Table 2:
Major diameter statistics. The first two columns give the
samples and the number of galaxies. The next three columns give
the mean value, standard deviation (sd), and standard error
(se) of the galaxy samples for
,
,
,
and all. The last column
gives the cluster position angle (cPA) in the galactic coordinate
system. The cPA is estimated using the least-square fit method (see
Fig. 1c).