correac/TangoSIDM_satellites

TangoSIDM: the effect of dark matter self-interactions on dwarf galaxies

Code and data repository for ...

Note

The repository contains:

• TangoSIDM data regarding Milky-Way type halos and their satellites in the TangoSIDM simulations suite. The large .hdf5 files in data/TangoSIDM/ are stored via Git Large File Storage. More information can be found in data/TangoSIDM/README.md.
• Gaia data for the Milky Way dwarf-spheroidal galaxies. More information can be found in data/Gaia/README.md.
• examples notebook to explore TangoSIDM data and reproduce the main results of the work. More information can be found in examples/README.md.

Citation

If you use this code and the data in your analysis, please use the following citations:

@article{TBD
  title={TangoSIDM: the effects of dark matter self-interactions on satellite gaalxies},
  author={Anau Montel, Noemi and Correa, Camila A},
  year={2024},
}

and

@article{Correa_2022,
   title={TangoSIDM: tantalizing models of self-interacting dark matter},
   volume={517},
   ISSN={1365-2966},
   url={http://dx.doi.org/10.1093/mnras/stac2830},
   DOI={10.1093/mnras/stac2830},
   number={2},
   journal={Monthly Notices of the Royal Astronomical Society},
   publisher={Oxford University Press (OUP)},
   author={Correa, Camila A and Schaller, Matthieu and Ploeckinger, Sylvia and Anau Montel, Noemi and Weniger, Christoph and Ando, Shin’ichiro},
   year={2022},
   month=oct, pages={3045–3063} }

If you use the data available in the data/Gaia/ folder, please make sure to cite the correct source as indicated in the data/Gaia/README.md file.