This paper presents the chemical abundance analysis of a sample of 27 red giant stars located in four populous intermediate-age globular clusters in the Large Magellanic Cloud, namely NGC 1651, 1783, 1978, and 2173. This analysis is based on high-resolution (R~47000) spectra obtained with the UVES@VLT spectrograph. For each cluster we derived up to 20 abundance ratios sampling the main chemical elemental groups, namely light odd-Z, {alpha} iron-peak, and neutron-capture elements.

Cone search capability for table J/AJ/136/375/stars (The stars studied: atmospheric parameters and abundances)

Cone search capability for table J/AJ/136/375/photcat (Photometric catalog of clusters NGC 1651 (table n1651), NGC 1783 (table n1783), NGC 1978 (table new1978), and NGC 2173 (table n2173))