A bstractThe normal sulphospinel CuIr 2 S 4 exhibits a temperature-induced metal± insulator (M±I) transition around TM Iˆ230 K with a structural transformation. This T M I increases markedly with increasing pressure. It has been veri®ed that the 5d electrons of Ir ions at the B sites located at the Fermi surface play a signi®cant role for the strong correlated electron system. Conversely, CuTi2S4 remains metallic down to 4.2 K without any structural transformations. These two compounds have the same normal spinel structure, whereas the number of d electrons at the B sites are quite di erent. High-purity spinel-type Cu(Ir 1 ¡ x Ti x ) 2 S 4 specimens have been successfully synthesized. The value of the lattice constant a indicates a broad minimum around xˆ0:12, not obeying Vegard's law. We have systematically studied the structural transformation and electrical and magnetic properties of Cu(Ir1¡xTix † 2S4. A phase diagram between T M I and x will be provided for the Cu(Ir 1 ¡ x Ti x † 2 S 4 system. TM I varies drastically with x and disappears at around xˆ0:06. A novel relationship, namely a`mirror image e ect', between the value of residual resistivity and the magnitude of the electronic density of states, D … "F † , at the Fermi level, has been observed accurately. } 1. I ntroduction The metal±insulator (M±I) transition in CuIr 2 S 4 has been extensively investigated in the past decade (Furubayashi et al. ). The sulphospinel CuIr 2 S 4 has the normal spinel-type structure where Cu ions occupy the A (tetrahedral) sites and Ir ions occupy the B (octahedral) sites, as shown in ®gure 1. CuIr 2 S 4 exhibits the temperature-induce d M±I transition around T M Iˆ2 30 K with structural transformation , showing hysteresis on heating and cooling. The resistivity of CuIr 2 S 4 jumps discontinuousl y by nearly three orders of magnitude at T M I as indicated in ®gure 2. With decreasing temperature, the symmetry changes from cubic to tetragonal, accompanied by a change from high-temperatur e Pauli paramagnetism in the metallic state to weak diamagnetism due to the atomic core orbital in the insulating state. A detailed structure analysis of the insulating phase has been made (Oshima et al. 1999, Ishibashi et al. 2001, Oikawa et al. 2001, Sun et al. 2001, Radaelli et al. 2002. The temperature dependence of magnetic susceptibility