Kinematics and Angular Momentum in Early Type Galaxy Halos
  We use the kinematics of discrete tracers, primarily globular clusters (GCs)
and planetary nebulae (PNe), along with measurements of the integrated
starlight to explore the assembly histories of early type galaxies. Data for
GCs and stars are taken from the SLUGGS wide field, 2-dimensional,
chemo-dynamical survey (Brodie et al. 2014). Data for PNe are from the PN.S
survey (see contributions by Gerhard and by Arnaboldi, this volume). We find
widespread evidence for 2-phase galaxy assembly and intriguing constraints on
hierarchical merging under a lambda CDM cosmology.
