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Table 1.
Summary of available photometric data in each band used for the SED fitting.
Telescope/ | Filter | λmean | Ngal |
---|---|---|---|
Instrument | (μm) | ||
GALEX | FUV | 0.155 | 348 |
NUV | 0.234 | 2 352 | |
CFHT/MegaCam | u | 0.369 | 6 793 |
g | 0.482 | 6960 | |
r | 0.643 | 6955 | |
i | 0.772 | 5689 | |
z | 0.900 | 6958 | |
iy | 0.769 | 1272 | |
CFHT/Wircam | Ks | 2.150 | 476 |
VISTA | Kvideo | 2.158 | 6445 |
WISE | W1 | 3.353 | 4499 |
W2 | 4.603 | 4499 | |
W3 | 11.561 | 4499 | |
W4 | 22.088 | 4499 | |
Spitzer/IRAC | I1 | 3.557 | 1 299 |
I2 | 4.505 | 1334 | |
I3 | 5.739 | 411 | |
I4 | 7.927 | 118 | |
Spitzer/MIPS | 24 μm | 23.843 | 219 |
70 μm | 72.555 | 17 | |
160 μm | 157.000 | 4 |
Notes. The third column, λmean, is the centre of the specific filter band given in μm. The last column, Ngal, provides the number of detections in the sample of 6961 UCMG candidates.
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