Table 4
Photometric properties of the clusters in our sample.
| Cluster | xc (pix) | yc (pix) | Δ (pix) | RAc (J2000) | Decc (J2000) | Δ(′′) | Reference image | NG06 (′′) | log Ltot(L⊙) |
|
|
|||||||||
| NGC 1851 | 2919 | 3011 | 7 | 05:14:06.7 | −40:02:49.3 | 0.3 | ACS SURVEY | 0.1 | 5.25 |
| NGC 1904 | 262 | 289 | 9 | 05:24:11.0 | −24:31:27.9 | 0.5 | u2vo0402t_c0f.fits | 0.0 | 4.95 |
| NGC 5694 | 453 | 367 | 8 | 14:39:36.3 | −26:32:19.6 | 0.4 | u2y70105t_c0f.fits | 0.7 | 5.10 |
| NGC 5824 | 365 | 313 | 3 | 15:03:58.6 | −33:04:05.3 | 0.2 | u2y70205t_c0f.fits | 0.4 | 5.39 |
| NGC 6093 | 3007 | 2943 | 16 | 16:17:02.4 | −22:58:32.6 | 0.7 | ACS SURVEY | 1.0 | 5.18 |
| NGC 6266 | 1764 | 3424 | 6 | 17:01:13.0 | −30:06:48.2 | 0.3 | j92103050_drz.fits | 2.8 | 5.57 |
Notes. The columns are: (1) name of the cluster (2, 3) position of the center on the image in pixel, (4) uncertainties in pixel, (5, 6) position of the center on the image in RA and Dec, (7) uncertainties in arcseconds, (8) reference image used for the center determination, (9) distance to the center derived in Noyola & Gebhardt (2006), and (10) total luminosity of the cluster.
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