  We study the lensing phenomena of the strong gravity regime of the
five-dimensional charged, equally rotating black holes with a cosmological
constant, familiarly known as the Cveti\v c-L\"u-Pope black holes. These black
holes are characterized by three observable parameters, the mass $M$, the
charge $Q$ and the angular momentum $J$, in addition to the cosmological
constant. We investigate the strong gravitational lensing observables, mainly
the photon sphere radius, the minimum impact parameter, the deflection angle,
the angular size, and the magnification of the relativistic images. We model
the $M87$ and $SgrA^*$ for these observables. We also focus on the relativistic
time delay effect in the strong field regime of gravity and the impact of the
observable on it. The analytical expressions for the observables of the
relativistic images with vanishing angular momentum ($j=0$) are discussed in
some detail.
