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franciscovillaescusa committed Apr 26, 2024
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Expand Up @@ -61,7 +61,13 @@ The video below shows an example of a CAMELS-Magneticum simulation:
Swift-EAGLE
~~~~~~~~~~~

The simulations in the Swift-EAGLE suite have been run with the smoothed particle hydrodynamics and gravity code `Swift <https://arxiv.org/abs/2305.13380>`__. Swift is a parallel, open-source, versatile and modular code, with a range of hydrodynamics solvers, gravity solvers, and sub-grid models for galaxy formation (see `Swift website <https://swift.strw.leidenuniv.nl/>`__). In this suite we use the `SPHENIX <https://academic.oup.com/mnras/article/511/2/2367/6423434?login=true>`__ flavour of SPH, coupled with a modified version of the Evolution and Assembly of GaLaxies and their Environments (`EAGLE <https://virgo.dur.ac.uk/2014/11/11/EAGLE/index.html>`__) subgrid model for galaxy formation and evolution (see `Schaye et al. 2015 <https://academic.oup.com/mnras/article/446/1/521/1316115?login=true>`__ and `Crain et al. 2015 <https://academic.oup.com/mnras/article/450/2/1937/984366?login=true>`__). This includes element-by-element radiative cooling and heating rates from `Ploeckinger & Schaye 2020 <https://academic.oup.com/mnras/article/497/4/4857/5876367?login=true>`__, stellar evolution and enrichment from `Wiersma et al. 2009 <https://academic.oup.com/mnras/article/399/2/574/1059162?login=true>`__, and single thermal-mode feedback from massive stars and accreting AGN (see `Schaye & Dalla Vecchia <https://academic.oup.com/mnras/article/383/3/1210/1037943>`__, `Booth & Schaye 2009 <https://academic.oup.com/mnras/article/398/1/53/1092579?login=true>`__, `Rosas-Guevara et al. 2015 <https://academic.oup.com/mnras/article/454/1/1038/1143767?login=true>`__).
The simulations in the Swift-EAGLE suite have been run with the smoothed particle hydrodynamics and gravity code `Swift <https://arxiv.org/abs/2305.13380>`__. Swift is a parallel, open-source, versatile and modular code, with a range of hydrodynamics solvers, gravity solvers, and sub-grid models for galaxy formation (see `Swift website <https://swift.strw.leidenuniv.nl/>`__). In this suite we use the `SPHENIX <https://academic.oup.com/mnras/article/511/2/2367/6423434?login=true>`__ flavour of SPH, coupled with a modified version of the Evolution and Assembly of GaLaxies and their Environments (`EAGLE <https://virgo.dur.ac.uk/2014/11/11/EAGLE/index.html>`__) subgrid model for galaxy formation and evolution (see `Schaye et al. 2015 <https://academic.oup.com/mnras/article/446/1/521/1316115?login=true>`__ and `Crain et al. 2015 <https://academic.oup.com/mnras/article/450/2/1937/984366?login=true>`__). This includes element-by-element radiative cooling and heating rates from `Ploeckinger & Schaye 2020 <https://academic.oup.com/mnras/article/497/4/4857/5876367?login=true>`__, star formation (`Schaye & Dalla Vecchia 2008 <https://ui.adsabs.harvard.edu/abs/2008MNRAS.383.1210S/abstract>`__), stellar evolution and enrichment from `Wiersma et al. 2009 <https://academic.oup.com/mnras/article/399/2/574/1059162?login=true>`__, and single thermal-mode feedback from massive stars and accreting AGN (see `Dalla Vecchia & Schaye 2012 <https://ui.adsabs.harvard.edu/abs/2012MNRAS.426..140D/abstract>`__, `Booth & Schaye 2009 <https://academic.oup.com/mnras/article/398/1/53/1092579?login=true>`__, `Rosas-Guevara et al. 2015 <https://academic.oup.com/mnras/article/454/1/1038/1143767?login=true>`__).

.. raw:: html

<iframe width="560" height="315" src="https://www.youtube.com/embed/XDpBT6JwRAE?si=9-crxJZT31CEKei_" title="YouTube video player" frameborder="0" allow="accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share" referrerpolicy="strict-origin-when-cross-origin" allowfullscreen></iframe>
<br><br>



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