Table C.1: Photometric parameters for the MS 0451 sample.
ID RA Dec z V R I MB A C
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
C1 04:54:2.2 -02:57:10 0.5421 21.94 20.85 19.95 -21.06 0.25219 0.32179
C2 04:54:17.2 -03:01:56 0.5486 22.02 21.00 20.07 -20.91 0.15682 0.34844
C3 04:54:18.6 -03:01:03 0.5465 22.16 21.20 20.49 -20.68 0.07922 0.27806
C4 04:54:17.6 -02:59:23 0.5324 22.34 21.41 20.72 -20.37 0.36244 0.33291
C5 04:54:1.5 -02:59:24 0.5312 22.42 21.01 19.81 -20.82 0.15670 0.52285
C6 04:54:1.3 -02:59:22 0.5305 21.83 21.15 20.59 -20.59 0.32947 0.40650
C7 04:54:5.0 -02:59:40 0.5277 19.75 19.23 18.86 -22.45 0.32994 0.20636
C8 04:54:4.4 -03:00:14 0.5325 20.80 20.10 19.46 -21.68 0.27380 0.27789
C9 04:54:15.0 -03:00:22 0.5246 20.56 19.89 19.46 -21.76 0.33459 0.26970
C10 04:54:17.7 -03:02:29 0.5312 21.92 21.61 21.21 -20.05 0.19672 0.21096
C11 04:54:10.3 -03:00:46 - - - - - - -
F1 04:54:2.7 -02:58:41 0.9009 23.27 22.75 21.46 -20.97 0.18516 0.18578
F2 04:54:3.8 -02:59:19 0.5795 20.88 20.11 19.42 -21.96 0.27311 0.22909
F3 04:54:14.9 -02:58:17 0.5667 21.88 21.24 20.64 -20.66 0.33834 0.20427
F4 04:54:7.8 -03:00:33 0.1867 20.54 20.37 20.00 -18.78 0.17365 0.32308
F5 04:54:10.0 -03:00:28 0.1573 19.05 18.72 18.26 -19.95 0.19844 0.30783
F6 04:54:18.9 -03:00:05 0.0982 19.23 18.93 18.55 -18.56 0.14823 0.27114
F7 04:54:2.3 -02:58:10 0.9125 22.22 21.91 20.73 -21.64 0.42715 0.16334
F8 04:54:10.4 -03:00:47 0.4443 - - - - - -
F9 04:54:10.2 -03:01:57 0.3259 20.83 20.03 19.08 -20.15 0.29565 0.53731
F10 04:54:0.5 -02:58:15 0.4947 22.47 21.86 21.38 -19.67 0.20119 0.23420
F11 04:54:20.6 -03:00:16 - 21.25 20.67 20.04 - 0.18512 0.27344
Column (1): object ID; Cols. (2, 3): RA and Dec (J2000); Col. (4): object redshift; Cols. (5-7): V, R, I extinction corrected total magnitudes from the FORS2/VLT images; Col. (8): rest frame Johnson-B magnitudes k-corrected with kcorrect (Blanton & Roweis 2007); Col. (9): asymmetry index; Col. (10): concentration index.
For F11, the redshift is uncertain as explained in Sect. 2.3. Redshift of galaxy F7 and C11 are taken from Moran (2008). Galaxy C11 and F8 are so close together on the FORS images that their magnitudes could not be measured separately.

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