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Table 1.

Broad- and narrow-band set of filters employed as input data in the CIGALE SED fitting, where λmean defines the central wavelength of the filters, and MAGAB quantifies the apparent magnitudes for each filter over the 0.25, 0.5, and 0.75 quantiles.

Telescope/Camera Filter name λmean MAGAB
[μm] 25%/50%/75%
GALEX FUV 0.154 24.19/24.83/25.50
NUV 0.231 23.48/24.41/25.01
CFHT/Megacam U 0.382 24.20/25.37/26.39
Subaru/HSC g 0.485 23.46/24.69/25.80
r 0.622 22.57/23.78/24.93
i 0.750 21.74/22.91/24.18
z 0.889 21.29/22.30/23.51
Y 0.976 21.00/21.93/23.03
IA427 0.427 23.84/25.00/25.94
IA464 0.464 23.51/24.67/25.59
IA484 0.484 23.50/24.68/25.69
IA505 0.505 23.30/24.52/25.48
IA527 0.527 23.26/24.49/25.52
IA574 0.574 22.92/24.11/25.12
IA624 0.624 22.65/23.86/24.97
IA679 0.679 22.08/23.34/24.52
IB709 0.709 22.11/23.37/24.59
IB738 0.738 21.95/23.17/24.44
IB767 0.767 21.74/22.93/24.25
IB827 0.827 21.56/22.66/24.00
NB711 0.711 22.00/23.24/24.41
NB816 0.816 21.60/22.72/24.04
U-VISTA Y 1.021 20.92/21.81/22.86
J 1.253 20.51/21.30/22.19
H 1.645 20.09/20.84/21.62
Ks 2.153 19.63/20.30/21.08
NB118 1.191 20.70/21.49/22.35
Spitzer/IRAC CH1 0.744 19.49/19.98/20.49
CH2 1.011 19.59/20.02/20.43
CH3 1.408 19.63/20.04/20.41
CH4 2.879 19.75/20.24/20.68
Spitzer/MIPS – 23.674 17.43/17.93/18.50

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