New Exponential and Polynomial $\xi$-attractors

We introduce a new family of cosmological attractors with non-minimal coupling of gravity and non-canonical kinetic terms. In the Einstein frame, these models transform into a class of exponential and polynomial attractors with the spectral index $n_s$ spanning a broad range $1-2\mathrm{/}N\le n_s<1-1\mathrm{/}N$, and $r$ can decrease to zero in the limit $\xi \to \mathrm{\infty }$. This is sufficient to match any combination of Planck, BICEP/Keck, ACT, SPT, and DESI data. We present a supergravity implementation of these models.