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

<p>1D FLASH simulations with STIR, for alpha_lambda = 1.23, 1.25, and 1.27.&nbsp; Run with SFHo EOS, M1 with 12 energy groups.</p> <p>For more information on these simulations, see Warren, Couch, O&#39;Connor, &amp; Morozova (arXiv:1912.03328) and Couch, Warren, &amp; O&#39;Connor (2020).</p> <p>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.&nbsp; The columns are: progenitor mass [M_sun], fit coefficient A, fit coefficient B, fit coefficient C, and the R^2 of the fit.</p>