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https://github.com/edoaltamura/rotational-ksz-macsis

Repository for suppelementary material from my publication on the rotational kinetic SZ effect in MACSIS
https://github.com/edoaltamura/rotational-ksz-macsis

cosmology data-analysis galaxy-clusters high-performance-computing hydrodynamics

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Repository for suppelementary material from my publication on the rotational kinetic SZ effect in MACSIS

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![Rotational kSZ](https://img.shields.io/badge/ArXiv-2302.07936-red)
![MIT License](https://img.shields.io/github/license/edoaltamura/entropy-core-problem)
![PyPI - Python Version](https://img.shields.io/pypi/pyversions/3)
![DiRAC](https://img.shields.io/badge/DiRAC-COSMA7-green)
![Stargazers](https://img.shields.io/github/stars/edoaltamura/macsis-cosmosim)
![Issues](https://img.shields.io/github/issues/edoaltamura/macsis-cosmosim)

# Rotational kinetic SZ effect in MACSIS clusters

#### Data products from the study by [Altamura et al. (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230207936A/abstract)
This repository contains suppelementary material from my publications on the rkSZ effect, and a collection of analysis tools for the MACSIS cosmological simulations. MACSIS is a suite of zoom-in simulations of galaxy clusters run with `Gadget-3` and the BAHAMAS sub-grid model. An overview of the most massive MACSIS cluster is shown below, with the kSZ maps in the insets at the bottom.

![Overview of the MACSIS 0 cluster](img/map_with_vectors_0.png)

## 📚 Citing
When using data products or code from this repository, and the results or insights derived from it, we recommend citing [Altamura et al. (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230207936A/abstract) using the [bibliography styles provided in ADS](https://ui.adsabs.harvard.edu/abs/2023arXiv230207936A/exportcitation).