Row 1: the results of cross correlating our night 1 data with the Fe model. The location of the peak K_p and RV values are indicated by converging dotted white lines in each plot with a significant detection. For plots without a significant detection, the expected planetary signal location is indicated by nonconverging dotted white lines (i.e., RV = 0 km s⁻¹; K_p ∼ 176.5 km s⁻¹). The color bars indicate the significances of the maps, determined via dividing out the standard deviation away from the peak signal, calculated via a 3σ-clipped map (see Section 5.1). Row 2: the same as row one, but for night 2. Row 3: the same as row 1, but for nights 1 and 2 combined, with each night weighted by its respective average SNR. Surrounding plots labeled “both” are slices of the 2D K_p−RV maps at the peak K_p and peak RV for the blue (blue line), red (red line), and combined (black line) results. The dashed black lines represent the combined peak RV and K_p.