Open Access

Table 1.

Summary of COSMOS2020 photometric bands used in this work.

Instrument Filter Effective Width
/Survey λ [Å] [Å]
MegaCam/CFHT u* 3823.3 670

Suprime-Cam IB427 4256.05 305.6
/Subaru B 4400.33 1399.1
IB464 4633.48 330.5
IB505 5060.57 378.1
IB527 5261.1 242
V 5477.8 955
IB574 5764.8 271.5
r 6136.24 1918
IB679 6778.75 555.3
IB709 7070.67 511.5
IB738 7358.64 490.2
i+ 7630.05 1872.5
IB827 8241.69 514.3
z++ 9020.18 1960.4
Y 9759.16 1752.8

VIRCAM YUD 10 214.2 970
/VISTA JUD 12 534.6 1720
(UltraVISTA-DR2) HUD 16 453.4 2900
K S UD $ K^{\mathrm{UD}}_{S} $ 21 539.9 3090

IRAC/Spitzer Ch1 35 634.3 7460
(SPLASH) Ch2 45 110.1 10 110
Ch3 57 593.4 14 140
Ch4 79 594.9 28 760

MIPS/Spitzer 24 μm 232 096 110 494

PACS/Herschel Green 979 036 558 974
Red 1.54 × 106 1.26 × 106
SPIRE/Herschel PSW 2.43 × 106 1.26 × 106
PMW 3.41 × 106 1.46 × 106
PLW 4.82 × 106 2.92 × 106

SCUBA/JCMT 2.450 GHz 4.48 × 106 1.04 × 106

Notes. The effective wavelength is the median wavelength weighted by transmission and the widths are defined as the difference between the maximum and the minimum wavelengths (calculated as the first and the last wavelengths with a transmission of at least 1%).

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