Fast, Slow, Early, Late: Quenching Massive Galaxies at z similar to 0.8

We investigate the stellar populations for a sample of 161 massive, mainly quiescent galaxies at < z(obs)> = 0.8 with deep Keck/DEIMOS rest-frame optical spectroscopy (HALO7D survey). With the fully Bayesian framework Prospector, we simultaneously fit the spectroscopic and photometric data with an advanced physical model (including nonparametric star formation histories, emission lines, variable dust attenuation law, and dust and active galactic nucleus emission), together with an uncertainty and outlier model. We show that both spectroscopy and photometry are needed to break the dust-age-metallicity degeneracy. We find a large diversity of star formation histories: although the most massive (M-star > 2 x 10(11) M-circle dot) galaxies formed the earliest (formation redshift of z(f) approximate to 5-10 with a short star formation timescale of tau(SF) less than or similar to 1 Gyr), lower-mass galaxies have a wide range of formation redshifts, leading to only a weak trend of z(f) with M-star. Interestingly, several low-mass galaxies have formation redshifts of z(f) approximate to 5-8. Star-forming galaxies evolve about the star-forming main sequence, crossing the ridgeline several times in their past. Quiescent galaxies show a wide range and continuous distribution of quenching timescales (tau(quench) approximate to 0-5 Gyr) with a median of = 1.0(-0.9)(+0.8) Gyr z(quench) approximate to 0.8-5.0 (< z(quench)> =1.3(-0.4)(+0.7)). This large diversity of quenching timescales and epochs points toward a combination of internal and external quenching mechanisms. In our sample, rejuvenation and "late bloomers" are uncommon. In summary, our analysis supports the "grow-and-quench" framework and is consistent with a wide and continuously populated diversity of quenching timescales.