| Summary: | We examine the kinematic morphology of early-type galaxies (ETGs) in eight galaxy clusters in the Sydney-AAO Multi-object Integral-field spectrograph Galaxy Survey. The clusters cover a mass range of 14.2 < log(M_(200)/M_☉) < 15.2 and we measure spatially resolved stellar kinematics for 315 member galaxies with stellar masses 10.0 © 2017 American Astronomical Society. Received 2017 April 4. Accepted 2017 June 15. Published 2017 July 21. We thank the anonymous referee for their positive and valuable comments that have improved this paper. S.B. would like to thank Michele Cappellari for helpful discussions. S.B. acknowledges the funding support from the Australian Research Council through a Future Fellowship (FT140101166). J.v.d.S. is funded under Bland-Hawthorn's ARC Laureate Fellowship (FL140100278). M.S.O. acknowledges the funding support from the Australian Research Council through a Future Fellowship Fellowship (FT140100255). N.S. acknowledges the support of a University of Sydney Postdoctoral Fellowship. S.M.C. acknowledges the support of an Australian Research Council Future Fellowship (FT100100457). This work was supported by the UK Science and Technology Facilities Council through the "Astrophysics at Oxford" grant ST/K00106X/1. R.L.D. acknowledges travel and computer grants from Christ Church, Oxford and support from the Oxford Centre for Astrophysical Surveys which is funded by the Hintze Family Charitable Foundation. Support for A.M.M. is provided by NASA through Hubble Fellowship grant HST-HF2-51377 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. S.K.Y. acknowledges support from the Korean National Research Foundation (2017R1A2A1A05001116) and by the Yonsei University Future Leading Research Initiative (2015-22-0064). This study was performed under the umbrella of the joint collaboration between Yonsei University Observatory and the Korean Astronomy and Space Science ...
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