JADES-GS NS 7892 , the SIMBAD biblio

JADES-GS NS 7892 , the SIMBAD biblio (8 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST12:07:46

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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
2015AJ....150...31R viz 16       D               1 9968 140 UVUDF: ultraviolet through near-infrared catalog and photometric redshifts of galaxies in the Hubble Ultra Deep Field. RAFELSKI M., TEPLITZ H.I., GARDNER J.P., et al.
2023ApJS..269...16R viz 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 108       D       C       3 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.
2024A&A...685A..99C viz 18       D               1 14 ~ JADES: The incidence rate and properties of galactic outflows in low-mass galaxies across 3 < z < 9. CARNIANI S., VENTURI G., PARLANTI 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.
2024A&A...692A.184T 179             C F     1 18 ~ Spatially resolved emission lines in galaxies at 4 ≤ z < 10 from the JADES survey: Evidence for enhanced central star formation. TRIPODI R., D'EUGENIO F., MAIOLINO R., 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.

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