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Table 1.

Photometric bands available in the four fields covered by the VANDELS survey and used for the estimation of stellar masses, SFR, and UV slope.

Field Bands used
CDFS-HST F435W, F606W, F775W, F814W, F850LP, F098M, F105W, F125W, F140W, F160W, VIMOS-R, ISAAC-Ks, HAWKI-Ks, IRAC-ch1, IRAC-ch2

CDFS-GROUND B-WFI, F606W, F850LP, subaru-IA484, subaru-IA527, subaru-IA598, subaru-IA624, subaru-IA651, VIMOS-R, subaru-IA679, subaru-IA738, subaru-IA767, VISTA-Z, VISTA-Y, VISTA-J, VISTA-H, VISTA-K, IRAC-ch1, IRAC-ch2

UDS-HST subaru-B, F606W, subaru-V, subaru-i, F814W, subaru-z, HAWKI-Y, WFCAM-J, F125W, F160W, wfcam-H, wfcam-K, HAWKI-Ks, IRAC-ch1, IRAC-ch2

UDS-GROUND subaru-B, subaru-V, subaru-i, subaru-z, subaru-znew, VISTA-Y, wfcam-J, wfcam-H, wfcam-K, IRAC-ch1, IRAC-ch2

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