Testing dark energy models with a new sample ofstrong-lensing systems

Inspired by a new compilation of strong lensing systems (SLS), which consist of 205 points in the redshift range $0.0625 1$ or high velocity dispersion $\sigma > 276$ km s$^{-1}$). Model selection criteria show that using SLS, the $\omega$-cold dark matter and Chevallier-Polarski-Linder models are preferred in different regions of the data.