These EOS routines and tables are from O'Connor and Ott (2010), A New Spherically-Symmetric General Relativistic Hydrodynamics Code for Stellar Collapse to Neutron Stars and Black Holes, Class. Quant. Grav., 27 114103, 2010, and, of course, the original authors of the EOS. If you have any questions or have discovered a bug in our routines/tables, please e-mail Evan at or start an issue on the GitHub page for either the EOSmaker repo or the EOSdriver repo. Please note that the routines and tables provided here come with absolutely no warranty and we are unable to guarantee that we will be able to provide support or help if you run into problems integrating them with your simulation code. If you decide to use the provided EOS routines and data in published work, it is YOUR responsibility to check their physical correctness and consistency.

• Equation of state maker routines:
  Fortran 90 routines that allow you to read in original EOS tables (i.e. H. Shen et al. 2011 or G. Shen et al. 2011ab, or Hempel-like EOS) and construct an .h5 table compatible with EOSdriver. This is available via github at https://www.github.com/evanoconnor/EOSmaker
  
• Equation of state driver routines:
  Fortran 90 routines that allow you to read in our EOS tables and that contain various routines for interpolation and EOS inversion. This is available via github at https://www.github.com/evanoconnor/EOSdriver
  
• Equation of State Tables:
  We provide tables for the nuclear equations of state of Lattimer and Swesty (1991), H. Shen et al. (2011), G. Shen et al. (2011ab), and Hempel et al. (2012), Steiner et al. (2012), Banik et al. (2014). Details on the tables and how they were generated (with EOSmaker above) can be found in O'Connor and Ott, Class. Quant. Grav., 27 114103, 2010. The tables are provided in HDF5 format and are 200-500 MB in size and can be accessed most easily with EOSdriver.
  
  

We also make available a selection of EOSs from the SRO code. This code, documentation, and other information is available here: https://bitbucket.org/andschn/sroeos/src/master/. These EOS work with the EOSdriver routines mentioned above (although please see the caveats in section 7 of the SRO User Guide), there is also a C++ version here: https://bitbucket.org/zelmani/eosdrivercxx/src/master/. These 96 EOS are used in da Silva Schneider et al. (2019) (arXiv). They are broken down into four sets as detailed in the paper (see Table 1 in the paper). In each set the two parameters are varied +/- 0,1,2 sigma away from the reference value, this gives 25 EOS for each set. The 0 sigma EOS is common among all 4 sets, given 96 in total.