**Table 5:** Derived/estimated properties for optical dropout ERO galaxies with near-IR and Spitzer detections. Listed are the object ID (Col. 1), the photometric redshift estimate (Col. 2), the extinction (Col. 3), the type of the best fit template (Col. 4), the distance modulus corresponding to $z_{\rm phot}$ (Col. 5), the absolute $K\rm s$ -band magnitude non-corrected for lensing (Col. 6), the absolute rest-frame $K\rm s$ -band magnitude non-corrected for lensing (Col. 7), the estimated stellar mass (from scaling the SED fit or from $M^{\rm rest}(K\rm s)$ assuming L_K/M=3.2, Col. 8), the estimated star formation rate non-corrected for lensing (Col. 9), and the age of the stellar population (Col. 10). To correct the above mentioned absolute quantities for gravitational magnification the appropriate magnification factors listed in Table 4 must be used.
Object	$z_{\rm phot}$	$A_{\rm v}$	Template	DM^a	$M^{\rm rest}(K{\rm s})-2.5\log(\mu)$	${\rm Mass}\times \mu$	${\it SFR}\times \mu$	Stellar age
		[mag]		[mag]	[mag]	$M_{\odot}$	$M_{\odot}$ yr^-1	[Gyr]
A1835-#1	$\sim$ 0.4-1.5	?	Fits uncertain - see text
A1835-#2	$\sim$ 2.8-3	2.4-3	young burst	47.0	-27.7	$\sim$ $1.2 \times 10^{12}$	$\sim$ 2100	<0.36
A1835-#4	$\sim$ 1.2	0-1.6	burst/elliptical	44.60	-21.6	$\sim$ $1.7 \times 10^{10}$	$\sim$ 5	0.7 to 4.5
A1835-#17	$\sim$ 0.7-0.8	$\sim$ 3.8	burst	43.0	-21.7	$\sim 1.3 \times 10^{10}$ ?	$\sim$ 0.9	? (see text)
AC114-#1	$\sim$ 1.3-1.6	$\sim$ 1.6-2.8	burst	44.84	-26.4	$(1.3{-}2.6) \times 10^{12}$		$\sim$ 0.9-4.5 Gyr
AC114-#1	$\sim$ 1.0	+3.8	M51	44.03	-25.9		$\sim$ 48

^a Distance modulus computed for minimum redshift.

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