Detailed spectroscopy following the $^{14}$C on $^{36}$S fusion-evaporation reaction

High-spin state in neutron-rich Sc isotopes were produced using the ${^36}$S($^{14}$C,$pnn\gamma$) reaction at 34-MeV at Florida State University(FSU). The FSU $\gamma$-array, which is a mix of both signal crystal and clover-style HPGe detectors, was used to detect the prompt $\gamma$-radiation. A silicon telescope placed at $0^\circ$ was used to detect and clearly identify charged particles released from the reaction. The level scheme for $^{47}$Sc has been extend, approaching the neutron separation energy. Natural alignment following the reaction has allowed angular distributions to be extracted. States with clear particle-hole configurations have been identified from proton$-\gamma-\gamma$ coincidences. The experimental results will be presented and discussed in light of recent shell-model calculations.