JADES-GS+053.11852-27.81297 , the SIMBAD biblio

JADES-GS+053.11852-27.81297 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:02:57


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Title First 3 Authors
2014ApJS..214...24S viz 15       D               1 97940 733 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al.
2015ApJ...803...34B viz 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.
2018ApJS..237...12O viz 16       D               1 25243 42 HDUV: the Hubble Deep UV Legacy Survey. OESCH P.A., MONTES M., REDDY N., et al.
2021ApJS..257...68S viz 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.
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...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               1 88 ~ Extreme emission line galaxies detected in JADES JWST/NIRSpec - I. Inferred galaxy properties. BOYETT K., BUNKER A.J., CURTIS-LAKE E., 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.

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