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Table 1.

Ultraviolet-optical-IR data used in the SED fitting.

Instrument/ Band Central (a) Width (b) Depth (c)
Telescope λ [Å] [Å] (1.0″, 0.15″, 0.5″)
(Survey)
MegaCam u 3858 598 27.3
/CFHT

ACS/HST F814W 8333 2511 27.5

HSC g 4847 1383 27.6
/Subaru r 6219 1547 27.2
HSC-SSP i 7699 1471 27.0
PDR3 z 8894 766 26.6
y 9761 786 26.0

Suprime-Cam IB427 4266 207 25.7
/Subaru IA484 4851 229 26.2
IB505 5064 231 25.9
IA527 5261 243 26.1
IB574 5766 273 25.3
IB624 6232 300 26.1
IB679 6780 336 25.3
IB709 7073 316 25.7
IB738 7361 324 25.8
IB767 7694 365 25.3
IB827 8243 343 25.3

VIRCAM Y 10216 923 25.8
/VISTA J 12525 1718 25.8
UltraVISTA H 16466 2905 25.5
DR5 Ks 21557 3074 25.3

NIRCam F115W 11540 2250 27.2
F150W 15010 3170 27.4
F277W 27760 6730 28.1
F444W 44010 10230 28.0

MIRI F770W 76390 19500 25.2

Notes.

(a)

Median of the transmission curve.

(b)

Full width of the transmission curve at half maximum.

(c)

5σ depth computed in empty apertures with diameters of 1.0″ for the ground-based, 0.15″ for the space-based JWST/NIRCam and HST/ACS and 0.5″ for JWST/MIRI images, averaged over the NIRCam area.

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