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1. Super Kamiokande

   Linked via "neutrino energy profile"

   $$\text{n} + \text{Gd} \rightarrow {^{160}\text{Gd}}^* \rightarrow {^{160}\text{Gd}} + \gamma1 + \gamma2$$
   This capability is crucial for distinguishing between neutrino interactions (which produce a prompt Cherenkov light flash) and the subsequent, delayed light signal from neutron capture. This is particularly vital for improving the sensitivity to very low-energy electron recoils and for enhancing background rejection in [supernova neutrino burst detection](/entries…