CMB targets after the latest Planck data release

We show that a combination of the simplest $\alpha$-attractors and KKLTI models related to Dp-brane inflation covers most of the area in the ($n_s$, $r$) space favored by Planck 2018. For $\alpha$-attractor models, there are discrete targets $3\alpha =1,2,\mathrm{.}\mathrm{.}\mathrm{.},7$, predicting 7 different values of $r = 12\alpha/N^{2}$intherange$10^{-2} \gtrsim r \gtrsim 10^{-3}$\mathrm{.}Inthesmall$r$limit,$\alpha$-attractorsandDp-braneinflationmodelsdescribevertical$\beta$-stripesinthe($n_{s}$,$r$)space,with$n_{s}=1-\beta/N$,$\beta=2, {5\over 3},{8\over 5}, {3\over 2},{4\over 3}$. A phenomenological description of these models and their generalizations can be achieved in the context of pole inflation. Most of the $1\sigma$ area in the ($n_s$, $r$) space favored by Planck 2018 can be covered models with $\beta =2$ and $\beta =5\mathrm{/}3$. Future precision data on $n_s$ may help to discriminate between these models even if the precision of the measurement of $r$ is insufficient for the discovery of gravitational waves produced during inflation.