The SAMI Pilot Survey: Stellar Kinematics of Galaxies in Abell 85, 168
  and 2399
  We present the SAMI Pilot Survey, consisting of integral field spectroscopy
of 106 galaxies across three galaxy clusters, Abell 85, Abell 168 and Abell
2399. The galaxies were selected by absolute magnitude to have $M_r<-20.25$
mag. The survey, using the Sydney-AAO Multi-object Integral field spectrograph
(SAMI), comprises observations of galaxies of all morphological types with 75\%
of the sample being early-type galaxies (ETGs) and 25\% being late-type
galaxies (LTGs). Stellar velocity and velocity dispersion maps are derived for
all 106 galaxies in the sample.
  The $\lambda_{R}$ parameter, a proxy for the specific stellar angular
momentum, is calculated for each galaxy in the sample. We find a trend between
$\lambda_{R}$ and galaxy concentration such that LTGs are less concentrated
higher angular momentum systems, with the fast-rotating ETGs (FRs) more
concentrated and lower in angular momentum. This suggests that some dynamical
processes are involved in transforming LTGs to FRs, though a significant
overlap between the $\lambda_{R}$ distributions of these classes of galaxies
implies that this is just one piece of a more complicated picture.
  We measure the kinematic misalignment angle, $\Psi$, for the ETGs in the
sample, to probe the intrinsic shapes of the galaxies. We find the majority of
FRs (83\%) to be aligned, consistent with them being oblate spheroids (i.e.
disks). The slow rotating ETGs (SRs), on the other hand, are significantly more
likely to show kinematic misalignment (only 38\% are aligned). This confirms
previous results that SRs are likely to be mildly triaxial systems.
