Heo, Jeong-EunJeong-EunHeoYoon, SoyoungSoyoungYoonLee, Dae-SubDae-SubLeeKong, In-taekIn-taekKongLee, Sang-HoonSang-HoonLeevan Putten, Maurice H. P. M.Maurice H. P. M.van PuttenDELLA VALLE, MassimoMassimoDELLA VALLE2020-05-122020-05-1220161384-1076http://hdl.handle.net/20.500.12386/24723Gravitational wave bursts in the formation of neutron stars and black holes in energetic core-collapse supernovae (CC-SNe) are of potential interest to LIGO-Virgo and KAGRA. Events nearby are readily discovered using moderately sized telescopes. CC-SNe are competitive with mergers of neutron stars and black holes, if the fraction producing an energetic output in gravitational waves exceeds about 1%. This opportunity motivates the design of a novel Sejong University Core-CollapsE Supernova Survey (SUCCESS), to provide triggers for follow-up searches for gravitational waves. It is based on the 76 cm Sejong university telescope (SUT) for weekly monitoring of nearby star-forming galaxies, i.e., M51, M81-M82 and blue dwarf galaxies from the unified nearby galaxy catalog with an expected yield of a few hundred per year. Optical light curves will be resolved for the true time-of-onset for probes of gravitational waves by broadband time-sliced matched filtering.STAMPAenArticle10.1016/j.newast.2015.06.0072-s2.0-84937053818000361776700003https://www.sciencedirect.com/science/article/pii/S13841076150007312016NewA...42...24HFIS/05 - ASTRONOMIA E ASTROFISICA