Motivic Telescope Conjecture in telescopic form

Let $X$ be a finite motivic spectrum of type $(m,n)$ with a non-nilpotent self-map $v:\Sigma^{-r,-s}X\to X$ of type $(m,n)$. Write $\langle E\rangle$ for the Bousfield class of a motivic spectrum $E$, and $v^{-1}X$ for the telescope of $v$. Motivic Telescope Conjecture. The Bousfield class $\langle v^{-1}X\rangle$ depends only on $m$ and $n$, and

$$\langle v^{-1}X\rangle=\langle K(\beta_{ij})\rangle.$$

This is the telescopic formulation of the motivic Telescope Conjecture; its relationship with the localization and smashing formulations depends on further conjectural smashing and localization properties.