CEERS Key Paper III: The Diversity of Galaxy Structure and Morphology at z=3-9 with JWST
arXiv:2210.14713 · doi:10.3847/2041-8213/acad01
Abstract
We present a comprehensive analysis of the evolution of the morphological and structural properties of a large sample of galaxies at z=3-9 using early JWST CEERS NIRCam observations. Our sample consists of 850 galaxies at z>3 detected in both CANDELS HST imaging and JWST CEERS NIRCam images to enable a comparison of HST and JWST morphologies. Our team conducted a set of visual classifications, with each galaxy in the sample classified by three different individuals. We also measure quantitative morphologies using the publicly available codes across all seven NIRCam filters. Using these measurements, we present the fraction of galaxies of each morphological type as a function of redshift. Overall, we find that galaxies at z>3 have a wide diversity of morphologies. Galaxies with disks make up a total of 60\% of galaxies at z=3 and this fraction drops to ~30% at z=6-9, while galaxies with spheroids make up ~30-40% across the whole redshift range and pure spheroids with no evidence for disks or irregular features make up ~20%. The fraction of galaxies with irregular features is roughly constant at all redshifts (~40-50%), while those that are purely irregular increases from ~12% to ~20% at z>4.5. We note that these are apparent fractions as many selection effects impact the visibility of morphological features at high redshift. The distributions of Sérsic index, size, and axis ratios show significant differences between the morphological groups. Spheroid Only galaxies have a higher Sérsic index, smaller size, and higher axis ratio than Disk/Irregular galaxies. Across all redshifts, smaller spheroid and disk galaxies tend to be rounder. Overall, these trends suggest that galaxies with established disks and spheroids exist across the full redshift range of this study and further work with large samples at higher redshift is needed to quantify when these features first formed.
Accepted for publication to ApJL, 24 pages, 14 figures
References in corpus (17)
- Cosmic Star Formation History
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since
- The All-wavelength Extended Groth Strip International Survey (AEGIS) Data Sets
- The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8
- Galaxy Merger Morphologies and Time-Scales from Simulations of Equal-Mass Gas-Rich Disc Mergers
- Evidence for Mature Bulges and an Inside-out Quenching Phase 3 Billion Years After the Big Bang
- The Morphological Diversities Among Star-forming Galaxies at High Redshifts in the Great Observatories Origins Deep Survey (GOODS)
- Non-parametric Star Formation History Reconstruction with Gaussian Processes I: Counting Major Episodes of Star Formation
- Panic! At the Disks: First Rest-frame Optical Observations of Galaxy Structure at with JWST in the SMACS 0723 Field
- The shapes of galaxies in the Sloan Digital Sky Survey
- Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
- Mock Lightcones and Theory Friendly Catalogs for the CANDELS Survey
- Optimized Photometric Redshifts for the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey (CANDELS)
- Galapagos-2/Galfitm/GAMA -- multi-wavelength measurement of galaxy structure: separating the properties of spheroid and disk components in modern surveys
- MegaMorph: classifying galaxy morphology using multi-wavelength Sérsic profile fits
- Identifying Galaxy Mergers in Simulated CEERS NIRCam Images using Random Forests
Cited by in corpus (71)
- JADES Imaging of GN-z11: Revealing the Morphology and Environment of a Luminous Galaxy 430 Myr After the Big Bang
- RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec
- CEERS Key Paper IV: Galaxies at are Bluer than They Appear -- Characterizing Galaxy Stellar Populations from Rest-Frame micron Imaging
- A Milky Way-like barred spiral galaxy at a redshift of 3
- A Large Population of Faint 8<z<16 Galaxies Found in the First JWST NIRCam Observations of the NGDEEP Survey
- The ALMA-ALPAKA survey I: high-resolution CO and [CI] kinematics of star-forming galaxies at z = 0.5-3.5
- Dynamically cold disks in the early Universe: myth or reality?
- ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields
- Sub-Millimetre Galaxies with Webb: Near-Infrared Counterparts and Multi-wavelength Morphology
- Discovery of the local counterpart of disc galaxies at z > 4: The oldest thin disc of the Milky Way using Gaia-RVS
- JWST/CEERS sheds light on dusty star-forming galaxies: forming bulges, lopsidedness and outside-in quenching at cosmic noon
- SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
- Uncovering the stellar structure of the dusty star-forming galaxy GN20 at z=4.055 with MIRI/JWST
- The evolution of the SFR and Sigma-SFR of galaxies in cosmic morning (4 < z < 10)
- The formation and survival of the Milky Way's oldest stellar disk
- A Robust Study of High-Redshift Galaxies: Unsupervised Machine Learning for Characterising morphology with JWST up to z ~ 8
- Redshifting galaxies from DESI to JWST CEERS: Correction of biases and uncertainties in quantifying morphology
- Galaxy morphologies at cosmic noon with JWST: A foundation for exploring gas transport with bars and spiral arms
- Rest-Frame Near-Infrared Radial Light Profiles up to z=3 from JWST/NIRCam: Wavelength Dependence of the Sérsic Index
- Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
- The robustness in identifying and quantifying high-redshift bars using JWST observations
- PANORAMIC: Discovery of an Ultra-Massive Grand-Design Spiral Galaxy at
- Dynamical modelling and origin of gas turbulence in z 4.5 galaxies
- GA-NIFS: A galaxy-wide outflow in a Compton-thick mini-BAL quasar at z = 3.5 probed in emission and absorption
- The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6
- First Light And Reionisation Epoch Simulations (FLARES) XI: [OIII] emitting galaxies at
- The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe
- JWST reveals a high fraction of disk breaks at
- COSMOS-Web: The emergence of the Hubble Sequence
- Exploring Spatially-Resolved Metallicities, Dynamics and Outflows in Low-Mass Galaxies at
- JWST/MIRI unveils the stellar component of the GN20 dusty galaxy overdensity at =4.05
- MIDIS. Near-infrared rest-frame morphology of massive galaxies at in the Hubble eXtreme Deep Field
- Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
- Deciphering the Milky Way disc formation time encrypted in the bar chrono-kinematics
- The JWST Emission Line Survey (JELS): Extending rest-optical narrow-band emission line selection into the Epoch of Reionization
- Cloud-cloud collisions triggering star formation in galaxy simulations
- The PSF Smoothing Effect on Concentration-Related Parameters of High Redshift Galaxies in HST and JWST
- The diverse physical origins of stars in the dynamically hot bulge: CALIFA vs. IllustrisTNG
- The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ~ 5.5
- A grand-design spiral galaxy 1.5 billion years after the Big Bang with JWST
- Galaxy Zoo JWST: Up to 75% of discs are featureless at
- Turbulent gas-rich discs at high redshift: origin of thick stellar discs through 3D 'baryon sloshing'
- Cosmic Stillness: High Quiescent Galaxy Fractions Across Upper Mass Scales in the Early Universe to z = 7 with JWST
- JWST Discovery of a High-Redshift Tidal Disruption Event Candidate in COSMOS-Web
- Through Thick and Thin: The Cosmic Evolution of Disk Scale Height
- Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
- Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
- On the kinematic nature of apparent discs at high redshifts: Local counterparts are not dominated by ordered rotation but by tangentially anisotropic random motion
- The AGORA High-resolution Galaxy Simulations Comparison Project. VIII: Disk Formation and Evolution of Simulated Milky Way Mass Galaxy Progenitors at
- An efficient unsupervised classification model for galaxy morphology: Voting clustering based on coding from ConvNeXt large model
- A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn
- Distinguishing the formation paths of massive compact ETGs through their internal dynamical structures
- Morphological evolution of disk galaxies and their concentration, asymmetry and clumpiness (CAS) properties in simulations across Toomre's parameter
- Amaryllis: a digital twin of the earliest galaxies in the Universe
- The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
- Cosmic wallflowers: the circumgalactic origins of isolated ultra-compact star clusters at
- Enhanced AGN Activity in Overdense Galactic Environments at
- Compact dust-obscured star-formation and the origin of the galaxy bimodality
- Modelling the photometric and morphological evolution of disc galaxies in the cluster environment
- ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey
- Discovery of a Lyα blob photo-ionised by a super-cluster of massive stars associated to a z = 3.49 galaxy
- Probing the influence of the protocluster environment on galaxy morphology at z = 2.23
- Discovery of a Barred-Spiral Galaxy at = 3.16 II. The Star Formation History
- Compact [OIII] emission-line regions ("Green Seeds") in emitters at Cosmic Noon from JWST Observations
- Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
- The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
- MIDIS: Quantifying the AGN component of X-ray-detected galaxies
- Euclid: Discovery of bright Lyman-break galaxies in UltraVISTA and Euclid COSMOS
- Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScience
- Morpho-kinematic of galaxies at cosmic noon
- Ergodicity of FIRE: star formation variations within and between simulated galaxies