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
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!)
- 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
- 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
- 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
- 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
- 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
- TRINITY IV: predictions for supermassive black holes at z ≳ 6, Zhang et al., 2024, MNRAS, 531, 4974
- 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
- MOSEL survey: Unwrapping the Epoch of Reionisation through mimic galaxies at Cosmic Noon, Jaiswar et al., 2024, PASA, 41, e040
- 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
- EPOCHS Paper V. The dependence of galaxy formation on galaxy structure at z < 7 from JWST observations, Conselice et al., 2024, MNRAS, 531, 4857
- An Edge-on Regular Disk Galaxy at z=5.289, Yan et al., 2024, arXiv, arXiv:2407.04209
- 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
- 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
- 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
- Finding dusty AGNs from the JWST CEERS survey with mid-infrared photometry, Chien et al., 2024, MNRAS, 532, 719
- JWST Reveals a Surprisingly High Fraction of Galaxies Being Spiral-like at 0.5 ≤ z ≤ 4, Kuhn et al., 2024, ApJL, 968, L15
- The Star-Forming Main Sequence in JADES and CEERS at z>1.4: Investigating the Burstiness of Star Formation, Clarke et al., 2024, arXiv, arXiv:2406.05178
- The PSF smoothing effect on concentration-related parameters of high-redshift galaxies in HST and JWST, Wang et al., 2024, A&A, 686, A100
- 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
- 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
- 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
- EPOCHS Paper X: Environmental effects on Galaxy Formation and Protocluster Galaxy candidates at 4.5<z<10 from JWST observations, Li et al., 2024, arXiv, arXiv:2405.17359
- A Steep Decline in the Galaxy Space Density beyond Redshift 9 in the CANUCS UV Luminosity Function, Willott et al., 2024, ApJ, 966, 74
- Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology, Lee et al., 2024, ApJ, 966, 113
- A JWST investigation into the bar fraction at redshifts 1 ≤ z ≤ 3, Le Conte et al., 2024, MNRAS, 530, 1984
- 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<z<13 from combined PEARLS GTO and public JWST NIRCam imaging, Austin et al., 2024, arXiv, arXiv:2404.10751
- 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
- Deciphering Lyman-α emission deep into the epoch of reionization, Witten et al., 2024, NatAs, 8, 384
- 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
- Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys, Hainline et al., 2024, ApJ, 964, 66
- 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
- Remarkably Compact Quiescent Candidates at 3 < z < 5 in JWST-CEERS, Wright et al., 2024, ApJL, 964, L10
- 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
- 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
- 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
- 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
- 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
- JWST/MIRI unveils the stellar component of the GN20 dusty galaxy overdensity at z=4.05, Crespo Gómez et al., 2024, arXiv, arXiv:2402.18672
- JWST reveals a high fraction of disk breaks at 1 ≤ z ≤ 3, Xu and Yu et al., 2024, A&A, 682, L17
- Characterization of JWST NIRCam PSFs and Implications for AGN+host Image Decomposition, Zhuang and Shen et al., 2024, ApJ, 962, 139
- 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
- The Structure and Morphology of Galaxies during the Epoch of Reionization Revealed by JWST, Sun et al., 2024, ApJ, 960, 104
- 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
- EPOCHS VI: the size and shape evolution of galaxies since z 8 with JWST Observations, Ormerod et al., 2024, MNRAS, 527, 6110
- 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
- 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
- Seen and unseen: bursty star formation and its implications for observations of high-redshift galaxies with JWST, Sun et al., 2023, MNRAS, 526, 2665
- Are we surprised to find SMBHs with JWST at z ≥ 9?, Schneider et al., 2023, MNRAS, 526, 3250
- 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
- Primordial power spectrum in light of JWST observations of high redshift galaxies, Parashari and Laha et al., 2023, MNRAS, 526, L63
- 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
- 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
- Stellar and AGN Feedback Probed with Outflows in JWST Galaxies at z=3-9: Implications of Frequent Nearly-Spherical Galactic Fountains, Xu et al., 2023, arXiv, arXiv:2310.06614
- 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
- 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
- Using cGANs for Anomaly Detection: Identifying Astronomical Anomalies in JWST Imaging, Pearce-Casey et al., 2023, RNAAS, 7, 217
- Efficient survey design for finding high-redshift galaxies with JWST, Vujeva et al., 2023, arXiv, arXiv:2310.15284
- 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
- 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
- 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
- A T-dwarf candidate from JWST early release NIRCam data, Wang et al., 2023, MNRAS, 523, 4534
- Source counts at 7.7-21 μm in CEERS field with JWST, Wu et al., 2023, MNRAS, 523, 5187
- 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
- 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
- Resolving Galactic-scale Obscuration of X-Ray AGNs at z ≳ 1 with COSMOS-Web, Silverman et al., 2023, ApJL, 951, L41
- 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
- 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
- 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
- Unveiling the nature of infrared bright, optically dark galaxies with early JWST data, Barrufet et al., 2023, MNRAS, 522, 449
- 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
- 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
- Massive galaxy formation caught in action at z ∼ 5 with JWST, Jin et al., 2023, A&A, 670, L11
- 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
- JWST Sneaks a Peek at the Stellar Morphology of z 2 Submillimeter Galaxies: Bulge Formation at Cosmic Noon, Chen et al., 2022, ApJL, 939, L7
- Two Remarkably Luminous Galaxy Candidates at z ≈ 10-12 Revealed by JWST, Naidu et al., 2022, ApJL, 940, L14
- 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