Asteroseismically Inferred Ages of 132,000 Red Giants with TESS

Table 2: Table of our collected data and computed values including spectroscopic, Gaia-derived, and asteroseismic results, as well as derived masses and ages (see text for details). This table is available in its entirety in machine-readable form in the online article and on Zenodo. Table 3: Table of our collected data and computed values including spectroscopic, Gaia-derived, and asteroseismic results, as well as derived masses and ages (see text for details) assuming our alternate, model-based mass loss scheme for red clump stars. This table is available in its entirety in machine-readable form in the online article and on Zenodo. Inlist_common_AT: Inlist_common file used for solar calibrated MESA modeling. Please view documentation for complete process on MESA modelling. COMPLETEGRID: All MESA model tracks from our grid. We advise that 5 models at low mass/ high metallicity did not run, so 619 out of 624 models successfully ran. These can be analyzed using the mesa_reader function in python.