Speaker
Miriam Biehle
Description
Core-collapse supernovae are exploding massive stars and the next Galactic event will be one of the most interesting astronomical events of the century. In recent paper (Phys.Rev.D 107 (2023) 8, 083017), the authors developed an algorithm for assessing the presence of standing accretion shock instability (SASI) in simulated gravitational waves in a core-collapse supernova, the so-called SASI-meter. In this poster we discuss the implementation of an online module to coherent WaveBurst high significance events with the purpose of assessing the presence of SASI. We discuss the computational times, receiver operating characteristic curves and results on noise only events.
Primary authors
Alejandro Casallas Lagos
(Faculty of Physics, Warsaw University)
Carlos Quintero
Claudia Moreno
Manuel Morales
Marek Szczepanczyk
(University of Warsaw)
Michele Zanolin
(Embry-Riddle Aeronautical University, Prescott)
Miriam Biehle
Vincente Serra
