Speaker
Dr
Francesco Salemi
(University of Rome, "La Sapienza" and INFN Roma)
Description
We present a case study on archival open GW data to test new methodological improvements in targeted searches for gravitational-wave transients associated with core-collapse supernovae.
The study involves core-collapse supernovae optically observed within 30 Mpc during the third observing run of Advanced LIGO and Advanced Virgo. We report the detection efficiency and the distance range for various models of gravitational-wave emissions.
Primary author
Dr
Francesco Salemi
(University of Rome, "La Sapienza" and INFN Roma)
