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

Sandro Tacchella, Charlie Conroy, S. M. Faber, Benjamin D. Johnson, Joel Leja, Guillermo Barro, Emily C. Cunningham, Alis J. Deason, Puragra Guhathakurta, Yicheng Guo, Lars Hernquist, David C. Koo, Kevin McKinnon, Constance M. Rockosi, Joshua S. Speagle, Pieter Van Dokkum, Hassen M. Yesuf

Research output: Contribution to journalArticlepeer-review

75 Scopus citations

Abstract

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 > 2 × 1011 M) galaxies formed the earliest (formation redshift of z f ≈ 5-10 with a short star formation timescale of τ SF ≥2 1 Gyr), lower-mass galaxies have a wide range of formation redshifts, leading to only a weak trend of z f with M. Interestingly, several low-mass galaxies have formation redshifts of z f ≈ 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 (τ quench ≈ 0-5 Gyr) with a median of τquench=1.0-0.9+0.8Gyr and of quenching epochs of z quench ≈ 0.8-5.0 (zquench=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.

Original languageEnglish (US)
Article number134
JournalAstrophysical Journal
Volume926
Issue number2
DOIs
StatePublished - Feb 1 2022

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Fast, Slow, Early, Late: Quenching Massive Galaxies at z ∼0.8'. Together they form a unique fingerprint.

Cite this