GEMS J033204.00-274441.3 , the SIMBAD biblio

GEMS J033204.00-274441.3 , the SIMBAD biblio (29 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:40:23

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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
2004ApJ...600L..93G viz 15       D               1 7819 1453 The Great Observatories Origins Deep Survey: initial results from optical and near-infrared imaging. GIAVALISCO M., FERGUSON H.C., KOEKEMOER A.M., et al.
2008ApJS..179...19L viz 15       D               1 586 273 The Chandra Deep Field-South survey: 2 Ms source catalogs. LUO B., BAUER F.E., BRANDT W.N., et al.
2010ApJS..187..560L viz 15       D               1 469 134 Identifications and photometric redshifts of the 2 Ms Chandra Deep Field-South sources. LUO B., BRANDT W.N., XUE Y.Q., et al.
2011ApJ...727L..31S 18       D               1 25 170 HST WFC3/IR observations of active galactic nucleus host galaxies at z ∼ 2: supermassive black holes grow in disk galaxies. SCHAWINSKI K., TREISTER E., URRY C.M., et al.
2011ApJS..195...10X viz 15       D               1 782 508 The Chandra Deep Field-South survey: 4 Ms source catalogs. XUE Y.Q., LUO B., BRANDT W.N., et al.
2011ApJ...743..146C viz 15       D               1 4132 61 Active and passive galaxies at z ∼ 2: rest-frame optical morphologies with WFC3. CAMERON E., CAROLLO C.M., OESCH P.A., et al.
2012A&A...537A..16F 16       D               2 65 147 Faint high-redshift AGN in the Chandra Deep Field South: the evolution of the AGN luminosity function and black hole demography. FIORE F., PUCCETTI S., GRAZIAN A., et al.
2013ApJ...762...45B 16       D               1 26 71 The X-ray star formation story as told by Lyman break galaxies in the 4 ms CDF-s. BASU-ZYCH A.R., LEHMER B.D., HORNSCHEMEIER A.E., et al.
2013MNRAS.428..354V 15       D               1 37 35 The high-redshift (z > 3) active galactic nucleus population in the 4-Ms Chandra Deep Field-South. VITO F., VIGNALI C., GILLI R., 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.
2014ApJ...796...60H viz 15       D               1 1489 120 CANDELS/GOODS-S, CDFS, and ECDFS : photometric redshifts for normal and X-Ray-detected galaxies. HSU L.-T., SALVATO M., NANDRA K., et al.
2014MNRAS.445.3557V 15       D               1 144 72 The hard X-ray luminosity function of high-redshift (3 < z ≲ 5) active galactic nuclei. VITO F., GILLI R., VIGNALI C., et al.
2016MNRAS.457..629C viz 16       D               1 650 33 ZFOURGE catalogue of AGN candidates: an enhancement of 160-µm-derived star formation rates in active galaxies to z = 3.2. COWLEY M.J., SPITLER L.R., TRAN K.-V.H., 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.
2017ApJS..228....2L viz 16       D               1 1061 334 The Chandra Deep Field-South survey: 7 Ms source catalogs. LUO B., BRANDT W.N., XUE Y.Q., et al.
2017Msngr.167...31M viz 16       D               1 879 3 VANDELS: Exploring the physics of high-redshift galaxy evolution. McLURE R., PENTERICCI L. (The VANDELS Team)
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.
2018MNRAS.473.2378V 16       D               1 123 109 High-redshift agn in the Chandra Deep Fields: the obscured fraction and space density of the sub-L* population. VITO F., BRANDT W.N., YANG G., et al.
2019ApJ...877....5L viz 16       D               1 439 2 Piercing through highly obscured and Compton-thick AGNs in the Chandra Deep Fields. I. X-ray spectral and long-term variability analyses. LI J., XUE Y., SUN M., et al.
2019ApJ...878...83W 16       D               1 79 3 Evolution of the gas mass fraction of progenitors to today's massive galaxies: ALMA observations in the CANDELS GOODS-S field. WIKLIND T., FERGUSON H.C., GUO Y., et al.
2019ApJ...887...23B viz 16       D               1 942 ~ A submillimeter perspective on the GOODS fields (SUPER GOODS). IV. The submillimeter properties of X-ray sources in the CDF-S. BARGER A.J., COWIE L.L., BAUER F.E., et al.
2020MNRAS.492.1887G viz 16       D               1 792 ~ Physical properties of the CDFS X-ray sources through fitting spectral energy distributions. GUO X., GU Q., DING N., et al.
2020MNRAS.496..695C viz 140       D S   X         3 154 49 Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5. CARNALL A.C., WALKER S., McLURE R.J., 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.
2023A&A...674A.221M 44           X         1 51 3 Insights into the reionization epoch from cosmic-noon-C IV emitters in the VANDELS survey. MASCIA S., PENTERICCI L., SAXENA 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.
2025A&A...694A.170P 327           X C       6 4 ~ GA-NIFS: A galaxy-wide outflow in a Compton-thick mini-broad-absorption-line quasar at z = 3.5 probed in emission and absorption. PERNA M., ARRIBAS S., JI X., et al.
2025A&A...696A..59P 47           X         1 37 ~ GA-NIFS: High number of dual active galactic nuclei at z ∼ 3. PERNA M., ARRIBAS S., LAMPERTI I., et al.
2025ApJ...987...46Z 19       D               1 466 ~ Identifying Compton-thick Active Galactic Nuclei with a Machine Learning Algorithm in Chandra Deep Field-South. ZHANG R., GUO X., GU Q., et al.

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