Inlist and Best Fit Model Files for "Precise Asteroseismic Ages for the Helmi Streams"

MESA (r22.05.1) and GYRE (version 7.1) inlist files used in the work described in "Precise Asteroseismic Ages for the Helmi Streams". The three subdirectories are provided in the archive: 1) The directory called "HD175305" contains the different MESA inlist files for different evolutionary periods (inlist_to_ZAMS=pre main sequence, inlist_to_middle=main sequence and subgiant phase, and inlist_to_end=red giant branch) of the stellar models calculated during our optimization procedure. The subfolder called HD175305_best_fit contains the model track and structure files associated with the best fit model we found for HD 175305. 2) The directory called "HD128279" contains the different MESA inlist files for different evolutionary periods (inlist_to_ZAMS=pre main sequence, inlist_to_middle=main sequence and subgiant phase, and inlist_to_end=red giant branch) of the stellar models calculated during our optimization procedure. The subfolder called HD128279_best_fit contains the model track and structure files associated with the best fit model we found for HD 128279. 3) The directory called "gyre_templates" contains the gyre inlists used to calculate the different radial, mixed-mode dipole, and quadrupole modes from the MESA profile files. Note that we did not use custom physics hooks in this modelling (default run_star_extras.f90 file).