Approximate 40 × 40 arcminute field of view showing the nova super-remnant around LMCN 1971-08a seen across different surveys and wavebands. The location of the nova is indicated with the cyan cross in each panel. The top row shows the surroundings of the nova in MCELS continuum-subtracted Hα, [S II] and [O III] data, with the NSR apparent in Hα and [S II] but negligible in [O III]. The bright “stars” in the MCELS images are points of oversubtraction from saturated stars. The left panel on the bottom row showing MeerKAT data does not clearly reveal a corresponding structure. The middle and right panels in the bottom row show data cube slices at ∼294 km s⁻¹ and ∼314 km s⁻¹, respectively, from the HI4PI survey, with potential evidence for the same northeast (in the 314 km s⁻¹ panel) and southwest (in the 294 km s⁻¹ panel) components of the NSR seen in the optical.