Two candidate (mini-)quenched galaxies in the protocluster, exhibiting strong Balmer breaks and very weak emission lines. Their model spectra and photometry (blue line and circles) and observed photometry (red squares) are shown in the left-hand panels, while their best-fit SFH (blue line) and associated uncertainty (shaded blue region) from PROSPECTOR are shown in the right-hand panels. The SFHs of these objects are best characterised by a sustained period of star formation, over more than 100 Myr, followed by a recent decline, over the last 10 Myr, which has reached SFR ∼ 0 M_⊙ yr⁻¹ by the time of observation. Both objects reside within the highly clustered regions of the protocluster providing a possible hint at the suppression of star formation within the innermost region.