Type IIP Supernova Progenitors. III. Blue to Red Supergiant Ratio in Low-metallicity Models with Convective Overshoot (Dataset)

<p>MESA input and output files associated with the published journal article Wagle et al. (2020; doi:10.3847/1538-4357/ab8bd5). We used MESA version r-10398 and MESA SDK version 20180822 to run these models.</p> <p>The &quot;MESA_inputs.tar.gz&quot; file contains work directories for initial mass of 13 solar mass and several overshoot parameter (f) values as listed in Table 2 of the published article. The models can be run directly from each working directory (&quot;f_*&quot;) by making (./mk) and then running MESA (./rn), after instantiating MESA SDK. The run-script (&quot;rn&quot;) is modified to start a MESA run from the pre-main-sequence (preMS) stage through core-collapse (CC) stage, if the LOGS and photos directories are absent. Otherwise, it restarts MESA from the latest &quot;photo&quot; binary file saved in the photos directory (that is, it assumes that the previous run was interrupted and restarts the run. So, to start a fresh run delete the &quot;LOGS&quot; and &quot;photos&quot; directories.) Each working directory has &quot;run_star_extras.f&quot; file which is modified to save the compactness parameters, mu_4, M_4 as extra history columns, as well as, to implement additional temporal resolution constraints as explained in section 2.2 of the article. Any other combination of mass and f-value from Table 2 of the article can be run by changing initial_mass in &quot;inlist_control&quot; file, and overshoot values in &quot;inlist_f*&quot; file.</p> <p>Each &quot;*M_z0.006_f_*.tar.xz&quot; file has a &quot;LOGS&quot; directory that contains corresponding &quot;history.data&quot;, &quot;profile.data&quot; at core-collapse (CC) stage and saved model (&quot;*.mod&quot;) at CC stage for each mass and f-value combination from Table 2 of the paper. (Note: Please copy the tar.xz files for each mass in a separate folder before decompressing them, in order to avoid overwriting the folders with the same f-values.) The LOGS directory also contains a folder &quot;png_plots&quot; that has saved &quot;.png&quot; files generated by &quot;inlist_pgstar&quot;. These files can be used to generate stellar evolution movies using the &quot;images_to_movie.sh&quot; script available in the MESA SDK.</p> <p>&nbsp;</p>