Projected distribution of Dorado galaxy members according to Firth et al. (2006) and Kourkchi & Tully (2017). Members are labelled according to their morphology and B-Band magnitude provided by HyperLeda. UVIT FUV.CaF2 fields listed in Table 1 are enclosed by a light-green circle that has the diameter of the UVIT field (28′). Target galaxies within each field are also labelled. The morphological, photometric, and star-forming properties obtained from the UVIT FUV.CaF2 data set about NGC 1533, and IC 2038 and IC 2039, shown as dark-grey circles in the figure, have been presented and discussed in Ram2021. Ram2020 also observed NGC 1581 and NGC 1543 in Hα+[N II]. All galaxies except NGC 1596 and NGC 1602 have been already observed with GALEX at lower resolution and sensitivity (see e.g., Marino et al. 2011a,b).