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Table 1:

Summary of the different imaging data used for this analysis.
Camera Band Date Exp. [s] Limit [mag]
Suprime B 2004-02-19 4320 27.3
V 2004-02-18 3240 26.6
r+ 2004-01-19 2160 26.8
i+ 2004-01-22 2880 26.2
z+ 2004-01-21 4320 25.2
Megacam $u\star$ 2004-2005(a) $\sim$40 000 26.4
ACS F814w 2004-04-08 2028 27.1(b)
WFPC2 F606W 2008-01-07 1200 26.5

The magnitude limits for the COSMOS observations are those shown in Capak et al. (2007) for the ground-based observations and in Koekemoer et al. (2007) for the HST observations. (a) The $u^\star $ frame was created by combining observations taken between the years 2004 and 2005, thus, the total exposure time of the COSMOS field in this band varies. (b) 27.1 is the magnitude limit for a point-like object in the ACS exposure and increases in brightness to 26.1 for a 1 $^{\prime \prime }$-wide extended object.


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