CEERS

CEERS Papers

We're excited to share with you results made possible by CEERS, both from our team members and other teams.

Publications from the CEERS team

Other publications using CEERS data

Publications from the CEERS team:

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• The ionizing photon production efficiency of star-forming galaxies at z~4-10, Llerena et al., 2024, arXiv, arXiv:2412.01358
• Evolution of the UV slope of galaxies at cosmic morning (z > 4): the properties of extremely blue galaxies, Dottorini et al., 2024, arXiv, arXiv:2412.01623
• CEERS Key Paper. IX. Identifying Galaxy Mergers in CEERS NIRCam Images Using Random Forests and Convolutional Neural Networks, Rose et al., 2024, ApJL, 976, L8
• ASTRODEEP-JWST: NIRCam-HST multi-band photometry and redshifts for half a million sources in six extragalactic deep fields, Merlin et al., 2024, A&A, 691, A240
• Physical properties of extreme emission-line galaxies at z ~ 4–9 from the JWST CEERS survey, Llerena et al., 2024, A&A, 691, A59
• Unveiling the Dark Side of UV/Optical Bright Galaxies: Optically Thick Dust Absorption, Cheng et al., 2024, arXiv, arXiv:2411.08100
• Strong spectral features from asymptotic giant branch stars in distant quiescent galaxies, Lu et al., 2024, NatAs.tmp,
• Evolution of the star formation rate and Σ_SFR of galaxies at cosmic morning (4 < z < 10), Calabrò et al., 2024, A&A, 690, A290
• A Census from JWST of Extreme Emission-line Galaxies Spanning the Epoch of Reionization in CEERS, Davis et al., 2024, ApJ, 974, 42
• Emission-line Ratios and Ionization Conditions of CEERS Star-forming Galaxies with JWST/NIRSpec, Gupta et al., 2024, RNAAS, 8, 266
• Compact dust-obscured star-formation and the origin of the galaxy bimodality, Tarrasse et al., 2024, arXiv, arXiv:2411.00279
• Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts, Brooks et al., 2024, arXiv, arXiv:2410.07340
• CEERS: Forging the First Dust -- Transition from Stellar to ISM Grain Growth in the Early Universe, Burgarella et al., 2024, arXiv, arXiv:2410.23959
• Spectroscopic confirmation of a dust-obscured, metal-rich dwarf galaxy at z~5, Bisigello et al., 2024, arXiv, arXiv:2410.10954
• A Search for z=5 H\alpha and H\beta+[O III] Dual-Line Emitting Galaxies in the JWST CEERS Field: Implications for the AGN Abundance, Guo et al., 2024, arXiv, arXiv:2409.19205
• Physical properties of strong 1 < z < 3 Balmer and Paschen line emitters observed with JWST, Seillé et al., 2024, A&A, 689, A102
• Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4–8 from CEERS, Chworowsky et al., 2024, AJ, 168, 113
• Broad-Line AGN at 3.5<z<6: The Black Hole Mass Function and a Connection with Little Red Dots, Taylor et al., 2024, arXiv, arXiv:2409.06772
• The Abundance and Properties of Barred Galaxies out to z~4 Using \textit{JWST} CEERS Data, Guo et al., 2024, arXiv, arXiv:2409.06100
• Characterizing the Average Interstellar Medium Conditions of Galaxies at z ~ 5.6–9 with Ultraviolet and Optical Nebular Lines, Hu et al., 2024, ApJ, 971, 21
• JWST/CEERS sheds light on dusty star-forming galaxies: Forming bulges, lopsidedness, and outside-in quenching at cosmic noon, Le Bail et al., 2024, A&A, 688, A53
• Peering into cosmic reionization: Lyα visibility evolution from galaxies at z = 4.5-8.5 with JWST, Napolitano et al., 2024, A&A, 688, A106
• The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5–14.5, Finkelstein et al., 2024, ApJL, 969, L2
• Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS, Long et al., 2024, ApJ, 970, 68
• CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI, Ronayne et al., 2024, ApJ, 970, 61
• Preliminary Evidence for Lensing-Induced Alignments of High-Redshift Galaxies in JWST-CEERS, Pandya et al., 2024, arXiv, arXiv:2407.17552
• New insight on the nature of cosmic reionizers from the CEERS survey, Mascia et al., 2024, A&A, 685, A3
• CEERS: Diversity of Lyα Emitters during the Epoch of Reionization, Jung et al., 2024, ApJ, 967, 73
• Galaxy morphology from z ~ 6 through the lens of JWST, Huertas-Company et al., 2024, A&A, 685, A48
• Cosmic evolution early release science survey (CEERS): multiclassing galactic dwarf stars in the deep JWST/NIRCam, Holwerda et al., 2024, MNRAS, 529, 1067
• The Rise of Faint, Red AGN at z>4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields, Kocevski et al., 2024, arXiv, arXiv:2404.03576
• Galaxies Going Bananas: Inferring the 3D Geometry of High-redshift Galaxies with JWST-CEERS, Pandya et al., 2024, ApJ, 963, 54
• Extremely Red Galaxies at z = 5–9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?, Barro et al., 2024, ApJ, 963, 128
• CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z > 2, Backhaus et al., 2024, ApJ, 962, 195
• Evolution of the Size–Mass Relation of Star-forming Galaxies Since z = 5.5 Revealed by CEERS, Ward et al., 2024, ApJ, 962, 176
• On the Nature of Disks at High Redshift Seen by JWST/CEERS with Contrastive Learning and Cosmological Simulations, Vega-Ferrero et al., 2024, ApJ, 961, 51
• CEERS Key Paper. VII. JWST/MIRI Reveals a Faint Population of Galaxies at Cosmic Noon Unseen by Spitzer, Kirkpatrick et al., 2023, ApJL, 959, L7
• CEERS: Increasing Scatter along the Star-Forming Main Sequence Indicates Early Galaxies Form in Bursts, Cole et al., 2023, arXiv, arXiv:2312.10152
• Near-infrared emission line diagnostics for AGN from the local Universe to z ~ 3, Calabrò et al., 2023, A&A, 679, A80
• A Milky Way-like barred spiral galaxy at a redshift of 3, Costantin et al., 2023, Natur, 623, 499
• Cosmic Evolution Early Release Science (CEERS) survey: The colour evolution of galaxies in the distant Universe, Wilkins et al., 2023, arXiv, arXiv:2311.08065
• Confirmation and refutation of very luminous galaxies in the early Universe, Arrabal Haro et al., 2023, Natur, 622, 707
• CEERS MIRI Imaging: Data Reduction and Quality Assessment, Yang et al., 2023, ApJL, 956, L12
• ALMA FIR View of Ultra-high-redshift Galaxy Candidates at z ~ 11-17: Blue Monsters or Low-z Red Interlopers?, Fujimoto et al., 2023, ApJ, 955, 130
• CEERS: MIRI deciphers the spatial distribution of dust-obscured star formation in galaxies at 0.1 < z < 2.5, Magnelli et al., 2023, A&A, 678, A83
• Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST, Akins et al., 2023, ApJ, 956, 61
• JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies, Gómez-Guijarro et al., 2023, A&A, 677, A34
• A z = 1.85 galaxy group in CEERS: Evolved, dustless, massive intra-halo light and a brightest group galaxy in the making, Coogan et al., 2023, A&A, 677, A3
• Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS, Kocevski et al., 2023, ApJL, 954, L4
• Delving deep: A population of extremely dusty dwarfs observed by JWST, Bisigello et al., 2023, A&A, 676, A76
• A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars, Larson et al., 2023, ApJL, 953, L29
• Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z ≃ 8-10, Arrabal Haro et al., 2023, ApJL, 951, L22
• CEERS Spectroscopic Confirmation of NIRCam-selected z ≳ 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of Their Properties, Fujimoto et al., 2023, ApJL, 949, L25
• CEERS Key Paper. VI. JWST/MIRI Uncovers a Large Population of Obscured AGN at High Redshifts, Yang et al., 2023, ApJL, 950, L5
• CEERS Key Paper. V. Galaxies at 4 < z < 9 Are Bluer than They Appear–Characterizing Galaxy Stellar Populations from Rest-frame ~ 1 μm Imaging, Papovich et al., 2023, ApJL, 949, L18
• CEERS: Spatially Resolved UV and Mid-infrared Star Formation in Galaxies at 0.2 < z < 2.5: The Picture from the Hubble and James Webb Space Telescopes, Shen et al., 2023, ApJ, 950, 7
• Selecting z~8 Galaxies with JWST Photometry in CEERS, Wang et al., 2023, RNAAS, 7, 109
• Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View, Costantin et al., 2023, ApJ, 946, 71
• First Look at z > 1 Bars in the Rest-frame Near-infrared with JWST Early CEERS Imaging, Guo et al., 2023, ApJL, 945, L10
• CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST, Kocevski et al., 2023, ApJL, 946, L14
• CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z = 3-9 with JWST, Kartaltepe et al., 2023, ApJL, 946, L15
• CEERS Key Paper. IV. A Triality in the Nature of HST-dark Galaxies, Pérez-González et al., 2023, ApJL, 946, L16
• CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results, Bagley et al., 2023, ApJL, 946, L12
• CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST, Finkelstein et al., 2023, ApJL, 946, L13
• The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations, Trump et al., 2023, ApJ, 945, 35
• Mock galaxy surveys for HST and JWST from the IllustrisTNG simulations, Snyder et al., 2023, MNRAS, 518, 6318
• Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations, Zavala et al., 2023, ApJL, 943, L9
• Probing the Earliest Phases in the Formation of Massive Galaxies with Simulated HST+JWST Imaging Data from Illustris, García-Argumánez et al., 2023, ApJ, 944, 3
• Identifying Galaxy Mergers in Simulated CEERS NIRCam Images Using Random Forests, Rose et al., 2023, ApJ, 942, 54
• New z > 7 Lyman-alpha Emitters in EGS: Evidence of an Extended Ionized Structure at z ~ 7.7, Jung et al., 2022, arXiv, arXiv:2212.09850
• A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging, Finkelstein et al., 2022, ApJL, 940, L55

Other publications using CEERS data

View as an ADS Library

(Papers listed here are the result of an ADS query for those with 'CEERS' in the abstract. If we're missing your paper and you would like us to add it here, please email Micaela Bagley [mbagley@utexas.edu]. We are happy to advertise your work!)

• Color profiles of disk galaxies at z=1-3 observed with JWST: Implications for outer-disk formation histories, Yu et al., 2024, arXiv, arXiv:2412.13064
• The Star-forming Main Sequence in JADES and CEERS at z > 1.4: Investigating the Burstiness of Star Formation, Clarke et al., 2024, ApJ, 977, 133
• Cosmic Stillness: High Quiescent Galaxy Fractions Across Upper Mass Scales in the Early Universe to z = 7 with JWST, Russell et al., 2024, arXiv, arXiv:2412.11861
• JWST/MIRI unveils the stellar component of the GN20 dusty galaxy overdensity at z = 4.05, Crespo Gómez et al., 2024, A&A, 691, A325
• A Galaxy with an Extremely Blue UV Slope β=-3 at z=9.25 Identified by JWST Spectroscopy: Evidence for a Weak Nebular Continuum and Efficient Ionizing Photon Escape?, Yanagisawa et al., 2024, arXiv, arXiv:2411.19893
• An Edge-on Regular Disk Galaxy at z = 5.289, Yan et al., 2024, ApJ, 975, 44
• Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at z = 4.5 - 8.5, Duan et al., 2024, arXiv, arXiv:2411.04944
• Galaxy Size and Mass Build-up in the First 2 Gyrs of Cosmic History from Multi-Wavelength JWST NIRCam Imaging, Allen et al., 2024, arXiv, arXiv:2410.16354
• Efficient Survey Design for Finding High-redshift Galaxies with JWST, Vujeva et al., 2024, ApJ, 974, 23
• JWST Reveals Bulge-dominated Star-forming Galaxies at Cosmic Noon, Benton et al., 2024, ApJL, 974, L28
• The Physical Origin of Extreme Emission Line Galaxies at High redshifts: Strong [Oiii] Emission Lines Produced by Obscured AGNs, Zhu et al., 2024, arXiv, arXiv:2410.12198
• Population synthesis and astrophysical inference for high-z JWST galaxies, Driskell et al., 2024, arXiv, arXiv:2410.11680
• Galaxy build-up in the first 1.5 Gyr of cosmic history: insights from the stellar mass function at z 4-9 from JWST NIRCam observations, Weibel et al., 2024, MNRAS, 533, 1808
• Fast-rotating massive Population III stars as possible sources of extreme N enrichment in high-redshift galaxies, Nandal et al., 2024, A&A, 688, A142
• The robustness in identifying and quantifying high-redshift bars using JWST observations, Liang et al., 2024, A&A, 688, A158
• JWST Measurements of Neutral Hydrogen Fractions and Ionized Bubble Sizes at z = 7–12 Obtained with Lyα Damping Wing Absorptions in 27 Bright Continuum Galaxies, Umeda et al., 2024, ApJ, 971, 124
• LIME: A LIne MEasuring library for large and complex spectroscopic data sets. I. Implementation of a virtual observatory for JWST spectra, Fernández et al., 2024, A&A, 688, A69
• Narrow line AGN selection in CEERS: spectroscopic selection, physical properties, X-ray and radio analysis, Mazzolari et al., 2024, arXiv, arXiv:2408.15615
• Unveiling the Cosmic Chemistry: Revisiting the Mass-Metallicity Relation with JWST/NIRSpec at 4 < z < 10, Sarkar et al., 2024, arXiv, arXiv:2408.07974
• Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies, Menci et al., 2024, JCAP, 2024, 072
• TRINITY IV: predictions for supermassive black holes at z ≳ 6, Zhang et al., 2024, MNRAS, 531, 4974
• Statistics for Galaxy Outflows at z ∼ 6–9 with Imaging and Spectroscopic Signatures Identified with JWST/NIRCam and NIRSpec Data, Zhang et al., 2024, ApJ, 970, 19
• Calibrating Nonparametric Morphological Indicators from JWST Images for Galaxies over 0.5 < z < 3, Ren et al., 2024, ApJ, 969, 4
• Finding dusty AGNs from the JWST CEERS survey with mid-infrared photometry, Chien et al., 2024, MNRAS, 532, 719
• EPOCHS Paper V. The dependence of galaxy formation on galaxy structure at z < 7 from JWST observations, Conselice et al., 2024, MNRAS, 531, 4857
• EPOCHS I. The Discovery and Star Forming Properties of Galaxies in the Epoch of Reionization at 6.5 < z < 18 with PEARLS and Public JWST data, Conselice et al., 2024, arXiv, arXiv:2407.14973
• A spectroscopic analysis of the ionizing photon production efficiency in JADES and CEERS: implications for the ionizing photon budget, Pahl et al., 2024, arXiv, arXiv:2407.03399
• Galaxy Mergers in the Epoch of Reionization I: A JWST Study of Pair Fractions, Merger Rates, and Stellar Mass Accretion Rates at z = 4.5-11.5, Duan et al., 2024, arXiv, arXiv:2407.09472
• The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope, Pallottini et al., 2024, arXiv, arXiv:2408.00061
• The PSF smoothing effect on concentration-related parameters of high-redshift galaxies in HST and JWST, Wang et al., 2024, A&A, 686, A100
• JWST Reveals a Surprisingly High Fraction of Galaxies Being Spiral-like at 0.5 ≤ z ≤ 4, Kuhn et al., 2024, ApJL, 968, L15
• Radio Emission from High-redshift Active Galactic Nuclei in the JADES and CEERS Surveys, Latif et al., 2024, AJ, 167, 251
• Exploring the AGN Fraction of a Sample of JWST's Little Red Dots at 5 < z < 8: Overmassive Black Holes Are Strongly Favored, Durodola et al., 2024, arXiv, arXiv:2406.10329
• A Steep Decline in the Galaxy Space Density beyond Redshift 9 in the CANUCS UV Luminosity Function, Willott et al., 2024, ApJ, 966, 74
• A JWST investigation into the bar fraction at redshifts 1 ≤ z ≤ 3, Le Conte et al., 2024, MNRAS, 530, 1984
• Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology, Lee et al., 2024, ApJ, 966, 113
• Tracing the rise of supermassive black holes. A panchromatic search for faint, unobscured quasars at z ≳ 6 with COSMOS-Web and other surveys, Andika et al., 2024, A&A, 685, A25
• Unveiling the hidden Universe with JWST: the contribution of dust-obscured galaxies to the stellar mass function at z 3 - 8, Gottumukkala et al., 2024, MNRAS, 530, 966
• EPOCHS Paper X: Environmental effects on Galaxy Formation and Protocluster Galaxy candidates at 4.5, Li et al., 2024, arXiv, arXiv:2405.17359
• Adding value to JWST spectra and photometry: stellar population and star formation properties of spectroscopically confirmed JADES and CEERS galaxies at z > 7, Duan et al., 2024, MNRAS, 529, 4728
• Insight from JWST/Near Infrared Camera into galaxy overdensities around bright Lyman-alpha emitters during reionization: implications for ionized bubbles at z 9, Whitler et al., 2024, MNRAS, 529, 855
• EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 < z < 13.5 Using 180 arcmin² of Deep, Blank Fields from the PEARLS Survey and Public JWST Data, Adams et al., 2024, ApJ, 965, 169
• Census for the rest-frame optical and UV morphologies of galaxies at z = 4-10: First phase of inside-out galaxy formation, Ono et al., 2024, PASJ, 76, 219
• EPOCHS III: Unbiased UV continuum slopes at 6.5, Austin et al., 2024, arXiv, arXiv:2404.10751
• Exploring the faintest end of mid-infrared luminosity functions up to z ≃ 5 with the JWST CEERS survey, Ling et al., 2024, MNRAS, 528, 6025
• Deciphering Lyman-α emission deep into the epoch of reionization, Witten et al., 2024, NatAs, 8, 384
• Explaining the high nitrogen abundances observed in high-z galaxies via population III stars of a few thousand solar masses, Nandal et al., 2024, A&A, 683, A156
• JWST spectroscopy of z 5-8 UV-selected galaxies: new constraints on the evolution of the Ly α escape fraction in the reionization era, Chen et al., 2024, MNRAS, 528, 7052
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations, Harvey et al., 2024, arXiv, arXiv:2403.03908
• Dust Extinction Measures for z ~ 8 Galaxies using Machine Learning on JWST Imaging, Fu et al., 2024, arXiv, arXiv:2403.18458
• Remarkably Compact Quiescent Candidates at 3 < z < 5 in JWST-CEERS, Wright et al., 2024, ApJL, 964, L10
• Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys, Hainline et al., 2024, ApJ, 964, 66
• Characterization of JWST NIRCam PSFs and Implications for AGN+host Image Decomposition, Zhuang and Shen et al., 2024, ApJ, 962, 139
• Galaxy Quenching at the High Redshift Frontier: A Fundamental Test of Cosmological Models in the Early Universe with JWST-CEERS, Bluck et al., 2024, ApJ, 961, 163
• JWST reveals a high fraction of disk breaks at 1 ≤ z ≤ 3, Xu and Yu et al., 2024, A&A, 682, L17
• Direct T _e-based Metallicities of z = 2–9 Galaxies with JWST/NIRSpec: Empirical Metallicity Calibrations Applicable from Reionization to Cosmic Noon, Sanders et al., 2024, ApJ, 962, 24
• A Robust Study of High-redshift Galaxies: Unsupervised Machine Learning for Characterizing Morphology with JWST up to z ∼ 8, Tohill et al., 2024, ApJ, 962, 164
• Polycyclic aromatic hydrocarbon luminous galaxies in JWST CEERS data, Lin et al., 2024, MNRAS, 527, 11882
• Near-IR clumps and their properties in high-z galaxies with JWST/NIRCam, Kalita et al., 2024, arXiv, arXiv:2402.02679
• EPOCHS VI: the size and shape evolution of galaxies since z 8 with JWST Observations, Ormerod et al., 2024, MNRAS, 527, 6110
• Stellar Half-mass Radii of 0.5 z < 2.3 Galaxies: Comparison with JWST/NIRCam Half-light Radii, van der Wel et al., 2024, ApJ, 960, 53
• Extreme N-emitters at high redshift: Possible signatures of supermassive stars and globular cluster or black hole formation in action, Marques-Chaves et al., 2024, A&A, 681, A30
• The Structure and Morphology of Galaxies during the Epoch of Reionization Revealed by JWST, Sun et al., 2024, ApJ, 960, 104
• MOSEL survey: Unwrapping the Epoch of Reionisation through mimic galaxies at Cosmic Noon, Jaiswar et al., 2024, PASA, 41, e040
• The evolution of galaxy morphology from redshift z=6 to 3: Mock JWST observations of galaxies in the ASTRID simulation, LaChance et al., 2024, arXiv, arXiv:2401.16608
• Are we surprised to find SMBHs with JWST at z ≥ 9?, Schneider et al., 2023, MNRAS, 526, 3250
• Seen and unseen: bursty star formation and its implications for observations of high-redshift galaxies with JWST, Sun et al., 2023, MNRAS, 526, 2665
• JWST Census for the Mass-Metallicity Star Formation Relations at z = 4-10 with Self-consistent Flux Calibration and Proper Metallicity Calibrators, Nakajima et al., 2023, ApJS, 269, 33
• JWST Identification of Extremely Low C/N Galaxies with [N/O] ≳ 0.5 at z ~ 6-10 Evidencing the Early CNO-cycle Enrichment and a Connection with Globular Cluster Formation, Isobe et al., 2023, ApJ, 959, 100
• JWST/NIRSpec spectroscopy of z = 7-9 star-forming galaxies with CEERS: new insight into bright Lyα emitters in ionized bubbles, Tang et al., 2023, MNRAS, 526, 1657
• Solution to the Conflict between the Estimations of Resolved and Unresolved Galaxy Stellar Mass from the Perspective of JWST, Song et al., 2023, ApJ, 958, 82
• Rest-frame Near-infrared Radial Light Profiles up to z = 3 from JWST/NIRCam: Wavelength Dependence of the Sérsic Index, Martorano et al., 2023, ApJ, 957, 46
• JWST CEERS and JADES Active Galaxies at z = 4-7 Violate the Local M _•-M _⋆ Relation at >3σ: Implications for Low-mass Black Holes and Seeding Models, Pacucci et al., 2023, ApJL, 957, L3
• Primordial power spectrum in light of JWST observations of high redshift galaxies, Parashari and Laha et al., 2023, MNRAS, 526, L63
• The JWST Hubble Sequence: The Rest-frame Optical Evolution of Galaxy Structure at 1.5 < z < 6.5, Ferreira et al., 2023, ApJ, 955, 94
• Redshift Evolution of Electron Density in the Interstellar Medium at z ~ 0-9 Uncovered with JWST/NIRSpec Spectra and Line-spread Function Determinations, Isobe et al., 2023, ApJ, 956, 139
• Using cGANs for Anomaly Detection: Identifying Astronomical Anomalies in JWST Imaging, Pearce-Casey et al., 2023, RNAAS, 7, 217
• Stellar and AGN Feedback Probed with Outflows in JWST Galaxies at z=3-9: Implications of More Spherical Galactic Fountains, Xu et al., 2023, arXiv, arXiv:2310.06614
• A JWST/NIRCam study of key contributors to reionization: the star-forming and ionizing properties of UV-faint z 7-8 galaxies, Endsley et al., 2023, MNRAS, 524, 2312
• No Tension: JWST Galaxies at z > 10 Consistent with Cosmological Simulations, McCaffrey et al., 2023, OJAp, 6, 47
• Excitation and Ionization Properties of Star-forming Galaxies at z = 2.0-9.3 with JWST/NIRSpec, Sanders et al., 2023, ApJ, 955, 54
• JWST/NIRSpec Balmer-line Measurements of Star Formation and Dust Attenuation at z 3-6, Shapley et al., 2023, ApJ, 954, 157
• Evolution of Nonparametric Morphology of Galaxies in the JWST CEERS Field at z ≃ 0.8-3.0, Yao et al., 2023, ApJ, 954, 113
• A T-dwarf candidate from JWST early release NIRCam data, Wang et al., 2023, MNRAS, 523, 4534
• A JWST/NIRSpec Exploration of the Connection between Ionization Parameter, Electron Density, and Star-formation-rate Surface Density in z = 2.7-6.3 Galaxies, Reddy et al., 2023, ApJ, 952, 167
• Redshifting galaxies from DESI to JWST CEERS: Correction of biases and uncertainties in quantifying morphology, Yu et al., 2023, A&A, 676, A74
• Sub-millimetre galaxies with Webb. Near-infrared counterparts and multi-wavelength morphology, Gillman et al., 2023, A&A, 676, A26
• Source counts at 7.7-21 μm in CEERS field with JWST, Wu et al., 2023, MNRAS, 523, 5187
• Morphologies of Galaxies at z ≳ 9 Uncovered by JWST/NIRCam Imaging: Cosmic Size Evolution and an Identification of an Extremely Compact Bright Galaxy at z 12, Ono et al., 2023, ApJ, 951, 72
• Resolving Galactic-scale Obscuration of X-Ray AGNs at z ≳ 1 with COSMOS-Web, Silverman et al., 2023, ApJL, 951, L41
• UV luminosity density results at z > 8 from the first JWST/NIRCam fields: limitations of early data sets and the need for spectroscopy, Bouwens et al., 2023, MNRAS, 523, 1009
• Unveiling the nature of infrared bright, optically dark galaxies with early JWST data, Barrufet et al., 2023, MNRAS, 522, 449
• JWST/NIRSpec Measurements of the Relationships between Nebular Emission-line Ratios and Stellar Mass at z 3-6, Shapley et al., 2023, ApJL, 950, L1
• Paschen-line Constraints on Dust Attenuation and Star Formation at z 1-3 with JWST/NIRSpec, Reddy et al., 2023, ApJ, 948, 83
• A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS, Carnall et al., 2023, MNRAS, 520, 3974
• Seeking the growth of the first black hole seeds with JWST, Trinca et al., 2023, MNRAS, 519, 4753
• Massive galaxy formation caught in action at z ∼ 5 with JWST, Jin et al., 2023, A&A, 670, L11
• The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 - 15 from deep JWST and ground-based near-infrared imaging, Donnan et al., 2023, MNRAS, 518, 6011
• Morpheus Reveals Distant Disk Galaxy Morphologies with JWST: The First AI/ML Analysis of JWST Images, Robertson et al., 2023, ApJL, 942, L42
• A Candidate for the Least-massive Black Hole in the First 1.1 Billion Years of the Universe, Onoue et al., 2023, ApJL, 942, L17
• Early JWST Imaging Reveals Strong Optical and NIR Color Gradients in Galaxies at z~2 Driven Mostly by Dust, Miller et al., 2022, ApJL, 941, L37
• Opening the Era of Quasar-host Studies at High Redshift with JWST, Ding et al., 2022, ApJL, 939, L28
• Two Remarkably Luminous Galaxy Candidates at z ≈ 10-12 Revealed by JWST, Naidu et al., 2022, ApJL, 940, L14
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• Rest-frame Near-infrared Sizes of Galaxies at Cosmic Noon: Objects in JWST's Mirror Are Smaller than They Appeared, Suess et al., 2022, ApJL, 937, L33
• Schrodinger's Galaxy Candidate: Puzzlingly Luminous at z≈17, or Dusty/Quenched at z≈5?, Naidu et al., 2022, arXiv, arXiv:2208.02794