Comparison of our retrieved C/O and |$^{12}$|C/|$^{13}$|C ratio from our combined retrieval of all four nights to other close-in planets, companions, and isolated targets. These were obtained from Line et al. (2021), Finnerty et al. (2023), Gandhi et al. (2023b), Xuan et al. (2024c), Costes et al. (2024), Regt et al. (2024), González Picos et al. (2024), Xuan et al. (2024a), Zhang et al. (2024), and Mulder et al. (2024). The error bars of the sub-stellar objects are colour coded by their age, with lighter shades being the youngest and darker shades being the oldest. We also show the solar C/O ratio (Asplund et al. 2021) in the left panel with the dotted line. In the right panel, we show the Solar system |$^{12}$|C/|$^{13}$|C value with the dotted line and the ISM value and 1|$\sigma$| uncertainty with the dashed line and shaded region, respectively (Wilson 1999; Milam et al. 2005).