Table 1: HST photometry for SN2000ft and reference star clusters.

Region		 ${\it {\it F330W}}$ ${\it F547M}$ ${\it {\it F606W}}$ ${\it F814W}$ $\frac{\it F547M}{\it {\it F606W}}$ $\frac{\it F814W}{\it {\it F606W}}$ $\frac{\it {\it F330W}}{\it {\it F606W}}$
(1)a (2)b (3) (4) (5) (6)c (7) (8)

C2		 1.69 $\times$ 10-16 1.05 $\times$ 10-16 8.85 $\times$ 10-17 4.95 $\times$ 10-17 1.2 0.6 1.9
C3 7.38 $\times$ 10-17 6.74 $\times$ 10-17 4.94 $\times$ 10-17 2.36 $\times$ 10-17 1.4 0.5 1.5
C5 6.42 $\times$ 10-17 4.03 $\times$ 10-17 4.67 $\times$ 10-17 2.27 $\times$ 10-17 0.9 0.5 1.4
Mean ... ... ... ... 1.1 $\pm$ 0.2 0.51 $\pm$ 0.04 1.6 $\pm$ 0.2

C24d		 3.54 $\times$ 10-17 ... 1.60 $\times$ 10-17 ... ... ... 2.2
C24(fit)e 2.90 $\times$ 10-17 1.97 $\times$ 10-17 1.63 $\times$ 10-17 1.01 $\times$ 10-17 1.2 0.6 1.8
SN_Regionf 1.48 $\times$ 10-17 ... 1.43 $\times$ 10-17 ... ... ... 1.0
SN 2000ftg ... 6.83 $\times$ 10-17 ... 1.08 $\times$ 10-16 4.8 7.6 ...
a Cluster label after Díaz-Santos et al. (2007). b Measured fluxes in Cols. (2) to (5) given in erg s-1 cm-2 Å-1. c Flux ratios for the different regions as obtained from the measured fluxes given in previous columns. d Photometry of the closest cluster (C24) identified at a distance of 0 $.\!\!^{\prime\prime}$1 from SN 2000ft. No measurement is given for filters F547M and F814W due to its close distance to SN 2000ft. e Flux values for the corresponding filters, obtained from the best-fitted spectral energy distribution to the cluster C24 photometry covering the ultraviolet to near-infrared range (Díaz-Santos et al. 2007). f F330W and F606W values represent the fluxes measured through an aperture of 0 $.\!\!^{\prime\prime}$14 diameter centered at the position where SN 2000ft is detected in the F547M and F814W images. g Photometry of SN 2000ft in F547M and F814W images taken in May 13, 2000.

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