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Table A.2

Aperture corrections derived for each filter in ELAIS-N1 and Lockman Hole, using the method described in Sect. 3.3.1.

Survey-Filter Galaxies-based corrections Stellar-based corrections
Fraction of flux in aperture (arcsec) Fraction of flux in aperture (arcsec)
1 2 3 4 5 6 7 1 2 3 4 5 6 7
ELAIS-N1
SpARCS-u 0.39 0.76 0.9 0.95 0.97 0.98 0.99 0.41 0.79 0.91 0.96 0.98 0.99 1.0
PS1-g 0.25 0.6 0.78 0.87 0.92 0.95 0.97 0.27 0.62 0.79 0.88 0.93 0.96 0.98
PS1-r 0.25 0.6 0.77 0.85 0.91 0.94 0.97 0.3 0.64 0.8 0.88 0.92 0.95 0.97
PS1-i 0.23 0.55 0.74 0.83 0.89 0.93 0.96 0.31 0.65 0.8 0.87 0.92 0.95 0.97
PS1-z 0.23 0.54 0.73 0.84 0.9 0.94 0.96 0.33 0.66 0.81 0.88 0.92 0.95 0.97
PS1-y 0.2 0.49 0.68 0.79 0.86 0.91 0.95 0.29 0.59 0.75 0.84 0.89 0.93 0.95
HSC-g 0.55 0.83 0.91 0.95 0.97 0.98 0.99 0.56 0.84 0.92 0.95 0.97 0.98 0.99
HSC-r 0.46 0.8 0.9 0.94 0.96 0.97 0.98 0.49 0.82 0.91 0.95 0.97 0.98 0.99
HSC-i 0.61 0.87 0.92 0.95 0.97 0.98 0.99 0.64 0.9 0.94 0.96 0.97 0.98 0.99
HSC-z 0.37 0.71 0.85 0.91 0.95 0.97 0.98 0.47 0.8 0.91 0.95 0.97 0.98 0.99
HSC-y 0.49 0.78 0.87 0.92 0.95 0.97 0.98 0.63 0.86 0.92 0.94 0.96 0.97 0.98
HSC-NB921 0.35 0.69 0.84 0.91 0.94 0.97 0.98 0.63 0.88 0.94 0.97 0.98 0.99 0.99
J 0.39 0.78 0.92 0.96 0.98 0.99 1.0 0.45 0.82 0.93 0.97 0.99 0.99 1.0
K 0.32 0.7 0.88 0.95 0.98 0.99 1.0 0.42 0.79 0.92 0.96 0.98 1.0 1.0
IRAC-3.6 μm 0.1 0.34 0.56 0.73 0.83 0.89 0.93 0.13 0.4 0.64 0.79 0.88 0.93 0.95
IRAC-4.5 μm 0.11 0.34 0.56 0.72 0.84 0.9 0.94 0.13 0.4 0.63 0.78 0.88 0.94 0.96
IRAC-5.8 μm 0.08 0.26 0.45 0.62 0.74 0.84 0.91 0.11 0.33 0.53 0.68 0.8 0.89 0.95
IRAC-8.0 μm 0.07 0.25 0.43 0.58 0.68 0.77 0.85 0.09 0.3 0.5 0.64 0.73 0.82 0.9
Lockman Hole
SpARCS-u 0.31 0.69 0.87 0.94 0.97 0.98 0.99 0.35 0.73 0.88 0.95 0.97 0.99 0.99
SpARCS-g 0.21 0.54 0.76 0.87 0.93 0.96 0.98 0.33 0.72 0.88 0.94 0.97 0.98 0.99
SpARCS-r 0.24 0.57 0.78 0.89 0.94 0.97 0.98 0.49 0.82 0.92 0.96 0.97 0.98 0.99
SpARCS-z 0.29 0.64 0.83 0.91 0.96 0.98 0.99 0.52 0.82 0.91 0.95 0.97 0.98 0.99
RCSLenS-g 0.23 0.57 0.78 0.88 0.93 0.96 0.98 0.48 0.83 0.93 0.96 0.98 0.99 0.99
RCSLenS-r 0.25 0.58 0.78 0.89 0.94 0.97 0.98 0.55 0.86 0.94 0.97 0.98 0.99 0.99
RCSLenS-i 0.33 0.68 0.85 0.93 0.97 0.99 0.99 0.61 0.89 0.95 0.97 0.99 0.99 1.0
RCSLenS-z 0.28 0.62 0.8 0.89 0.94 0.97 0.99 0.56 0.84 0.92 0.96 0.97 0.98 0.99
J 0.29 0.67 0.86 0.95 0.98 1.0 1.0 0.46 0.82 0.93 0.97 0.98 0.99 1.0
K 0.32 0.7 0.88 0.96 0.99 1.01 1.01 0.47 0.82 0.92 0.96 0.98 0.99 1.0
IRAC-3.6 μm 0.1 0.33 0.56 0.73 0.83 0.89 0.93 0.13 0.4 0.63 0.79 0.88 0.92 0.95
IRAC-4.5 μm 0.11 0.34 0.56 0.72 0.83 0.9 0.94 0.13 0.4 0.63 0.77 0.87 0.93 0.96
IRAC-5.8 μm 0.08 0.27 0.46 0.61 0.74 0.84 0.91 0.1 0.32 0.52 0.67 0.78 0.88 0.94
IRAC-8.0 μm 0.07 0.25 0.44 0.58 0.68 0.77 0.85 0.09 0.29 0.49 0.62 0.7 0.79 0.88

Notes. The raw aperture fluxes released in the catalogues should be divided by the values listed to correct the fluxes for aperture effects. The galaxies-based aperture corrections are appropriate for moderately distant galaxies and are applied to both the value-added catalogues and multi-wavelength catalogues in our recommended aperture sizes. Stellar-based corrections (not applied to catalogues) are derived using stars in Gaia-DR2 with 18 < Gmag < 20.

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