Kilonova emission from GW230529 and mass gap neutron star-black hole mergers

Data release associated with Kilonova emission from GW230529 and mass gap neutron star-black hole mergers, 2025, https://doi.org/10.48550/arXiv.2409.10651 Data Includes: kilonova simulations for the BNSs-BNSw, NSBHs-BBHw, NSBHs-NSBHw posteriors studied in the article, for different EOS kilonova simulation for the LVK O5 simulations for BNS and mass-gap NSBH mergers studied in the article, for different EOS inj_final.json is made after applying the following cuts in the original injection.json file simulated from list_*.dat luminosity distance: < 600 Mpc primary mass: < 6 M⊙ seconday mass: < 2.069 (for softer EOS), < 2.436 (for fiducial EOS), < 2.641 (for stiffer EOS) log₁₀(dynamical mass) and log₁₀(wind ejecta mass) > 10⁻⁴ M⊙ list_*_final.dat has the same cuts applied in 3.1, 3.2, 3.3 to make the analysis consistent.