Extrapolated bar fractions for different redshifts from this work. Based on Fig. 4, we display our cumulative distribution (dashed grey histogram) and normalise it by the observed bar fraction in the Local Universe in studies that consider both weak and strong bars (0.67; e.g. Eskridge et al. 2000; Menéndez-Delmestre et al. 2007; Marinova & Jogee 2007). With this, we derive the extrapolated bar fraction over time in our sample (green dots). Additionally, the shaded green region accounts for the systematic error in our bar age measurements of ${}_{-1.4}^{+1.8}\text{Gyr}$. With the grey error bars, we also display the likely ranges in the cumulative distribution considering this systematic error as well. We compare our results with the observed bar fraction from different works, finding a remarkable agreement with works that consider both weak and strong bars.