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Core-collapse supernovae are one of the most energetic events in the universe($10^{46} J$). When a massive star (M $>$ 8 M$_{\odot}$) ignites its lastfusion stage where silicon fusion makes iron, its end is then very close.Basically, the core of the star falls inwardly and the gravitational energy isthen released in a supernova explosion. The basic picture of this explosion wasconfirmed by the few neutrinos detected from the SN1987a supernova atKamiokande, IMB and Baksan detectors. However, there are many details that arestill unknown. Since then, a large detector network has grown with bettercapabilities. Nowadays, in the case of a supernova explosion in our galaxy, theinformation that we would acquire would allow us to learn much more about theseenergetic events and constrain our models. Here, I present a brief summary ofthis network with special emphasis in SuperK-Gd (the upgraded Super-Kamiokandedetector with efficient neutron tagging).

Supernovae in SuperK-Gd and other experiments