Table 3: Main characteristics of the datasets in Groth. Column (1): observing band. Column (2): effective wavelength of the filter calculated by convolving the Vega spectrum (Colina & Bohlin 1994) with the transmission curve of the filter+detector. Column (3): limiting AB magnitude. Column (4): source from where the data were obtained.
Band $\lambda_{\rm eff}(\mu {\rm m})$ $m_{\lim}$ Source
(1) (2) (3) (4)
Kp............ 2.114 20.3 CAHA-Oprime
R............. 0.652 - Subaru deep imaging
u............. 0.381 27 CFHTLS
g............. 0.486 28.3 CFHTLS
r............. 0.626 27.5 CFHTLS
i............. 0.769 27 CFHTLS
z............. 0.887 26.4 CFHTLS
B............. 0.437 24.5 CFHT-12k
R............. 0.660 24.2 CFHT-12k
I............. 0.813 23.5 CFHT-12k
J............. 1.255 22 WHT-INGRID
K............. 2.170 21.8 WHT-INGRID
IRAC-3.6....... 3.561 21.6 Spitzer GTO
IRAC-4.5....... 4.510 21.8 Spitzer GTO
IRAC-5.8....... 5.690 21.8 Spitzer GTO
IRAC-8.0....... 7.957 21.7 Spitzer GTO
nuv........... 0.232 24.5 GALEX GTO
fuv........... 0.154 24.5 GALEX GTO
U............. 0.361 24.8 INT-WFC
B............. 0.436 25.5 INT-WFC
R, redshift.... 0.660 24.2 DEEP2


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