Table 7: Results of spectro-photometric fitting for sources with no AGN component. The five columns on the right contain the stellar masses of galaxies, their ongoing (within the last 10⁸ yr) star formation rate, two values of the intrinsic extinction, and the IR (8-1000 $\mu$ m restframe) luminosity produced by the ongoing starburst, estimated assuming an M 82-like template. The two $A_{\rm V}$ values are computed by averaging over the whole galaxy life and over the last 10⁸ yr (representing the amount of dust affecting the ongoing burst). In parenthesis the 3 $\sigma$ ranges derived from the exploration of the parameter space are reported.
ID Type Class z Mass $(\star)$ SFR(10⁸ yr) $A_{\rm V}$ (mean) $A_{\rm V}$ (10⁸ yr) L_IR

SWIRE phot. spec. spec. $[10^{11}~M_\odot]$ [ $M_\odot/\textrm{yr}]$ [mag] [mag] $[10^{11}~L_\odot]$

EN1_202261 P2 ELG 1.339 1.44 (1.41-2.36) 489 (171-741) 1.68 (1.29-1.73) 1.82 (1.71-1.88) 10.81 (8.48-12.84)

EN1_342445 P3L ELG 1.917 1.04 (0.91-1.84) 426 (268-480) 1.10 (0.57-1.17) 1.40 (0.96-1.49) 9.37 (6.89-12.81)

EN1_340451 P3 NLAGN 2.866 6.69 (6.12-7.29) 56.1 (29.6-106) 0.63 (0.41-0.76) 2.18 (1.43-2.32) 36.79 (25.45-50.58)

EN2_11091 P3L ELG 1.946 3.94 (2.37-4.20) 208 (197-575) 0.61 (0.29-0.89) 0.80 (0.71-1.82) 16.13 (10.58-20.94)

EN2_167372 P2L ELG 1.445 2.62 (2.08-2.77) 86.9 (25.4-192) 0.59 (0.07-0.93) 1.34 (0.35-1.80) 4.98 (0.96-12.77)

EN2_166134 P2 ELG 1.337 3.40 (3.05-3.86) 17.9 (9.90-200) 0.79 (0.50-0.89) 1.65 (1.20-2.02) 9.06 (5.82-12.41)

LH_572243 P2,X NLAGN 1.820 0.91 (0.85-0.92) 34.3 (27.7-91) 0.82 (0.79-0.90) 2.09 (1.99-2.28) 9.27 (9.04-10.51)

**Table 7:** Results of spectro-photometric fitting for sources with no AGN component. The five columns on the right contain the stellar masses of galaxies, their ongoing (within the last 10⁸ yr) star formation rate, two values of the intrinsic extinction, and the IR (8-1000 $\mu$ m restframe) luminosity produced by the ongoing starburst, estimated assuming an M 82-like template. The two $A_{\rm V}$ values are computed by averaging over the whole galaxy life and over the last 10⁸ yr (representing the amount of dust affecting the ongoing burst). In parenthesis the 3 $\sigma$ ranges derived from the exploration of the parameter space are reported.
ID	Type	Class	z	Mass $(\star)$	SFR(10⁸ yr)	$A_{\rm V}$ (mean)	$A_{\rm V}$ (10⁸ yr)	L_IR
SWIRE	phot.	spec.	spec.	$[10^{11}~M_\odot]$	[ $M_\odot/\textrm{yr}]$	[mag]	[mag]	$[10^{11}~L_\odot]$
EN1_202261	P2	ELG	1.339	1.44 (1.41-2.36)	489 (171-741)	1.68 (1.29-1.73)	1.82 (1.71-1.88)	10.81 (8.48-12.84)
EN1_342445	P3L	ELG	1.917	1.04 (0.91-1.84)	426 (268-480)	1.10 (0.57-1.17)	1.40 (0.96-1.49)	9.37 (6.89-12.81)
EN1_340451	P3	NLAGN	2.866	6.69 (6.12-7.29)	56.1 (29.6-106)	0.63 (0.41-0.76)	2.18 (1.43-2.32)	36.79 (25.45-50.58)
EN2_11091	P3L	ELG	1.946	3.94 (2.37-4.20)	208 (197-575)	0.61 (0.29-0.89)	0.80 (0.71-1.82)	16.13 (10.58-20.94)
EN2_167372	P2L	ELG	1.445	2.62 (2.08-2.77)	86.9 (25.4-192)	0.59 (0.07-0.93)	1.34 (0.35-1.80)	4.98 (0.96-12.77)
EN2_166134	P2	ELG	1.337	3.40 (3.05-3.86)	17.9 (9.90-200)	0.79 (0.50-0.89)	1.65 (1.20-2.02)	9.06 (5.82-12.41)
LH_572243	P2,X	NLAGN	1.820	0.91 (0.85-0.92)	34.3 (27.7-91)	0.82 (0.79-0.90)	2.09 (1.99-2.28)	9.27 (9.04-10.51)

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