JADES-GS NS 54612 , the SIMBAD biblio

JADES-GS NS 54612 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST11:54:53

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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
2006AJ....132..926C viz 15       D               2664 396 Galaxies in the Hubble Ultra Deep Field. I. Detection, multiband photometry, photometric redshifts, and morphology. COE D., BENITEZ N., SANCHEZ S.F., et al.
2007ApJ...668..839R viz 15       D               1309 41 The galaxy luminosity function at z ≃ 1 in the HUDF: probing the dwarf population. RYAN R.E.Jr, HATHI N.P., COHEN S.H., et al.
2009ApJ...703.2033R viz 15       D               1 505 23 Deep Keck u-band imaging of the Hubble Ultra Deep Field: a catalog of z ∼ 3 Lyman break galaxies. RAFELSKI M., WOLFE A.M., COOKE J., et al.
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.
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.
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.
2017A&A...608A...2I viz 16       D               1 1584 136 The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies. INAMI H., BACON R., BRINCHMANN J., et al.
2018MNRAS.475.5133R viz 16       D               1 11242 2 Testing the hierarchical assembly of massive galaxies using accurate merger rates out to z ∼ 1.5. RODRIGUES M., PUECH M., FLORES H., 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.
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.
2022MNRAS.511..120S 19       D               14 29 No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at <= z <= 3.5. SAXENA A., PENTERICCI L., ELLIS R.S., 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.
2024ApJ...974L..20Z 18       D               1 29 ~ Lyman Continuum Leakers at z > 3 in the GOODS-S Field: Starburst or Not? ZHU S., YUAN F.-T., JIANG C., et al.
2024ApJ...975...53Y 18       D               1 75 ~ Merging Signatures in an Offset Lyman Continuum Emitter at Redshift 3.8. YUAN F.-T., ZHENG Z.-Y., JIANG C., et al.
2025ApJ...982L..58Z 93               F     1 27 ~ Lyman Continuum Leakers at z > 3 in the GOODS-S Field: Mergers Dominated. ZHU S., ZHENG Z.-Y., YUAN F.-T., et al.
2025ApJ...986L..24J 19       D               1 99 ~ Potential-driven Metal Cycling: JADES Census of Gas-phase Metallicity for Galaxies at 1 < z < 7. JIA C., WANG E., LYU C., et al.
2025ApJ...994...35R 19       D               3 38 ~ Confirming Near- to Mid-infrared Photometrically Identified Obscured AGNs in the JWST Era. RIEKE G.H., SUN Y., LYU J., et al.
2026ApJ..1000L...3L 20       D               2 41 ~ First Statistical Detection of Mg II-traced Cool Gas Outflows with JWST toward Cosmic Dawn. LYU C., YU H., WANG E., et al.

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