We have trained CNN models to predict RPS parameters (IGM density rho_igm and relative velocity v_rel) from 2D density and kinematic maps of disc galaxies undergoing RPS.
We provide a sample of images which can be used for testing our trained model.
pip install -r requirements.txt- Install pre-trained model.
python src/predict.py
Paper available at: http://arxiv.org/abs/2008.03460