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 Code developed by members of the Surrey astrophysics group: Code developed by members of the Surrey astrophysics group:
-  * [[https://​github.com/​mgieles/​limepy|LIMEPY]] (//Lowered Isothermal Model Explorer in PYthon//) A python base code to solve a general class of lowered isothermal model, including Michie (1963)/King (1966)and Wilson (1975), including radial anisotropy and multi-mass systems (Gieles & Zocchi ​in prep)+  * [[https://​github.com/​mgieles/​limepy|LIMEPY]] (//Lowered Isothermal Model Explorer in PYthon//) A python base code to solve a general class of lowered isothermal model, including Michie (1963)/King (1966)and Wilson (1975), including radial anisotropy and multi-mass systems (Gieles & Zocchi, [[http://​arxiv.org/​abs/​1508.02120|ArXiv 1508.02120]])
   * [[https://​github.com/​emacss/​emacss|EMACSS]] (//Evolve Me a Cluster of StarS//) A rapid clusters evolution code developed by Poul Alexander (Cambridge) and Mark Gieles. The accompanying papers can be found here: [[http://​adsabs.harvard.edu/​abs/​2012MNRAS.422.3415A|version 1]]; [[http://​adsabs.harvard.edu/​abs/​2014MNRAS.437..916G|version 2]]; [[http://​adsabs.harvard.edu/​abs/​2014MNRAS.442.1265A|version 3]].   * [[https://​github.com/​emacss/​emacss|EMACSS]] (//Evolve Me a Cluster of StarS//) A rapid clusters evolution code developed by Poul Alexander (Cambridge) and Mark Gieles. The accompanying papers can be found here: [[http://​adsabs.harvard.edu/​abs/​2012MNRAS.422.3415A|version 1]]; [[http://​adsabs.harvard.edu/​abs/​2014MNRAS.437..916G|version 2]]; [[http://​adsabs.harvard.edu/​abs/​2014MNRAS.442.1265A|version 3]].
   * [[http://​personal.ph.surrey.ac.uk/​~fr0005/​nbody6tt.php|NBODY6tt]] An adapted version of [[http://​www.ast.cam.ac.uk/​~sverre/​web/​pages/​nbody.htm|Aarseth'​s NBODY6]] (//NBODY6 Tidal Tensor//) Allows user defined external potentials to be applied to the cluster. Written by Florent Renaud (Surrey, formerly at Strassbourg and Saclay) and Mark Gieles (Surrey). ​ Method papers can be found [[http://​adsabs.harvard.edu/​abs/​2011MNRAS.418..759R|here   * [[http://​personal.ph.surrey.ac.uk/​~fr0005/​nbody6tt.php|NBODY6tt]] An adapted version of [[http://​www.ast.cam.ac.uk/​~sverre/​web/​pages/​nbody.htm|Aarseth'​s NBODY6]] (//NBODY6 Tidal Tensor//) Allows user defined external potentials to be applied to the cluster. Written by Florent Renaud (Surrey, formerly at Strassbourg and Saclay) and Mark Gieles (Surrey). ​ Method papers can be found [[http://​adsabs.harvard.edu/​abs/​2011MNRAS.418..759R|here
 ]] and this was applied to [[http://​adsabs.harvard.edu/​abs/​2013MNRAS.431L..83R|clusters in merging galaxies]] and [[http://​adsabs.harvard.edu/​abs/​2014arXiv1411.1069B|star clusters in dwarf galaxies accreting on the Milky Way]]. ]] and this was applied to [[http://​adsabs.harvard.edu/​abs/​2013MNRAS.431L..83R|clusters in merging galaxies]] and [[http://​adsabs.harvard.edu/​abs/​2014arXiv1411.1069B|star clusters in dwarf galaxies accreting on the Milky Way]].