Bayesian Model Averaging (BMA) fit for TOI-2015. The top panel shows the transmission curves of the filters considered, and the bottom panel displays the residuals. The observed SpeX SXD spectrum is shown in blue, while the black line represents the BT-Settl CIFIST synthetic spectrum using the BMA-derived stellar parameters, as shown in Table 1. The fluxes related to the photometry are shown by colors: orange for Gaia DR3, red for 2MASS, and purple for WISE.