[SWM2014] GOODS-S 5030 , the SIMBAD biblio

[SWM2014] GOODS-S 5030 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST20:43:20

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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
2003A&A...403..493M viz 4820 24 H-band observations of the Chandra Deep Field South. MOY E., BARMBY P., RIGOPOULOU D., et al.
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.
2006A&A...452..119O viz 3542 8 ESO imaging survey: infrared observations of CDF-S and HDF-S. OLSEN L.F., MIRALLES J.-M., DA COSTA L., et al.
2006A&A...454..423V viz 15       D               926 193 The great observatories origins deep survey . VLT/FORS2 spectroscopy in the GOODS-South Field: Part II. VANZELLA E., CRISTIANI S., DICKINSON M., et al.
2008A&A...478...83V viz 15       D               885 308 The Great Observatories Origins Deep Survey. VLT/FORS2 spectroscopy in the GOODS-South field: Part III. VANZELLA E., CRISTIANI S., DICKINSON 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.
2014ApJS..214...24S viz 16       D               1 66903 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 16       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.
2015ApJ...806..147C 17       D               1 59 125 Radio loud AGNs are mergers. CHIABERGE M., GILLI R., LOTZ J.M., et al.
2016ApJS..225...27M viz 16       D               1 19341 548 The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ∼ 100,000 galaxies. MOMCHEVA I.G., BRAMMER G.B., VAN DOKKUM P.G., et al.
2016ApJ...830...51S viz 16       D               1 67524 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.
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.
2019ApJ...877....5L viz 17       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...886..124W viz 17       D               1 781 76 The KMOS3D survey: data release and final survey paper. WISNIOSKI E., FORSTER SCHREIBER N.M., FOSSATI M., et al.
2019ApJ...887...23B viz 17       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.
2020ApJ...888...78S viz 17       D               1 2590 25 A catalog of AGN host galaxies observed with HST/ACS: correlations between star formation and AGN activity. STEMO A., COMERFORD J.M., BARROWS R.S., et al.
2020MNRAS.492.1887G viz 17       D               1 792 ~ Physical properties of the CDFS X-ray sources through fitting spectral energy distributions. GUO X., GU Q., DING N., et al.
2020ApJ...905..170M viz 17       D               1 4760 24 Galaxy sizes since z = 2 from the perspective of stellar mass distribution within galaxies. MOSLEH M., HOSSEINNEJAD S., HOSSEINI-SHAHISAVANDI S.Z., et al.

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