Examples of line-of-sight stellar kinematic maps from the CALIFA V1200 grating dataset. Top row: color-composite SDSS image of each galaxy. Middle row: stellar velocity maps. Bottom row: stellar velocity dispersion maps. From left to right: NGC 6125, a slow-rotator elliptical in our sample (i.e., low velocity amplitude and overall large velocity dispersion); NGC 1167, an early-type spiral galaxy with large velocity and central velocity dispersion amplitudes; NGC 4210, a disk-dominated galaxy (i.e., high velocity amplitude and overall small velocity dispersion); ARP 220, an interacting system (i.e., with complex stellar velocity and velocity dispersions maps). All maps share the same velocity and velocity dispersion scale and are in units of km s^-1 as indicated in the colorbars. Isophotes (black lines) are constructed from the V1200 CALIFA data cube.