The grid compiles ~20000 spectra of six prominent UV resonant lines resulting from radiative transfer through idealised galactic wind models and contains 5760 different wind configurations. The winds correspond to spherical (expanding or static) thick shells extending from the inner radius Rin to the outer radius Rout.

A full description of the radiative transfer simulations, the wind models, and the grid of spectra is given in Garel et al. (2024).