We investigate the age and metallicity distributions of bright globular clusters (GCs) in the candidate intermediate-age early-type galaxies NGC 3610, 584 and 3377 using a combination of new Gemini's Near InfraRed Imager and Spectrometer K'-band imaging and existing optical VI photometry from Hubble Space Telescope data.
Cone search capability for table J/MNRAS/420/1317/table4 (*Magnitudes, colors, photometric age, metallicity and mass of globular clusters in the three post-merger remnant galaxies corrected for foreground reddening)