Table 1: Photometry for the stars resolved and the cores of the clusters, assuming E(B-V)=0.23 and d=3.84 Mpc. The x and y coordinates corresponds to the position in the chip and the first component in each cluster, S_0 and N_0 respectively, is the nucleus.
ID x y $M_{{\it F814W}}$ $M_{{\it F555W}}$ $M_{{\it F336W}}$

S_0 156.464 141.761 -11.40 -11.36 -12.52

S_1 152.662 135.563 -7.35 -7.76 -9.34

S_2 149.287 144.951 -7.81 -7.49 -8.77

S_3 156.938 149.177 -8.24 -7.70 -9.26

S_4 152.218 153.100 -6.65 -6.90 -8.31

S_5 164.261 141.302 -7.34 -6.43 -7.91

N_0 179.242 144.106 -10.69 -11.09 -12.54

N_1 185.427 134.498 -7.47 -7.75 -9.33

N_2 172.494 140.542 -5.13 -5.99 -7.87

N_3 168.281 140.623 -6.13 -6.73 -8.30

N_4 177.742 131.582 -6.83 -7.50 -9.35

**Table 1:** Photometry for the stars resolved and the cores of the clusters, assuming E(B-V)=0.23 and d=3.84 Mpc. The x and y coordinates corresponds to the position in the chip and the first component in each cluster, S_0 and N_0 respectively, is the nucleus.
ID	x	y	$M_{{\it F814W}}$	$M_{{\it F555W}}$	$M_{{\it F336W}}$
S_0	156.464	141.761	-11.40	-11.36	-12.52
S_1	152.662	135.563	-7.35	-7.76	-9.34
S_2	149.287	144.951	-7.81	-7.49	-8.77
S_3	156.938	149.177	-8.24	-7.70	-9.26
S_4	152.218	153.100	-6.65	-6.90	-8.31
S_5	164.261	141.302	-7.34	-6.43	-7.91
N_0	179.242	144.106	-10.69	-11.09	-12.54
N_1	185.427	134.498	-7.47	-7.75	-9.33
N_2	172.494	140.542	-5.13	-5.99	-7.87
N_3	168.281	140.623	-6.13	-6.73	-8.30
N_4	177.742	131.582	-6.83	-7.50	-9.35

Source LaTeX | All tables | In the text

	1 Introduction
	2 Multicolor photometry
	3 The binary cluster Sersic 13N-S
	4 Conclusions
	References