Cryogenic Artificial Intelligence Tools - A Python Package for the Data Analysis of Rare Event Search Experiments with Machine Learning.
Project description
Cait (Cryogenic Artificial Intelligence Tools) is a Python 3 software package for the machine learning based analysis of raw data from cryogenic dark matter experiments. It is tailored to the needs of the CRESST and COSINUS experiment, but applicable to other, similar data structures.
Documentation: https://cait.readthedocs.io/
Source Code: https://github.com/fewagner/cait
Bug Report: https://github.com/fewagner/cait/issues
Installation
Cait is hosted on the Python package index.
$ pip install cait
You can now import the library in Python, e.g.
import cait as ai
Version History
Master branch is on the latest release version and stable.
Previous versions are hosted on the accordingly named Git branch.
The Changelog starts with Version 1.0.
Version numbers follow the segmantic versioning guide (https://semver.org/).
Citations
If you use Cait in your research work, please reference the package accordingly.
Cait uses a number of Python packages. If you use methods that are based on those packages, please consider referencing them: h5py, numpy, matplotlib, scipy, numba, sklearn, uproot, torch, pytorch-lightning, plotly.
Cait has methods implemented that were used in prior research work. Please consider referencing them:
2020, F. Wagner, Machine Learning Methods for the Raw Data Analysis of cryogenic Dark Matter Experiments”, https://doi.org/10.34726/hss.2020.77322 (accessed on the 9.7.2021)
2019, D. Schmiedmayer, Calculation of dark-matter exclusions-limits using a maximum Likelihood approach, https://repositum.tuwien.at/handle/20.500.12708/5351 (accessed on the 9.7.2021)
2019, CRESST Collaboration et. al., First results from the CRESST-III low-mass dark matter program, doi 10.1103/PhysRevD.100.102002
2020, M. Stahlberg, Probing low-mass dark matter with CRESST-III : data analysis and first results, available via https://doi.org/10.34726/hss.2021.45935 (accessed on the 9.7.2021)
2019, M. Mancuso et. al., A method to define the energy threshold depending on noise level for rare event searches” (arXiv:1711.11459)
2018, N. Ferreiro Iachellini, Increasing the sensitivity to low mass dark matter in cresst-iii witha new daq and signal processing, doi 10.5282/edoc.23762
2016, F. Reindl, Exploring Light Dark Matter With CRESST-II Low-Threshold Detectors”, available via http://mediatum.ub.tum.de/?id=1294132 (accessed on the 9.7.2021)
1995, F. Pröbst et. al., Model for cryogenic particle detectors with superconducting phase transition thermometers, doi 10.1007/BF00753837
We want you …
… to contribute! We are always happy about any contributions to our software. To coordinate efforts, please get in touch with felix.wagner(at)oeaw.ac.at such that we can include your features in the upcoming release. If you have any troubles with the current release, please open an issue in the Bug Report.
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