We present results from a new and unique integral-field spectrograph, SAURON.
It has a large field of view and high throughput and is primarily built for the
study of stellar & gaseous kinematics and stellar populations in galaxies. Its
aim is to carry out a systematic survey of the velocity fields, velocity
dispersions, and line-strength distributions of nearby ellipticals, lenticular
galaxies and spiral bulges. Its wide field is especially useful for the study
of complicated velocity structures. Together with other spectroscopic data,
images, and dynamical modelling, SAURON will help to constrain the intrinsic
shapes, mass-to-light ratios, and stellar populations of early-type galaxies
and spiral bulges.Comment: 1 page, 1 figure, to appear in Revista Mexicana de Astrofisica y
Astronomia Conf. Serie