Figure 9.
![Colour–magnitude diagram of $M_{W_{JH}}$ versus [WJH − H], plotted using our function ExoCMD_model. The following parameters were entered for the model: Teff = 1000–2500 K, log g = 2.3, 3.0, 4.0, and 5.0, SpT = G5, and [Fe/H] = 2. As before, points have been coloured according to C/O ratio in order to highlight the differences between carbon- and oxygen-rich atmospheres. Brown dwarfs are plotted in the background as grey diamonds.](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/mnras/499/1/10.1093_mnras_staa2350/1/staa2350fig9.jpeg?Expires=1749597126&Signature=4tGvN92jwPOTLDqfNtQAA5QgvmBL8JpiZHARwn8lLVQHSmkw4EJhu~L8JW7BHsVxHJLUVDhoRvi4H~MfL0jyMDnMX19-j~68y2jholEWUgaSu3ZXWvr3yEnvr2lebnK3pbEPjqKLkbnrg7m9AUTSstxDtYmm-f4~uPCPqPiM~vJyOJIQE1F1EzxXUFg8Ku~U1RYiMcdFz0MW5MWg0to5hZ~lBoHxX3vpLhCOlm2Z9R9zED0B8JfwixXWBi9cW23k9GMjtV35BnHvpBDhiT3kIaAB4jYGCJ4HVa6oD~B3AiSY77AwbS~IzH0ac4sTuj4gkqlc-8LGG1W85FnoPBIwBQ__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
Colour–magnitude diagram of |$M_{W_{JH}}$| versus [WJH − H], plotted using our function ExoCMD_model. The following parameters were entered for the model: Teff = 1000–2500 K, log g = 2.3, 3.0, 4.0, and 5.0, SpT = G5, and [Fe/H] = 2. As before, points have been coloured according to C/O ratio in order to highlight the differences between carbon- and oxygen-rich atmospheres. Brown dwarfs are plotted in the background as grey diamonds.
