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| JADES-GS+053.11243-27.77461 , the SIMBAD biblio (44 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST04:55:01 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2014ApJ...786..108O | 413 | D | X C | 10 | 12 | 276 | The most luminous z ∼ 9-10 galaxy candidates yet found: the luminosity function, cosmic star-formation rate, and the first mass density estimate at 500 myr. | OESCH P.A., BOUWENS R.J., ILLINGWORTH G.D., et al. | |
|
2015ApJ...803...34B |
16 | D | 1 | 10313 | 1045 | UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields. | BOUWENS R.J., ILLINGWORTH G.D., OESCH P.A., et al. | ||
| 2015ApJ...808....6H | 57 | D | X | 2 | 8 | 33 | The sizes of candidate z∼9-10 galaxies: confirmation of the bright CANDELS sample and relation with luminosity and mass. | HOLWERDA B.W., BOUWENS R., OESCH P., et al. | |
| 2016MNRAS.455..659W | 17 | D | 1 | 8 | 21 | Quantifying the UV-continuum slopes of galaxies to z ∼ 10 using deep Hubble+Spitzer/IRAC observations. | WILKINS S.M., BOUWENS R.J., OESCH P.A., et al. | ||
| 2016ApJ...830...67B | 18 | D | 1 | 33 | 139 | The bright end of the z ∼ 9 and z ∼ 10 UV luminosity functions using all five CANDELS fields. | BOUWENS R.J., OESCH P.A., LABBE I., et al. | ||
| 2019ApJ...880...25B | 17 | D | 1 | 51 | 65 | Newly discovered bright z ∼ 9-10 galaxies and improved constraints on their prevalence using the full CANDELS area. | BOUWENS R.J., STEFANON M., OESCH P.A., et al. | ||
|
2021ApJS..257...68S |
17 | D | 1 | 9083 | 17 | The Spitzer/IRAC Legacy over the GOODS fields: full-depth 3.6, 4.5, 5.8, and 8.0 µm mosaics and photometry for >9000 galaxies at z ∼ 3.5-10 from the GOODS Reionization Era wide-Area Treasury from Spitzer (GREATS). | STEFANON M., LABBE I., OESCH P.A., et al. | ||
| 2022ApJ...928...52F | 45 | X | 1 | 32 | 68 | A Census of the Bright z = 8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields. | FINKELSTEIN S.L., BAGLEY M., SONG M., et al. | ||
| 2023ApJ...943...81S | 17 | D | 1 | 10 | 8 | Deep Spitzer/IRAC Data for z ∼ 10 Galaxies Reveal Blue Balmer Break Colors: Young Stellar Populations at ∼500 Myr of Cosmic Time. | STEFANON M., BOUWENS R.J., LABBE I., et al. | ||
| 2023A&A...677A.115C | 17 | D | 1 | 30 | ~ | JADES: Probing interstellar medium conditions at z ∼ 5.5-9.5 with ultra-deep JWST/NIRSpec spectroscopy. | CAMERON A.J., SAXENA A., BUNKER A.J., et al. | ||
|
2023ApJS..269...16R |
17 | D | 2 | 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. | ||
| 2024ApJ...960...56H | 108 | D | X | 3 | 32 | ~ | Pure Spectroscopic Constraints on UV Luminosity Functions and Cosmic Star Formation History from 25 Galaxies at zspec = 8.61-13.20 Confirmed with JWST/NIRSpec. | HARIKANE Y., NAKAJIMA K., OUCHI M., 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...683A.238J |
18 | D | 1 | 95 | ~ | JADES: The emergence and evolution of Lyα emission and constraints on the intergalactic medium neutral fraction. | JONES G.C., BUNKER A.J., SAXENA A., 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. | ||
| 2024ApJ...967...28N | 18 | D | 1 | 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. | ||
| 2024NatAs...8..657B | 90 | C | 2 | 5 | ~ | A massive interacting galaxy 510 million years after the Big Bang. | BOYETT K., TRENTI M., LEETHOCHAWALIT N., et al. | ||
| 2024ApJ...971...43M | 63 | D | X | 2 | 45 | ~ | Diverse Oxygen Abundance in Early Galaxies Unveiled by Auroral Line Analysis with JWST. | MORISHITA T., STIAVELLI M., GRILLO C., et al. | |
| 2024ApJ...971..124U | 18 | D | 1 | 35 | ~ | 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 H., OUCHI M., NAKAJIMA K., 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.536.2355J | 47 | X | 1 | 13 | ~ | JADES: measuring reionization properties using Lyman-alpha emission. | JONES G.C., BUNKER A.J., SAXENA A., et al. | ||
| 2025A&A...693A..50N | 47 | X | 1 | 24 | ~ | Seven wonders of Cosmic Dawn: JWST confirms a high abundance of galaxies and AGN at z ≃ 9-11 in the GLASS field. | NAPOLITANO L., CASTELLANO M., PENTERICCI L., et al. | ||
| 2025ApJ...980..225T | 112 | D | X | 3 | 29 | ~ | Deep Rest-UV JWST/NIRSpec Spectroscopy of Early Galaxies: The Demographics of C IV and N-emitters in the Reionization Era. | TOPPING M.W., STARK D.P., SENCHYNA P., et al. | |
| 2025A&A...694A.254H | 47 | X | 1 | 4 | ~ | ASTRAEUS X. Indications of a top-heavy initial mass function in highly star-forming galaxies from JWST observations at z > 10. | HUTTER A., CUETO E.R., DAYAL P., 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. | ||
| 2025MNRAS.538.3210B | 187 | C F | 2 | 8 | ~ | Accelerated by dark matter: a high-redshift pathway to efficient galaxy-scale star formation. | BOYLAN-KOLCHIN M. | ||
| 2025ApJ...983...91P | 606 | S X C | 11 | 4 | ~ | Constraining Reionization with Lyα Damping-wing Absorption in Galaxy Spectra: A Machine Learning Model Based on Reionization Simulations. | PARK H., JUNG I., YAJIMA H., et al. | ||
| 2025A&A...696A..87C | 93 | C | 1 | 15 | ~ | The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction? | CARNIANI S., D'EUGENIO F., JI X., et al. | ||
| 2025MNRAS.539.1834M | 93 | F | 2 | 13 | ~ | FOREVER22: insights into star formation and clustering properties of protoclusters from simulations and JWST. | MOROKUMA-MATSUI K., YAJIMA H. and ABE M. | ||
| 2025A&A...697A..89C | 5412 | T A | D | X C | 115 | 10 | ~ | JADES: The star formation and chemical enrichment history of a luminous galaxy at z ∼ 9.43 probed by ultra-deep JWST/NIRSpec spectroscopy. | CURTI M., WITSTOK J., JAKOBSEN P., et al. |
| 2025A&A...697A..96R | 19 | D | 2 | 11 | ~ | High N/O ratio at high redshift as a result of a strong burst of star formation and differential galactic winds. | RIZZUTI F., MATTEUCCI F., MOLARO P., et al. | ||
| 2025A&A...697A.175S | 252 | D | S X C | 4 | 41 | ~ | JADES: A large population of obscured, narrow-line active galactic nuclei at high redshift. | SCHOLTZ J., MAIOLINO R., D'EUGENIO F., et al. | |
| 2025MNRAS.541L..71I | 47 | X | 1 | 8 | ~ | JADES: nitrogen enhancement in high-redshift broad-line active galactic nuclei. | ISOBE Y., MAIOLINO R., D'EUGENIO F., et al. | ||
| 2025MNRAS.541.2134J | 1166 | X C F | 23 | 6 | ~ | JADES - the small blue bump in GN-z11: insights into the nuclear region of a galaxy at z = 10.6. | JI X., MAIOLINO R., FERLAND G., et al. | ||
| 2025ApJ...991..217T | 47 | X | 1 | 32 | ~ | JWST/NIRSpec Observations of High-ionization Emission Lines in Galaxies at High Redshift. | TANG M., STARK D.P., PLAT A., et al. | ||
| 2025ApJ...992L..27T | 47 | X | 1 | 5 | ~ | Insights for Early Massive Black Hole Growth from JWST Detection of the [Ne v] λ3427 Emission Line. | TRAKHTENBROT B., RICCI C., TREISTER E., et al. | ||
| 2025MNRAS.543.3367F | 93 | X | 2 | 15 | ~ | New ionization models and the shocking nitrogen excess at z > 5. | FLURY S.R., ARELLANO-CORDOVA K.Z., MORAN E.C., et al. | ||
| 2025ApJ...993...70H | 140 | X C | 2 | 12 | ~ | First Direct Carbon Abundance Measured at z > 10 in the Lensed Galaxy MACS0647-JD. | HSIAO T.Y.-Y., TOPPING M.W., COE D., et al. | ||
| 2025ApJ...994L..29Z | 140 | X | 3 | 6 | ~ | Only Nitrogen-enhanced Galaxies Have Detectable Ultraviolet Nitrogen Emission Lines at High Redshift. | ZHU P., KEWLEY L.J., HSIAO T.Y.-Y., et al. | ||
| 2025ApJ...994...65N | 532 | D | X C | 11 | 10 | ~ | Fe Abundances of Early Galaxies at z = 9-12 Derived with Deep JWST Spectra. | NAKANE M., OUCHI M., NAKAJIMA K., et al. | |
| 2025MNRAS.544.1588A | 47 | X | 1 | 53 | ~ | CLASSY XII: nitrogen enrichment shaped by gas density and feedback. | ARELLANO-CORDOVA K.Z., BERG D.A., MINGOZZI M., et al. | ||
| 2026A&A...705L..12V | 9 | ~ | A pristine, star-forming complex at z = 4.19. | VANZELLA E., MESSA M., ZANELLA A., et al. | |||||
| 2026ApJ...998....5Z | 650 | A | D | X | 14 | 10 | ~ | The Nature of Nitrogen-enhanced High-redshift Galaxies. | ZHU P., TRUSSLER J. and KEWLEY L.J. |
| 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. |