  We use a combination of Planck cosmic microwave background (CMB) anisotropy
data and non-CMB data that include Pantheon+ type Ia supernovae, Hubble
parameter [$H(z)$], growth factor ($f\sigma_8$) measurements, and a collection
of baryon acoustic oscillation (BAO) data, but not recent DESI 2024 BAO
measurements, to confirm the DESI 2024 (DESI+CMB+PantheonPlus) data compilation
support for dynamical dark energy with an evolving equation of state parameter
$w(z) = w_0 + w_a z/(1+z)$. From our joint compilation of CMB and non-CMB data,
in a spatially-flat cosmological model, we obtain $w_0 = -0.850 \pm 0.059$ and
$w_a = -0.59^{+0.26}_{-0.22}$ and find that this dynamical dark energy is
favored over a cosmological constant by $\sim 2\sigma$. Our data constraints on
the flat $w_0w_a$CDM model are slightly more restrictive than the DESI 2024
constraints, with the DESI 2024 and our values of $w_0$ and $w_a$ differing by
$-0.27\sigma$ and $0.44\sigma$, respectively. Our data compilation slightly
more strongly favors the flat $w_0w_a$CDM model over the flat $\Lambda$CDM
model than does the DESI 2024 data compilation.
