Resolve closely located sources accurately with LEAP (S/N = 20 dB, source separation: 1′30′′, antenna layout: 24 LOFAR core stations, background: CLEAN image). Panel a: LEAP reconstruction. Panel b: CLEAN image from the same set of visibility measurements. Panel c: CLEAN image from additional visibilities with higher time resolution (8.01 s between adjacent integration times) and longer baselines (56 LOFAR core and remote stations). The setup in (c) with longer baselines reduces the telescope angular resolution to 6.10′′.