Table 2: Summary of the principal characteristics of the NIR images used for the determination of the LF. Area $_{\rm eff}$ is the area of the region actually used in this work.
Cluster Telescope/Instrument Filter Resolution Completeness Area $_{\rm eff}$ References

$\hbox{$.\!\!^{\prime\prime}$ }$ AB mag arcmin²/Mpc²

RDCS J0910+5422 Palomar 5 m/PFIC $K_{\rm s}$ $0\hbox{$.\!\!^{\prime\prime}$ }9$ 21.5 4.35/1.06 Stanford et al. (2002)

RDCS J1252.9-2927 VLT/ISAAC $K_{\rm s}$ $0\hbox{$.\!\!^{\prime\prime}$ }45$ 24.5 3.69/0.93 Rosati et al. (2004)

Lidman et al. (2004)

Demarco et al. (in prep.)

RX J0848+4453 HST/NICMOS F160W $0\hbox{$.\!\!^{\prime\prime}$ }22$ 25 1.84/0.47 Stanford et al. (1997)

Holden et al. (2004)

van Dokkum & Stanford (2003)

**Table 2:** Summary of the principal characteristics of the NIR images used for the determination of the LF. Area $_{\rm eff}$ is the area of the region actually used in this work.
Cluster	Telescope/Instrument	Filter	Resolution	Completeness	Area $_{\rm eff}$	References
			$\hbox{$.\!\!^{\prime\prime}$ }$	AB mag	arcmin²/Mpc²
RDCS J0910+5422	Palomar 5 m/PFIC	$K_{\rm s}$	$0\hbox{$.\!\!^{\prime\prime}$ }9$	21.5	4.35/1.06	Stanford et al. (2002)
RDCS J1252.9-2927	VLT/ISAAC	$K_{\rm s}$	$0\hbox{$.\!\!^{\prime\prime}$ }45$	24.5	3.69/0.93	Rosati et al. (2004)
						Lidman et al. (2004)
						Demarco et al. (in prep.)
RX J0848+4453	HST/NICMOS	F160W	$0\hbox{$.\!\!^{\prime\prime}$ }22$	25	1.84/0.47	Stanford et al. (1997)
						Holden et al. (2004)
						van Dokkum & Stanford (2003)

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