Table 2: Photometric properties of the 14 compact Fornax cluster members detected only in the NUV GALEX archival images.
ID RA [2000] Dec [2000] V0 [mag] (V-I)0 ( ${\it NUV-V}$)0
NTT414 3:38:09.7 -35:23:01.3 19.57 (0.17) 0.97 (0.11) 4.12 (0.23)
NTT410 3:38:12.2 -35:24:06.5 19.71 (0.12) 1.18 (0.08) 2.86 (0.25)
UCD20 3:37:27.6 -35:30:12.6 20.04 (0.07) 1.02 (0.04) 3.72 (0.18)
UCD18 3:36:55.5 -35:21:36.0 20.29 (0.04) 0.71 (0.04) 1.29 (0.05)
FCOS 1_0630 3:38:56.1 -35:24:49.0 20.31 (0.08) 1.00 (0.07) 3.19 (0.16)
FCOS 2_2165 3:37:28.2 -35:21:23.0 20.60 (0.08) 0.95 (0.07) 3.44 (0.19)
gc235.7 3:36:12.7 -35:19:11.6 20.64 (0.07) 0.89 (0.03) 2.69 (0.11)
Y7225 3:37:47.2 -35:22:57.4 20.71 (0.10) 0.92 (0.08) 2.82 (0.18)
gc290.6 3:35:42.5 -35:13:52.0 20.92 (0.04) 0.94 (0.02) 1.70 (0.07)
FCOS 1_2089 3:38:48.9 -35:27:43.9 20.97 (0.09) 0.99 (0.08) 3.33 (0.22)
91.041 3:37:56.9 -35:31:50.9 21.12 (0.08) 0.90 (0.05) 2.93 (0.22)
86.112 3:38:41.4 -35:27:41.0 21.29 (0.07) 0.99 (0.05) 2.57 (0.24)
Y1149 3:36:58.0 -35:34:32.2 21.29 (0.06) 0.82 (0.05) 2.17 (0.10)
81.008 3:38:03.0 -35:26:28.3 21.41 (0.09) 0.96 (0.05) 2.55 (0.19)
The objects are ordered by increasing V0 magnitude. The object IDs indicate the following sources: NTTxxx = Kissler-Patig et al. (1999); UCDxx = Firth et al. (2007) and Evstigneeva et al. (2008); FCOS xxxxx = Mieske et al. (2002, 2004); Yxxxxx = Richtler et al. (2008); gcxxx and ucxxx = Bergond et al. (2007); xx.xxx = Dirsch et al. (2004).

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