Same as Fig. 3, but for the confirmed interlopers of the F200W dropout selection. The best-fit templates of objects COSMOS_31168, COSMOS_35731, COSMOS_76919, and UDS_56824 shown in red were obtained with ZPHOT after fixing the redshift at the spectroscopic values (black dashed line in the P(z) panels). The E(B − V) range for COSMOS_35731, COSMOS_76919, and UDS_56824 has been constrained within the 1σ range indicated by the Balmer decrement.