Table 2: Influence of the presence of emission lines at the level L[OII] on the estimates of photometric redshifts and stellar masses. q_0.5 refers to the median value, while q_0.9 refers to the 90% quantile.
L[OII] $\Delta~z$ $\Delta\log~(M/M_{\odot})$

[erg s^-1] q_0.5 q_0.9 - q_0.5 q_0.5 q_0.9-q_0.5

<38 -0.003 0.09 -0.03 0.45

40 -0.004 0.09 -0.04 0.45

42 0.008 0.20 -0.04 0.76

44 -0.027 0.34 -0.68 0.64

**Table 2:** Influence of the presence of emission lines at the level L[OII] on the estimates of photometric redshifts and stellar masses. q_0.5 refers to the median value, while q_0.9 refers to the 90% quantile.
L[OII]	$\Delta~z$	$\Delta\log~(M/M_{\odot})$
[erg s^-1]	q_0.5	q_0.9 - q_0.5	q_0.5	q_0.9-q_0.5
<38	-0.003	0.09	-0.03	0.45
40	-0.004	0.09	-0.04	0.45
42	0.008	0.20	-0.04	0.76
44	-0.027	0.34	-0.68	0.64

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