Operating System: CentOS Linux 7 (Core) with MESA version- r12115.

This dataset contains selected data used to generate the main figures in this work, based on MESA binary evolution calculations for the formation of ELM WDs. 

The data are organized by metallicity: z = 0.02 and 0.001, where z is the metallicity of the donor.
Within each metallicity folder, subdirectories are labeled by k = 0, 0.05, 0.10, 0.15, 0.20, and 0.25, where k represents the fraction of AML carried away through the L2 point.

Each file is named as Mdonor_MCO_k, where Mdonor is the initial donor mass (in solar masses) and MCO is the initial CO white dwarf mass (in solar masses).
Each file contains the results of models with the same initial donor mass, initial CO white dwarf mass and metallicity, but different initial orbital periods. Each row corresponds to the system properties at the end of the evolution for a given model.
These files correspond to the end of the calculation or just before the onset of the second mass transfer phase due to GW.

Files ending with "_1" (Mdonor_MCO_k_1) represent the moment of Roche-lobe detachment.
