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| [MPC2023] GLASS 10021 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST17:30:52 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2023A&A...672A.155M | 17 | D | 1 | 31 | 20 | Closing in on the sources of cosmic reionization: First results from the GLASS-JWST program. | MASCIA S., PENTERICCI L., CALABRO A., et al. | ||
|
2023ApJS..269...33N |
17 | D | 1 | 187 | ~ | JWST Census for the Mass-Metallicity Star Formation Relations at z = 4-10 with Self-consistent Flux Calibration and Proper Metallicity Calibrators. | NAKAJIMA K., OUCHI M., ISOBE Y., et al. | ||
| 2023ApJ...959..100I | 17 | D | 1 | 67 | ~ | 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 Y., OUCHI M., TOMINAGA N., et al. | ||
| 2024ApJ...967...28N | 18 | D | 2 | 54 | ~ | Lyα Emission at z = 7-13: Clear Evolution of Lyα Equivalent Width Indicating a Late Cosmic Reionization History. | NAKANE M., OUCHI M., NAKAJIMA K., et al. | ||
| 2024ApJ...971...43M | 18 | D | 1 | 45 | ~ | Diverse Oxygen Abundance in Early Galaxies Unveiled by Auroral Line Analysis with JWST. | MORISHITA T., STIAVELLI M., GRILLO C., et al. | ||
| 2024ApJ...973..111J | 63 | D | X | 2 | 48 | ~ | Multivariate Predictors of Lyman Continuum Escape. II. Predicting Lyman Continuum Escape Fractions for High-redshift Galaxies. | JASKOT A.E., SILVEYRA A.C., PLANTINGA A., et al. | |
| 2025ApJ...980..138H | 19 | D | 1 | 68 | ~ | JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7-14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe. | HARIKANE Y., INOUE A.K., ELLIS R.S., et al. | ||
| 2025ApJ...985...24C | 47 | X | 1 | 22 | ~ | Unveiling the Cosmic Chemistry. II. “Direct” Te-based Metallicity of Galaxies at 3 < z < 10 with JWST/NIRSpec. | CHAKRABORTY P., SARKAR A., SMITH R., et al. |