Constraining properties of the next nearby core-collapse supernova with multi-messenger signals: gravitational wave frequency fits

1D FLASH simulations with STIR, for alpha_lambda = 1.23, 1.25, and 1.27.  Run with SFHo EOS, M1 with 12 energy groups.

For more information on these simulations, see Warren, Couch, O'Connor, & Morozova (arXiv:1912.03328) and Couch, Warren, & O'Connor (2020).

Includes fit to the gravitational wave peak frequency versus time post-bounce, for a functional fit of the form f = A*sqrt(t) + B*t + C, where the frequency f is in Hz and the time t is in seconds.  The columns are: progenitor mass [M_sun], fit coefficient A, fit coefficient B, fit coefficient C, and the R^2 of the fit.