ATLAS3D project. XXIII.
Davor Krajnović, A. M. Karick, R. L. Davies, T. Naab, M. Sarzi, E. Emsellem, M. Cappellari, P. Serra, P. T. de Zeeuw, N. Scott, Mcdermid, R.M., Weijmans, A.-M., Davis, T.A., Alatalo, K., Blitz, L., Bois, M., Bureau, M., Bournaud, F., Crocker, A., Duc, P.-A. · Swinburne figshare (Swinburne University of Technology) · 2014
The ATLAS3D sample is defined in Paper I and consists o early-type galaxies, visually selected from a magnitude (brighter than -21.5mag in the K band) and volume-limited (within 42 Mpc) parent sample. The full sample was observed with the integral-field spectrograph (IFS) SAURON (Bacon et al. 2001MNRAS.326...23B) mounted on William Herschel Telescope. The extraction of kinematics from the SAURON data is described in Paper I (Cappellari et al., 2011MNRAS.413..813C) and Emsellem et al. (2004MNRAS.352..721E), for the sub-sample of 48 galaxies previously presented in the SAURON survey. (1 data file).