Since I joined the Super-Kamiokande (SK) collaboration in 2009, my main motivation has been the detection of core collapse supernova (ccSN) neutrinos. This includes those from all the past ccSNe, the diffuse supernova neutrino background (DSNB). Currently having the best world limit, some SK collaborators have been working on EGADS, a project to realise GADZOOKS!. By loading the SK water with gadolinium, we will be able to detect DSNB, our main motivation, and improve SN detection and other studies.