More spectroscopic evidence for (mini-)quenching at high redshift: The Lyα drop and the Balmer break of JADES-GS+53.16136-27.77803 clearly establish the redshift at z = 4.4. The absence of emission lines suggests that this galaxy is in a quiescent phase (which is likely only temporarily) and has not formed a significant amount of stellar mass over the last 10 Myr before the epoch of observation.