Photometric detection at $7.7\mu \mathrm{m}$ of a galaxy beyond redshift $14$ with JWST/MIRI

Abstract

The James Webb Space Telescope (JWST) has spectroscopically confirmed numerous galaxies at $z>10$. While weak rest-ultraviolet emission lines have only been seen in a handful of sources, the stronger rest-optical emission lines are highly diagnostic and accessible at mid-infrared wavelengths with the Mid-Infrared Instrument (MIRI) of JWST. We report the photometric detection of the distant spectroscopically confirmed galaxy JADES-GS-z14-0 at $z=14.32_{-0.20}^{+0.08}$ with MIRI at $7.7\mu \mathrm{m}$. The most plausible solution for the stellar population properties is that this galaxy contains half a billion solar masses in stars with a strong burst of star formation in the most recent few million years. For this model, at least one-third of the flux at $7.7\mu \mathrm{m}$ comes from the rest-optical emission lines $\mathrm{H}\beta$ and/or $[\mathrm{OIII}]\lambda \lambda 4959,5007$. The inferred properties of JADES-GS-z14-0 suggest rapid mass assembly and metal enrichment during the earliest phases of galaxy formation. This work demonstrates the unique power of mid-infrared observations in understanding galaxies at the redshift frontier.

arXiv commentSubmitted; main text has 5 pages, 3 figures and 1 table; extended text has 9 pages, 5 figures, and 2 tables

References in corpus (53)

• SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
• Array Programming with NumPy
• Astropy: A Community Python Package for Astronomy
• The NumPy array: a structure for efficient numerical computation
• Stellar population synthesis at the resolution of 2003
• The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
• Star Formation in Galaxies Along the Hubble Sequence
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• Modules for Experiments in Stellar Astrophysics (MESA)
• PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
• Gaia Data Release 3: Summary of the content and survey properties
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
• MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
• Detailed Structural Decomposition of Galaxy Images
• dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
• Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions
• MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones
• The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
• Detailed Decomposition of Galaxy Images. II. Beyond Axisymmetric Models
• The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging
• The propagation of uncertainties in stellar population synthesis modeling III: model calibration, comparison, and evaluation
• A Study of the Gas-Star Formation Relation over Cosmic Time
• The Hubble Ultra Deep Field
• Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms
• An updated MILES stellar library and stellar population models
• Stellar Population Inference with Prospector
• A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch
• CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST
• An updated analytic model for the attenuation by the intergalactic medium
• The Science Performance of JWST as Characterized in Commissioning
• Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
• Nebular Continuum and Line Emission in Stellar Population Synthesis Models
• Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15
• The Main Sequence of star-forming galaxies across cosmic times
• Identification and properties of intense star-forming galaxies at redshifts z>10
• On the mass function of star clusters
• Spectroscopic confirmation of two luminous galaxies at $z\sim 14$
• A JWST/NIRCam Study of Key Contributors to Reionization: The Star-forming and Ionizing Properties of UV-faint $z\sim 7-8$ Galaxies
• The Universe at z>10: Predictions for JWST from the UniverseMachine DR1
• Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
• UNCOVER: Illuminating the Early Universe -- JWST/NIRSpec Confirmation of $z>12$ Galaxies
• The MillenniumTNG Project: The galaxy population at $z\ge 8$
• AGN Selection and Demographics: A New Age with JWST/MIRI
• Templates for Fitting Photometry of Ultra-High-Redshift Galaxies
• First Light And Reionisation Epoch Simulations (FLARES) V: The redshift frontier
• Impact of the cosmic background radiation on the initial mass function of metal-poor stars
• A luminous and young galaxy at z=12.33 revealed by a JWST/MIRI detection of Hα and [OIII]
• MIDIS: Strong (Hb + [OIII]) and Ha emitters at redshift $z\simeq 7-8$ unveiled with JWST/NIRCam and MIRI imaging in the Hubble eXtreme Deep Field (XDF)
• The quantum efficiency and diffractive image artifacts of Si:As IBC mid-IR detector arrays at 5 $-$ 10 $\mu$m: Implications for the JWST/MIRI detectors
• The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release
• JADES Data Release 3 -- NIRSpec/MSA spectroscopy for 4,000 galaxies in the GOODS fields
• First Light And Reionisation Epoch Simulations (FLARES) XI: [OIII] emitting galaxies at $5<z<10$

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