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Table 3.

COSMOS broad and intermediate bands used in this work.

Instrument Band λ (μm) # of sources # final
GALEX FUV 0.153 331 5
GALEX NUV 0.229 376 7
CFHT u 0.355 376 7
SUBARU B 0.443 376 7
SUBARU V 0.544 376 7
SUBARU r 0.622 376 7
Suprime Cam i 0.767 376 7
Suprime Cam z 0.902 376 7
Intermediate bands 0.427 376 7
0.464 376 7
0.505 376 7
0.527 376 7
0.574 376 7
0.624 376 7
0.709 376 7
0.738 376 7
0.767 376 7
0.827 376 7
HSC Y 376 7
VISTA Y 1.019 376 7
VISTA J 1.250 376 7
VISTA H 1.639 376 7
VISTA Ks 2.142 376 7
Spitzer IRAC1 3.6 376 7
Spitzer IRAC2 4.5 376 7
Spitzer IRAC3 5.8 300 5
Spitzer IRAC4 8.0 179 1
Spitzer MIPS 24 194 4
Herschel PACS 100 53 0
Herschel PACS 160 40 0
Herschel SPIRE 250 42 1
Herschel SPIRE 350 18 1

Notes. The data up to Spitzer/IRAC4 are from Laigle et al. (2016) while the IR data are from Jin et al. (2018). The number of sources with a detection in each band is provided in the last two columns for the whole sample and the selected quenched sources.

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