Constraining properties of the next nearby core-collapse supernova with multi-messenger signals: multi-messenger signals

<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 the multi-messenger data from the STIR simulations.&nbsp; The filename indicates the turbulent mixing parameter a and progenitor mass m of the simulation.&nbsp; Columns are time [s], shock radius [cm], explosion energy [ergs], electron neutrino mean energy [MeV], electron neutrino rms energy [MeV], electron neutrino luminosity [10^51 ergs/s], electron antineutrino mean energy [MeV], electron antineutrino rms energy [MeV], electron antineutrino luminosity [10^51 ergs/s], x neutrino mean energy [MeV], x neutrino rms energy [MeV], x neutrino luminosity [10^51 ergs/s], gravitational wave frequency from eigenmode analysis of the protoneutron star structure [Hz].&nbsp; Note that the x neutrino luminosity is for <strong>one</strong> neutrino flavor - to get the total mu/tau neutrino and antineutrino luminosities requires multiplying this number by 4.</p> <p>v1.1 - removed unnecessary duplicate files</p> <p>v1.2&nbsp;- upload failed. &nbsp;Obsolete.</p> <p>v1.3&nbsp;- packaging alpha values as separate tar files for easy download.</p>