  This manuscript revisits the phenomenological emergent dark energy model
(PEDE) by confronting it with recent cosmological data from early and late
times. In particular we analyze PEDE model by using the baryon acoustic
oscillation (BAO) measurements coming from both Dark Energy Spectroscopy
Instrument (DESI) data release 1 and Sloan Digital Sky Survey (SDSS).
Additionally, the measurements from cosmic chronometers, supernovae type Ia
(Pantheon+), quasars, hydrogen II galaxies and cosmic background radiation
distance priors are considered. By performing a Bayesian analysis based on
Monte Carlo Markov Chain, we find consistent results on the constraints when
SDSS and DESI are considered. However, we find higher values on the Hubble
constant than Supernova $H_0$ for the Equation of State (SH0ES) does although
it is still in agreement, within $1\sigma$ confidence level, when BAO
measurements are added. Furthermore, we estimate the age of the Universe
younger $\sim3\%$ than the one predicted by the standard cosmology.
Additionally, we report values of $q_0 = -0.771^{+0.007}_{-0.007}$, $z_T =
0.764^{+0.011}_{-0.011}$ for the deceleration parameter today and the
deceleration-acceleration transition redshift, respectively.
