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| JADES-GS NS 10035295 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:17:50 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2023ApJS..269...16R 
|
17 | D | 1 | 2653 | ~ | JADES Initial Data Release for the Hubble Ultra Deep Field: Revealing the Faint Infrared Sky with Deep JWST NIRCam Imaging. | RIEKE M.J., ROBERTSON B., TACCHELLA S., et al. | ||
| 2024A&A...681A..70L | 18 | D | 2 | 15 | ~ | JADES: Detecting [OIII]λ4363 emitters and testing strong line calibrations in the high-z Universe with ultra-deep JWST/NIRSpec spectroscopy up to z ∼ 9.5. | LASETER I.H., MASEDA M.V., CURTI M., et al. | ||
| 2024A&A...684A..75C | 18 | D | 2 | 76 | ~ | JADES: Insights into the low-mass end of the mass-metallicity-SFR relation at 3 < z < 10 from deep JWST/NIRSpec spectroscopy. | CURTI M., MAIOLINO R., CURTIS-LAKE E., et al. | ||
| 2024MNRAS.535.1796B | 18 | D | 2 | 88 | ~ | Extreme emission line galaxies detected in JADES JWST/NIRSpec - I. Inferred galaxy properties. | BOYETT K., BUNKER A.J., CURTIS-LAKE E., et al. | ||
| 2025MNRAS.538.1921M | 19 | D | 1 | 79 | ~ | JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe. | MAIOLINO R., RISALITI G., SIGNORINI M., et al. | ||
| 2025ApJ...984..182X | 19 | D | 1 | 29 | ~ | Stellar- and AGN-driven Outflows in JWST Galaxies at z = 3-9: More Frequent, Wider Opening Angles, and Mostly Bounded. | XU Y., OUCHI M., NAKAJIMA K., et al. | ||
| 2025A&A...697A.175S | 19 | D | 1 | 41 | ~ | JADES: A large population of obscured, narrow-line active galactic nuclei at high redshift. | SCHOLTZ J., MAIOLINO R., D'EUGENIO F., et al. | ||
| 2026A&A...706A.302C | 20 | D | 1 | 42 | ~ | JWST-discovered AGN: Evidence of heavy obscuration in the type 2 sample from the first stacked X-ray detection. | COMASTRI A., LANZUISI G., VITO F., et al. |
