Notes. Column (1): lensed galaxy names as reported in the paper, with other common names in parentheses. Column (2): spectroscopic redshifts from the literature. Column (3): coordinates of the lensed sources (RA and Dec). Columns (4) and (5): magnification factors and stellar masses, with nominal correction from a Chabrier to a Salpeter IMF when required, from Jones et al. (2013, J1038), Shirazi et al. (2014, J0022), Saintonge et al. (2013, J1343), Johnson et al. (2017, J1110), Kostrzewa-Rutkowska et al. (2014, J0143). For J1038, J0022 and J1110 we specifically refer to the A2 knot measurements, as reported in the aforementioned papers; all other values do not refer to individual images, but to the lensed galaxy. Stellar mass of J1958 from this work (see Sect. 8). All stellar masses are corrected for the lensing magnification factors reported in Col. (4). Column (6): SFR from the Hα flux corrected for extinction and lensing magnification using Kennicutt (1998) relation (J1958 and J1343 from Leethochawalit et al. 2016; J0022 from Shirazi et al. 2014, using the Hβ flux). Lensing-corrected SFR of J1110 from Johnson et al. (2017) and obtained by SED fitting analysis, nominally corrected from a Chabrier to a Salpeter IMF. Column (7): dates (MM/YY). Column (8): LUCI filters; for J0022, we used a clear filter to detect Hα line redshifted at ∼2.45 μm. Column (9): curved slit width. Column (10): time on target. Column (11): seeing as measured by the DIMM station. Column (12): spatial profile FWHM obtained integrating the reference star flux within a 100 px interval along the x-axis. Column (13): estimate of the spatial resolution in the source plane. For J1038, J0022 and J1110 we refer to the A2 knots, using the magnifications derived by Jones et al. (2013), Shirazi et al. (2014) and Johnson et al. (2017), respectively.