Atmospheric planetary signal obtained with the Fe I, Cr I, and Ti I templates (top, central, and bottom row, respectively). The left column shows the K_p-υ_sys bi-dimensional map, with the color bar encoding the significance of the detection. The cross in white dashes marks the position where the planetary signal is expected according to Table 1. The central (right) column shows the cut along the vertical (horizontal) direction on the map and corresponding to the peak detection, together with its Gaussian best fit (dashed blue line).