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Table 4.

Data availability per class and photometric band.

Class Sources [3.6] σ[3.6] [4.5] σ[4.5] [5.8] σ[5.8] [8.0] σ[8.0] [24] σ[24]
(#) (%) (%) (%) (%) (%) (%) (%) (%) (%) (%)
BSG 261 100 100 100 100 100 80 100 70 100 41
YSG 103 100 100 100 100 100 92 100 78 99 30
RSG 512 100 100 100 100 99 99 100 93 99 41
BeBR 17 100 100 100 100 100 100 100 100 100 94
LBV 6 100 100 100 100 100 100 100 100 100 66
WR 53 100 100 100 100 100 94 100 86 100 43
GAL 24 100 100 100 100 100 100 100 100 100 100

Class Sources g σg r σr i σi z σz y σy
(#) (%) (%) (%) (%) (%) (%) (%) (%) (%) (%)

BSG 261 96 96 96 96 96 96 96 96 96 96
YSG 103 96 96 96 96 96 96 96 96 96 96
RSG 512 96 93 97 97 97 97 97 97 97 97
BeBR 17 100 100 100 100 100 100 100 100 94 94
LBV 6 100 100 100 100 100 100 100 100 100 100
WR 53 83 83 84 83 88 88 90 88 86 84
GAL 24 100 100 100 100 100 100 100 95 100 100

Class Sources JUK G GBP GRP

(#) (%) (%) (%) (%)
BSG 261 81 90 87 87
YSG 103 82 96 95 95
RSG 512 84 96 94 94
BeBR 17 70 100 100 100
LBV 6 66 83 66 66
WR 53 75 71 50 50
GAL 24 83 95 83 83

Notes. The first column lists the classes used and the second one the corresponding number of sources in the sample. For each class, the subsequent columns provide the fractions of sources with secure measurements in the corresponding photometric bands and their errors (which do not include objects with problematic measurements and upper limits).

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