Table 2: IRAC and MIPS 24 $\mu$ m photometry of the EROs listed in Table 1 taken from Paper I. All fluxes are given in $\mu$ Jy. Upper limits are 1-sigma noise values at the position of the sources. Due to source blending the data is uncomplete, i.e. not available for objects A1835-#3, A1835-#10, and A1835-#11, and partially for A1835-#1.
IRAC/Spitzer MIPS

Object 3.6 4.5 5.8 8.0 24.0

A1835-#1 2.9 $\pm$ 0.2 4.0 $\pm$ 0.2 blended <10

A1835-#2 14.4 $\pm$ 0.2 23.3 $\pm$ 0.3 37.6 $\pm$ 1.5 50.9 $\pm$ 1.6 320 $\pm$ 11

A1835-#4 1.9 $\pm$ 0.2 1.0 $\pm$ 0.3 <1.2 <1.5 <10

A1835-#17 2.4 $\pm$ 0.2 1.6 $\pm$ 0.2 <1.2 <1.5 <10

AC114-#1 67.3 $\pm$ 0.5 64.4 $\pm$ 0.5 50.3 $\pm$ 1.5 44.9 $\pm$ 2.2 189.0 $\pm$ 8.9

**Table 2:** IRAC and MIPS 24 $\mu$ m photometry of the EROs listed in Table 1 taken from Paper I. All fluxes are given in $\mu$ Jy. Upper limits are 1-sigma noise values at the position of the sources. Due to source blending the data is uncomplete, i.e. not available for objects A1835-#3, A1835-#10, and A1835-#11, and partially for A1835-#1.
	IRAC/Spitzer	MIPS
Object	3.6	4.5	5.8	8.0	24.0
A1835-#1	2.9 $\pm$ 0.2	4.0 $\pm$ 0.2	blended	<10
A1835-#2	14.4 $\pm$ 0.2	23.3 $\pm$ 0.3	37.6 $\pm$ 1.5	50.9 $\pm$ 1.6	320 $\pm$ 11
A1835-#4	1.9 $\pm$ 0.2	1.0 $\pm$ 0.3	<1.2	<1.5	<10
A1835-#17	2.4 $\pm$ 0.2	1.6 $\pm$ 0.2	<1.2	<1.5	<10
AC114-#1	67.3 $\pm$ 0.5	64.4 $\pm$ 0.5	50.3 $\pm$ 1.5	44.9 $\pm$ 2.2	189.0 $\pm$ 8.9

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