Posterior distributions obtained when removing the synthetic VLTI/GRAVITY data from the atmospheric fit. The input atmosphere is the same as case 1 (cf. Table 2), and as in Fig. 7 we also compare the results when applying CROCODILE to MRCCS data alone (orange), LRSP data (blue), and on both MRCCS+LRSP combined (green). However, this time the low-resolution spectroscopy only included synthetic VLT/SPHERE data in the Y – H bands. The input values are shown as dashed red lines.