We present a comprehensive analysis of the spatial, kinematic and chemical properties of stars and globular clusters (GCs) in the 'ordinary' elliptical galaxy NGC 4494 using data from the Keck and Subaru telescopes. We derive galaxy surface brightness and colour profiles out to large galactocentric radii. We compare the latter to metallicities derived using the near-infrared Calcium Triplet. We obtain stellar kinematics out to ~3.5 effective radii.
Cone search capability for table J/MNRAS/415/3393/tablea1 (Individual values for NGC 4494 galaxy light)
Cone search capability for table J/MNRAS/415/3393/tablea2 (Individual spectroscopically confirmed globular clusters and Ultra-Compact Dwarfs around NGC 4494)
Cone search capability for table J/MNRAS/415/3393/table3 (Catalog of photometrically selected globular cluster candidates with i0<24)
Cone search capability for table J/MNRAS/415/3393/table4 (List of spectroscopically identified contaminants and non-globular cluster fillers)