JADES-GS NC 210751 , the SIMBAD biblio

JADES-GS NC 210751 , the SIMBAD biblio (8 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:53:09


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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.
2016ApJ...830...51S viz 16       D               1 67525 168 The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al.
2021A&A...647A.150G viz 17       D               1 2166 44 The VANDELS ESO public spectroscopic survey. Final data release of 2087 spectra and spectroscopic measurements. GARILLI B., McLURE R., PENTERICCI L., 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.
2023A&A...678A..25T viz 17       D               1 1733 ~ The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue. TALIA M., SCHREIBER C., GARILLI B., 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.
2024MNRAS.532.3102S 18       D               3 34 ~ The NIRVANDELS survey: the stellar and gas-phase mass-metallicity relations of star-forming galaxies at z = 3.5. STANTON T.M., CULLEN F., McLURE R.J., et al.

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