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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. The V−I versus I−K′ colour–colour diagram is found to break the age–metallicity...
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