scripts associated with the manuscript titled "A Transformer Network for High-Throughput Material Characterisation with X-ray Photoelectron Spectroscopy" by Simperl and Werner. 

All data files are released under the Creative Commons Attribution 4.0 International (CC-BY) license, while all code files are distributed under the MIT license.

The repository contains simulated X-ray photoelectron spectroscopy (XPS) spectra stored as hdf5 files in the zipped (h5_files.zip) folder, which was generated using the software developed by the authors. The NIST Standard Reference Database 100 – Simulation of Electron Spectra for Surface Analysis (SESSA) is freely available at https://www.nist.gov/srd/nist-standard-reference-database-100.  

The neural network architecture is implemented using the PyTorch Lightning framework and is fully available within the attached materials as Transformer_SimulatedSpectra.py contained in the python_scripts.zip. 

The trained model and the list of materials for the train, test and validation sets are contained in the models.zip folder.

The repository contains all the data necessary to replot the figures from the manuscript. These data are available in the form of .csv files or .h5 files for the spectra. In addition, the repository also contains a Python script (Plot_Data_Manuscript.ipynb) which is contained in the python_scripts.zip file.

Context and methodology

The dataset and accompanying Python code files included in this repository were used to train a transformer-based neural network capable of directly inferring chemical concentrations from simulated survey X-ray photoelectron spectroscopy (XPS) spectra of bulk compounds.

The spectral dataset provided here represents the raw output from the SESSA software (version 2.2.2), prior to the normalization procedure described in the associated manuscript. This step of normalisation is of paramount importance for the effective training of the neural network.

The repository contains the Python scripts utilised to execute the spectral simulations and the neural network training on the Vienna Scientific Cluster (VSC5). In order to obtain guidance on the proper configuration of the Command Line Interface (CLI) tools required for SESSA, users are advised to consult the official SESSA manual, which is available at the following address: https://nvlpubs.nist.gov/nistpubs/NSRDS/NIST.NSRDS.100-2024.pdf.

To run the neural network training we provided the requirements_nn_training.txt file that contains all the necessary python packages and version numbers. All other python scripts can be run locally with the python libraries listed in requirements_data_analysis.txt. 

Data details

HDF5 (in zip folder): As described in the manuscript, we simulate X-ray photoelectron spectra for each of the 7,587 inorganic [1] and organic [2] materials in our dataset. To reflect realistic experimental conditions, each simulated spectrum was augmented by systematically varying parameters such as peak width, peak shift, and peak type—all configurable within the SESSA software—as well as by applying statistical Poisson noise to simulate varying signal-to-noise ratios. These modifications account for experimentally observed and material-specific spectral broadening, peak shifts, and detector-induced noise. Each material is represented by an individual HDF5 (.h5) file, named according to its chemical formula and mass density (in g/cm³). For example, the file for SiO2 with a density of 2.196 gcm-3 is named SiO2_2.196.h5. For more complex chemical formulas, such as Co(ClO4)2 with a density of 3.33 gcm-3, the file is named Co_ClO4_2_3.33.h5. Within each HDF5 file, the metadata for each spectrum is stored alongside a fixed energy axis and the corresponding intensity values. The spectral data are organized hierarchically by augmentation parameters in the following directory structure, e.g. for Ac_10.0.h5 we have SNR_0/WIDTH_0.3/SHIFT_-3.0/PEAK_gauss/Ac_10.0/. These files can be easily inspected with H5Web in Visual Studio Code or using h5py in Python or any other h5 interpretable program.

Session Files: The .ses files are SESSA specific input files that can be directly loaded into SESSA to specify certain input parameters for the initilization (ini), the geometry (geo) and the simulation parameters (sim_para) and are required by the python script Simulation_Script_VSC_json.py to run the simulation on the cluster.

Json Files: The two json files (MaterialsListVSC_gauss.json, MaterialsListVSC_lorentz.json) are used as the input files to the Python script Simulation_Script_VSC_json.py. These files contain all the material specific information for the SESSA simulation.

csv files: The csv files are used to generate the plots from the manuscript described in the section "Plotting Scripts".

npz files: The two .npz files (element_counts.npz, single_elements.npz) are python arrays that are needed by the Transformer_SimulatedSpectra.py script and contain the number of each single element in the dataset and an array of each single element present, respectively.

SESSA Simulation Script

There is one python file that sets the communication with SESSA:



Simulation_Script_VSC_json.py: This script is the heart of the simulation as it controls the communication through the CLI with SESSA using the specified input paramters in the .json and .ses files together with external functions specified in VSC_function.py


Technical Details

Simulation_Script_VSC_json.py: This script uses the functions of the VSC_function.py script (therefore needs to be placed in the same directory as this script) and can be called with the following command:

 python3 Simulation_Script_VSC_json.py MaterialsListVSC_gauss.json 0

It simulates the spectrum for the material at index 0 in the .json file and with the corresponding parameters specified in the .json file.

It is important that before running this script the following paths need to be specified:



sessa_path: The path to their SESSA installation in sessa_path and the path to their session files in

folder_path: The path to their .ses files. In this directory an output folder will be generated where all the output files, including the simulated spectra, are written to.   


To run SESSA on a computing cluster it is important to have a working Xvfb (virtual frame buffer) or a similar tool available to which any graphical output from SESSA can be written to. 

Neural Network Training Script

Before running the training script it is important to normalize the data such that the squared integral of the spectrum is 1 (as described in the manuscript) and shown in the code: normalize_spectra.py 

For the neural network training we use the Transformer_SimulatedSpectra.py where the external functions used are specified in external_functions.py. This script contains the full description of the neural network architecture, the hyperparameter tuning and the Wandb logging. 

In the models.zip folder the fully trained network final_trained_model.ckpt presented in the manuscript is available as well as the list of training, validation and testing materials (test_materials_list.pt, train_materials_list.pt, val_materials_list.pt) where the corresponding spectra are extracted from the hdf5 files. The file types .ckpt and .pt can be read in by using the pytorch specific load functions in Python, e.g.

torch.load(train_materials_list)

Technical Details

normalize_spectra.py: To run this script properly it is important to set up a python environment with the necessary libraries specified in the requirements_data_analysis.txt file. Then it can be called with

python3 normalize_spectra.py

where it is important to specify the path to the .h5 files containing the unnormalized spectra.

Transformer_SimulatedSpectra.py: To run this script properly on the cluster it is important to set up a python environment with the necessary libraries specified in the requirements_nn_training.txt file. This script also relies on external_functions.py, single_elements.npz and element_counts.npz (that should be placed in the same directory as the python script) file. This is important for creating the datasets for training, validation and testing and ensures that all the single elements appear in the testing set. You can call this script (on the cluster) within a slurm script to start the GPU training. 

python3 Transformer_SimulatedSpectra.py

It is important that before running this script the following paths need to be specified:



data_path: General path where all the data is stored

neural_network_data: The location where you keep your normalized hdf5 files

wandb_api_key: The api key to use wandb

ray_tesults: The location where you want to save your tuning results

checkpoints: The location where you want to save your ray checkpoints

saved_model_path: The location where you want to save your final models


The following parameters can be set to true or false:



ray_tune_activate: This activates the hyperparameter tuning

full_training_activate: This activates the full training where the hyperparameters need to be set manually 

continue_training: If we want to train the same model for more epochs. In that case, it is important to set the data to the same train, validation and testing materials as the initially training when importing the dataloaders at the beginning. 


Plotting Scripts

With the script Plot_Data_Manuscript.ipynb we can plot all the figures in the manuscript using the .csv files and the normalized .h5 files. In order to use this code it is necessary to define the path variables at the beginning of the script accordingly to where the data (the .csv and .h5 files) are saved locally. The necessary Python libraries can be installed from requirements_data_analysis.txt.   

Figure Data

Figure 2: The data for figure 2 showing the chemical distribution in the dataset can directly be plotted with the file elements_counts_periodic_table.csv

Figure 3: The data for figure 3 showing the survey spectrum of SiO2 and the augmented data features for noise, shift and width can be extracted from SiO2_2.196.h5. 

Figure 5: The data for the validation and training loss curve can be retrieved from the metrics.csv file that contains the data for the training and validation loss. 

Figure 6: The polar plot indicating the distriubtion of the mean absolute error for the chemical concentration for each correctly predicted material can be generated from the tp_elements_only_metrics.csv.

Figure 7: The confusion matrix can be produced from the confusion_matrix.csv containing for each element the values for true negative (tn), false negative (fn), false positive (fp) and true positive (tp).

Figure 8a and 8c: The two example spectra can be produced from the hdf5 files for CoCr2O4_5.14.h5 and Pb2SiO4_7.6.h5 both for snr:10, width: 0.6eV, shift: -3.0eV and peak type: Lorentz.

Figure 8b and 8d: The predicted and true concentrations for each element can be extracted from the concentration_prediction_CoCr2O4.csv and concentration_prediction_Pb2SiO4.csv, respectively.