[3] Other research topics include detector development for a neutrinoless double beta decay search and the creation of an extreme low temperature diamond calorimeter.
The CsI(Tl) scintillating crystal used has a high light yield and is affordable for large mass.
In 2008, the 12 crystal array with 103.4 kg mass was completed and ran until December 2012 for a detector upgrade replacing the PMTs.
The KIMS and DM-Ice groups collaborated to make a new detector consisting of an array of NaI(Tl) scintillating crystals to confirm or refute the DAMA/LIBRA results.
[9] This rejection applies only to WIMPs with one of the 18 tested masses, exhibiting spin-independent interactions with sodium or iodine nucleons, within the context of a standard dark matter halo model.