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Table 1.

Measured 5σ limiting magnitudes for each band used in this work in the COSMOS field.

Filter Depth (5σ) Instrument
g 27.8 HSC
r 27.4 HSC
i 27.2 HSC
NB0816 26.2 HSC
z 26.7 HSC
NB0921 26.0 HSC
y 26.0 HSC

Y 26.2 VISTA
J 26.0 VISTA
H 25.7 VISTA
Ks 25.3 VISTA

IE 27.7 Euclid
YE 26.4 Euclid
JE 26.4 Euclid
HE 26.3 Euclid

3.6 25.2 Spitzer/IRAC
4.5 25.2 Spitzer/IRAC

Notes. The local depths were measured by placing 1 . 8 Mathematical equation: $ 1{{\overset{\prime\prime}{.}}}8 $ diameter circular apertures on empty regions of the images. The depth quoted here is the mode of these local depths. Depths for Euclid were measured on images pixel-matched and PSF-homogenised to the VISTA Y band. IRAC depths were measured in 2 . 8 Mathematical equation: $ 2{{\overset{\prime\prime}{.}}}8 $ diameter circular apertures on the original resolution image to account for the poorer resolution.

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