SEVN tables from the paper "The impact of envelope binding energies on the merger rate density of binary compact objects" by Sgalletta et al. 2026

The repository contains the tables used in the SEVN simulations in the paper "The impact of envelope binding energies on the merger rate density of binary compact objects" by Sgalletta et al., 2026. Tables description The tables have been generated with the PARSEV v2.0 set of tracks described in Costa et al. 2025. SEVNtracks_parsec_ov05_AGB_ebind.zip: set of tables for the hydrogen-rich stars. Metallicity (Z) range: 1e-11 - 0.03 Mass range: 2-600 Msun (Z>0.0001), 2-2000 Msun (Z<=0.0001) SEVNtracks_parsec_pureHe36_ebind.zip: set of tables for the pure-helium stars. Metallicity range: 0.0001 - 0.05 Mass range: 0.36-350 Msun The tracks contain the compulsory properties for SEVN and the information on the lambda parameters, evaluated from the envelope binding energies, saved in the files lambda.dat. The tables have been generated with Trackcruncher, available at the link https://gitlab.com/sevncodes/trackcruncher (commit 78157fb4).