Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors

Abstract

We report two secure ($z=3.775,4.012$) and one tentative ($z\approx 3.767$) spectroscopic confirmations of massive and quiescent galaxies through $K$-band observations with Keck/MOSFIRE and VLT/X-Shooter. The stellar continuum emission, the absence of strong nebular emission lines and the lack of significant far-infrared detections confirm the passive nature of these objects, disfavoring the alternative solution of low-redshift dusty star-forming interlopers. We derive stellar masses of $\log (M_{\star }/M_{\odot })\sim 11$ and ongoing star formation rates placing these galaxies $\gtrsim 1-2$ dex below the main sequence at their redshifts. The adopted parametrization of the star formation history suggests that these sources experienced a strong ($⟨\mathrm{SFR}⟩\sim 1200-3500{\mathrm{M}}_{\odot }{\mathrm{yr}}^{-1}$) and short ($\sim 50$ Myr) burst of star formation, peaking $\sim 150-500$ Myr before the time of observation, all properties reminiscent of the characteristics of sub-millimeter galaxies (SMGs) at $z>4$. We investigate this connection by comparing the comoving number densities and the properties of these two populations. We find a fair agreement only with the deepest sub-mm surveys detecting not only the most extreme starbursts, but also more normal galaxies. We support these findings by further exploring the Illustris-TNG cosmological simulation, retrieving populations of both fully quenched massive galaxies at $z\sim 3-4$ and SMGs at $z\sim 4-5$, with number densities and properties in agreement with the observations at $z\sim 3$, but in increasing tension at higher redshift. Nevertheless, as suggested by the observations, not all the progenitors of quiescent galaxies at these redshifts shine as bright SMGs in their past and, similarly, not all bright SMGs quench by $z\sim 3$, both fractions depending on the threshold assumed to define the SMGs themselves.

20 pages (+appendix), 11 figures, accepted for publication in the Astrophysical Journal (ApJ). This work comes with a companion letter by Tanaka, Valentino, Toft et al. 2019, ApJL, 885, L34

References in corpus (45)

• The UKIRT Infrared Deep Sky Survey (UKIDSS)
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• The Cosmic Evolution Survey (COSMOS) -- Overview
• EAZY: A Fast, Public Photometric Redshift Code
• Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions
• Properties of galaxies reproduced by a hydrodynamic simulation
• A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
• Detection of quiescent galaxies in a bicolor sequence from z=0-2
• The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
• UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
• Compaction and Quenching of High-z Galaxies in Cosmological Simulations: Blue and Red Nuggets
• An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling
• The SCUBA-2 Cosmology Legacy Survey: 850um maps, catalogues and number counts
• The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs
• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: High resolution 870um source counts
• An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies
• The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation
• The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation
• A dominant population of optically invisible massive galaxies in the early Universe
• Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution, and implications for the IMF
• Radio imaging of the Subaru/XMM-Newton Deep Field - I. The 100-microJy catalogue, optical identifications, and the nature of the faint radio source population
• Photometric Redshift with Bayesian Priors on Physical Properties of Galaxies
• The Assembly Histories of Quiescent Galaxies Since z=0.7 from Absorption Line Spectroscopy
• An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: Spectroscopic redshifts
• Red & Dead CANDELS: massive passive galaxies at the dawn of the Universe
• How to distinguish starbursts and quiescently star-forming galaxies: The `bimodal' submillimetre galaxy population as a case study
• The space density of luminous dusty star-forming galaxies at $z>4$: SCUBA-2 and LABOCA imaging of ultrared galaxies from $Herschel$-ATLAS
• Exploring the z=3-4 massive galaxy population with ZFOURGE: the prevalence of dusty and quiescent galaxies
• An Extremely Massive Quiescent Galaxy at $z=3.493$: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models
• MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. I - Evolution of Structural and Dynamical Properties
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$ VI: Redshift and emission-line catalog and basic properties of star-forming galaxies
• Determining the stellar masses of submillimetre galaxies: the critical importance of star formation histories
• MOSFIRE Absorption Line Spectroscopy of z > 2 Quiescent Galaxies: Probing a Period of Rapid Size Growth
• Stellar Velocity Dispersion of a Massive Quenching Galaxy at z=4.01
• An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution
• An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
• Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
• Physical properties of z>4 submillimeter galaxies in the COSMOS field
• Massive and old quiescent galaxies at high redshift
• X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim 2$
• An alternate approach to measure specific star formation rates at 2<z<7
• Passive galaxies in the early Universe: ALMA confirmation of z~3-5 candidates in the CANDELS GOODS-South field
• Compact Star-Forming Galaxies as Old Starbursts Becoming Quiescent

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• GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
• Stellar Velocity Dispersion of a Massive Quenching Galaxy at z=4.01
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• The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>1
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• COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at $0<z<5$ Revealed by X-ray and Radio Stacking
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• The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z=3-5 over 17.5 deg^2 in the SHELA Field
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• The GOGREEN Survey: Constraining the Satellite Quenching Timescale in Massive Clusters at $\mathbf{z}\gtrsim 1$
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
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• Illuminating the Dark Side of Cosmic Star Formation III: Building the largest homogeneous sample of Radio-Selected Dusty Star-Forming Galaxies in COSMOS with PhoEBO
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