Cross-correlation of the data with the Fe I model. Shown are the results for the 1-UT transit (top), and those for the 4-UT transit (bottom). The first column shows the contour plots of the temporal variation of the cross-correlation, with a dashed line to show the expected planetary velocity; the colorbar scale is in ppm. The second column is the K_p versus velocity map after summing the cross-correlations for different K_p, with colorbar scale in S/N. Green dashed lines are centered on the expected planetary position. The third column shows the final S/N of the detection, with the performed Gaussian fit in blue, as calculated at the theoretical K_p value.