Here we provide equation of state (EOS) tables for astrophysical simulations explored in [1]:

• LS220^† (Table)
• m^*_0.8 (Table)
• m^*_Shen (Table)
• (m^*,K)_Shen (Table)
• (m^*,E_sym)_Shen (Table)
• (m^*,K,E_sym)_Shen (Table)
• SkShen (Table)

See the publication for more details about the names and input parameters. When using these table please refer to our work [1].

The EOS tables are created using the open-source code SROEOS from [2,3]. As in [2], we refer to the LS220 generated EOS with the SROEOS code as LS220^†. For the construction of EOS tables, see also [4].

• [1] H. Yasin, S. Schäfer, A. Arcones, and A. Schwenk, Phys. Rev. Lett. 124, 092701 (2020)
• [2] A. S. Schneider, L. F. Roberts, and C. D. Ott, Phys. Rev. C 96, 065802 (2017)
• [3] A. S. Schneider, L. F. Roberts, and C. D. Ott, https://bitbucket.org/andschn/sroeos
• [4] E. O’Connor and C. D. Ott, https://sntheory.org/equationofstate

For questions and feedback please contact:

• Almudena Arcones
• Achim Schwenk

Neutrino-driven trajectories based on a steady-state model:

• Here trajectories corresponding to the nucleosynthesis groups described in J. Bliss et al., ApJ 855, 135 (2018).
• Here 36 trajectories used for (α,n) sensitivity study of J. Bliss et al., Phys. Rev. C 101, 055807 (2020).

If you use these trajectories, please cite: J. Bliss et al., ApJ 855, 135 (2018) and J. Bliss et al., Phys. Rev. C 101, 055807 (2020).

Representative trajectories for the MR-SN model 35OC-Rs (M. Obergaulinger & M. Á. Aloy, MNRAS, 469, L43, 2017) and their nucleosynthesis (M. Reichert et al., MNRAS, 501, 5733, 2021) can be found here.

If you use the trajectories and/or nucleosynthesis output please cite following papers:

• M. Obergaulinger & M. Á. Aloy, MNRAS, 469, L43 (2017)
• M. Reichert et al., MNRAS, 501, 5733 (2021)