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CANDELS UDS F160W J033235.56-275021.0 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST02:06:06 |
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 |
---|---|---|---|---|---|---|---|---|---|
2011A&A...533A.119E | 15 | D | 1 | 3965 | 926 | GOODS-Herschel: an infrared main sequence for star-forming galaxies. | ELBAZ D., DICKINSON M., HWANG H.S., et al. | ||
2014ApJ...791...52B | 17 | D | 1 | 47 | 144 | CANDELS+3D-HST: compact SFGs at z ∼ 2-3, the progenitors of the first quiescent galaxies. | BARRO G., FABER S.M., PEREZ-GONZALEZ P.G., et al. | ||
2014ApJS..214...24S | 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. | ||
2016ApJS..225...27M | 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 | 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. | ||
2018MNRAS.475.5133R | 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...878...83W | 17 | 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. | ||
2020ApJ...901..168A | 17 | D | 3 | 59 | 11 | Completing the census of AGN in GOODS-S/HUDF: new ultradeep radio imaging and predictions for JWST. | ALBERTS S., RUJOPAKARN W., RIEKE G.H., et al. |