  We describe a new technique to measure stellar kinematics and line-strengths
at large radii in nearby galaxies. Using the integral-field spectrograph SAURON
as a 'photon-collector', we obtain spectra out to four effective radii (Re) in
the early-type galaxy NGC 3379. By fitting orbit-based models to the extracted
stellar velocity profile, we find that ~40% of the total mass within 5 Re is
dark. The measured absorption line-strengths reveal a radial gradient with
constant slope out to 4 Re.
