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

Abstract

We investigate the stellar populations for a sample of 161 massive, mainly quiescent galaxies at $⟨z_{\mathrm{obs}}⟩=0.8$ 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 non-parametric star-formation histories, emission lines, variable dust attenuation law, and dust and AGN 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 ($M_{\star }>2\times 10^{11}{M}_{\odot }$) galaxies formed the earliest (formation redshift of $z_{\mathrm{f}}\approx 5-10$ with a short star-formation timescale of ${\tau }_{\mathrm{SF}}\lesssim 1\mathrm{Gyr}$), lower-mass galaxies have a wide range of formation redshifts, leading to only a weak trend of $z_{\mathrm{f}}$ with $M_{\star }$. Interestingly, several low-mass galaxies with have formation redshifts of $z_{\mathrm{f}}\approx 5-8$. 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 (${\tau }_{\mathrm{quench}}\approx 0-5\mathrm{Gyr}$) with a median of $⟨{\tau }_{\mathrm{quench}}⟩=1.0_{-0.9}^{+0.8}\mathrm{Gyr}$ and of quenching epochs of $z_{\mathrm{quench}}\approx 0.8-5.0$ ($⟨z_{\mathrm{quench}}⟩=1.3_{-0.4}^{+0.7}$). 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 & quench" framework and is consistent with a wide and continuously-populated diversity of quenching timescales.

arXiv comment30 pages, 12 figures + appendix, accepted by ApJ

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• DIGS: Deep Inference of Galaxy Spectra with Neural Posterior Estimation
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters: I. Ages of Quiescent Member Galaxies at 0.3 < z < 1.4
• A new perspective on the stellar Mass-Metallicity Relation of quiescent galaxies from the LEGA-C survey
• CLEAR: The Morphological Evolution of Galaxies in the Green Valley
• Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
• Neural Stellar Population Synthesis Emulator for the DESI PROVABGS
• Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim 9-17$
• DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at $z\sim 1$
• New JWST redshifts for the host galaxies of CDF-S XT1 and XT2: understanding their nature
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z\simeq 1$
• The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
• The physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies
• Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
• Ageing and Quenching through the ageing diagram II: physical characterization of galaxies
• Simulation-based inference of galaxy properties from JWST pixels
• The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
• COOL-LAMPS II. Characterizing the Size and Star Formation History of a Bright Strongly Lensed Early-Type Galaxy at Redshift 1.02
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• SQuIGG$\vec{L}$E: Observational Evidence of Low Ongoing Star Formation Rates in Gas-Rich Post-Starburst Galaxies
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
• The Dwarf Galaxy Population at $z\sim 0.7$: A Catalog of Emission Lines and Redshifts from Deep Keck Observations
• The Neon Gap: Probing Ionization with Dwarf Galaxies at z~1
• A census of quiescent galaxies across $0.5<z<8$ with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe
• Feeding the Dead: Neutral Gas Inflow in a Long-Quenched Ancient Massive Galaxy at $z\sim 2.7$ Observed with JWST/NIRSpec
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Extreme Neutral Outflow in a non-AGN Quiescent Galaxy at z~1.3
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
• Binary neutron star merger offsets from their host galaxies II. Short-duration gamma-ray bursts
• TP-AGB stars and stellar population properties of a post-starburst galaxy at $z\sim 2$ through optical and NIR spectroscopy with JWST
• Modelling the photometric and morphological evolution of disc galaxies in the cluster environment
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• LEGA-C stellar populations scaling relations. I: Chemo-archaeological downsizing trends at z~0.7
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon
• The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim 1$
• MIDIS: Unveiling the Star Formation History in massive galaxies at $1<z<4.5$ with spectro-photometric analysis
• Reconstructing the Assembly of Massive Galaxies. III: Quiescent Galaxies Loose Angular Momentum as They Evolve in a Mass-dependent Fashion
• From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?
• pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• The Photometric Analysis of the Environment Around Two Dusty Star-Forming Galaxies at $z\sim 2$
• Model-Independent Inference of Galaxy Star Formation Histories in the Local Volume
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Ageing and Quenching: Influence of Galaxy Environment and Nuclear Activity in Transition Stage
• On the hosts of neutron star mergers in the nearby Universe