Table 1: Photometry of the selected ERO subsample in Abell 1835 and AC 114 taken from Hempel et al. (2007, Paper II). All magnitudes are given in the Vega system. For conversion to the AB system see the filter properties listed in Table 3. Non-detections (lower limits) are 1 values. NA stands for non-available.

Object	V	R	I		SZ	J	H	Ks
A1835-#1	>28.1	>27.8	>26.7				22.40  0.08	20.74  0.02
A1835-#2	>28.1	>27.8	>26.7	>27.46	24.08  0.26	24.41  1.34	21.78  0.06	20.45  0.02
A1835-#3	>28.1	>27.8	>26.7	24.06  0.07a	23.78  0.10	24.32  0.47	22.55  0.07	21.58  0.03
A1835-#4	>28.1	>27.8	>26.7	25.48  0.14	24.44  0.15	23.56  0.18	22.90  0.07	21.95  0.03
A1835-#10	>28.1	>27.8	>26.7	25.56  0.11	24.00  0.12	23.72  0.26	23.36  0.13	21.67  0.03
A1835-#11	>28.1	>27.8	>26.7	>27.46	>26.9	23.92  0.37	23.49  0.18	21.29  0.03
A1835-#17	>28.1	>27.8	>26.7	>27.46	>26.9	>25.6	23.51  0.16	22.11  0.03
AC114-#1	>28.5	>27.7	>26.8	24.55  0.07	NA	21.26  0.04		18.62  0.001

a This source appears double in the image. The fainter component has 25.31  0.07. In the SED modeling the brighter magnitude or the sum of two have been used.