Landing-gear noise is predicted by conducting a Detached-Eddy Simulation of the turbulent region, and extrapolating the sound to the far field using the Ffowcs-WilliamsHawkings (FWH) equation. We use the Rudimentary Landing Gear (RLG), as well as two simpler configurations. Our past results conflicted with expectations based on Curle's approximation. Even at Mach numbers near 0.1, the sound attributed to surface pressure fluctuations ("S" sound) did not agree with the sound predicted with a permeable FWH surface ("P" sound). There was an apparent "quadrupole effect." We cautiously published this finding. In further work, we have found that it is not numerically robust at the level of grid resolution we had, of the order of 18 million points for the full RLG. Specifically, the P and the S results as well as their difference decrease tangibly when some measure of upwind differencing and thus numerical dissipation is introduced in the turbulent region; this brings results close to Curle's prediction (experimental comparisons are not presented). This is although the flow field obtained with minimal numerical dissipation is free of oscillations or spectral anomalies, and appears to represent a better simulation; upwind differencing smooths out the solution. In addition, for the simpler case of an isolated axle, simulations with finer grids by a factor of 2 and then 4 in each direction also produce lower noise and weaker apparent quadrupole content, even though they contain more small-scale turbulence. We discuss this troublesome disconnect between accepted criteria for the quality of a Large-Eddy Simulation, on one hand, and the noise predicted in the far field, on the other hand. In Appendices we discuss the detailed implications of theory regarding Mach-number scaling and relevant experimental findings, in preparation for later noise comparisons, and an independent verification of our FWH code.