(1) and (2) were taken into account. Lacking the crucial density dependence and also the ingredient (3), one cannot confront the Harada-Sasaki spectral function with the experimental data even if one had at one’s disposal a reliable evolution code – which one does not – and a reliable control on the experimental conditions. Even so, the analysis of Harada and Sasaki gives a clear indication as to what the dileptons might be “seeing" in hot and dense medium. First of all, mass shifts in the TSF cannot occur without the intrinsic background dependence (IBD) taken into account: Hadronic (thermal and dense) quantum (loop) corrections can broaden the spectra but do not shift the invariant mass. Next as a consequence of the IBD, a finite temperature and density take the parameter $a$ away from the vector dominance point $a=2$ which is sitting on an unstable trajectory and makes the VD violated, maximally at the VM fixed point with $a=1$. Lepton pairs will be produced more or less equally from the pions by direct coupling and through vector mesons, thereby modifying the spectral structure from that in which vector dominance is assumed, a procedure which is practiced in the field. The HLS/VM 