First Author | Title | Year | Keyword1 | Keyword2 |
---|---|---|---|---|
Arellano-Córdova, K. Z. | A First Look at the Abundance Pattern-O/H, C/O, and Ne/O-in z > 7 Galaxies with JWST/NIRSpec | 2022 | abundances | metallicity |
Boyett, K. | Early Results from GLASS-JWST. VI. Extreme Rest-optical Equivalent Widths Detected in NIRISS Wide Field Slitless Spectroscopy | 2023 | abundances | metallicity |
Curti, M. | The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z ∼ 8 | 2023 | abundances | metallicity |
Heintz, K. E. | The Gas and Stellar Content of a Metal-poor Galaxy at z = 8.496 as Revealed by JWST and ALMA | 2023 | abundances | metallicity |
Isobe, Y. | Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations | 2023 | abundances | metallicity |
Lin, X. | Metal-enriched Neutral Gas Reservoir around a Strongly Lensed Low-mass Galaxy at z = 4 Identified by JWST/NIRISS and VLT/MUSE | 2023 | abundances | metallicity |
Nakajima, K. | JWST Census for the Mass-Metallicity Star-Formation Relations at z=4-10 with Self-Consistent Flux Calibration and the Proper Metallicity Calibrators | 2023 | abundances | metallicity |
Bland-Hawthorn, J. | The rapid onset of stellar bars in the baryon-dominated centers of disk galaxies | 2023 | morphology | - |
Chen, C.-C. | JWST Sneaks a Peek at the Stellar Morphology of z 2 Submillimeter Galaxies: Bulge Formation at Cosmic Noon | 2022 | morphology | - |
Ferreira, L. | Panic! at the Disks: First Rest-frame Optical Observations of Galaxy Structure at z > 3 with JWST in the SMACS 0723 Field | 2022 | morphology | - |
Ferreira, L. | The JWST Hubble Sequence: The Rest-Frame Optical Evolution of Galaxy Structure at $1.5 < z < 8$ | 2022 | morphology | - |
Fudamoto, Y. | Red Spiral Galaxies at Cosmic Noon Unveiled in the First JWST Image | 2022 | morphology | - |
Guo, Y. | First Look at z > 1 Bars in the Rest-frame Near-infrared with JWST Early CEERS Imaging | 2023 | morphology | - |