Observations were carried out in visitor mode with FLAMES mounted at UT2 of ESO-VLT on 2014 December 11-13 (Program 094.D-0363(A)). Spectra were collected with the scientific aim of inferring Li and Al abundances for large samples of RGB stars, below and above the RGB bump luminosity, in several GCs, as part of our dedicated survey (see Paper I, D'Orazi et al., 2014ApJ...791...39D). (1 data file).