language: | |
- en | |
library_name: tf-keras | |
license: wtfpl | |
pipeline_tag: image-segmentation | |
# *Cavity Detection Tool* (CADET) | |
[***CADET***](https://tomasplsek.github.io/CADET/) is a machine learning pipeline trained for identification of surface brightness depressions (so-called *X-ray cavities*) on noisy *Chandra* images of early-type galaxies and galaxy clusters. The pipeline consists of a convolutional neural network trained for producing pixel-wise cavity predictions and a DBSCAN clustering algorithm, which decomposes the predictions into individual cavities. The pipeline is further described in [Plšek et al. 2023](https://arxiv.org/abs/2304.05457). | |
 | |
## How to use | |
```python | |
from huggingface_hub import from_pretrained_keras | |
model = from_pretrained_keras("Plsek/CADET-v1") | |
y_pred = model.predict(X.reshape(1,128,128,1)) | |
``` | |
## How to cite | |
The ***CADET*** pipeline was originally developed as a part of my [diploma thesis](https://is.muni.cz/th/x68od/?lang=en) and was further described in [Plšek et al. 2023](https://arxiv.org/abs/2304.05457). If you use the ***CADET*** pipeline in your research, please cite the following paper: | |
``` | |
@misc{plšek2023cavity, | |
title={CAvity DEtection Tool (CADET): Pipeline for automatic detection of X-ray cavities in hot galactic and cluster atmospheres}, | |
author={Tomáš Plšek and Norbert Werner and Martin Topinka and Aurora Simionescu}, | |
year={2023}, | |
eprint={2304.05457}, | |
archivePrefix={arXiv}, | |
primaryClass={astro-ph.HE} | |
} | |
``` |