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Disambiguation of "Wuyts, Stijn"

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The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2016)cite arxiv:1603.01139Comment: submitted to ApJ.

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Geert Wuyts

Stijn Cleemput

 

Other publications of authors with the same name

Metallicity evolution at 0.8 < z < 2.6 from the LUCI, SINS/zC-SINF and KMOS-3D surveys, , , , , , , , , and 26 other author(s). (2014)cite arxiv:1405.6590Comment: 7 pages, 3 figures, submitted to ApJL.The Assembly of Milky Way-like Galaxies Since z~2.5, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1304.2391Comment: Submitted to ApJ Letters. 7 pages, 5 figures.The SINS/zC-SINF survey of z~2 galaxy kinematics: Outflow properties, , , , , , , , , and 15 other author(s). (2012)cite arxiv:1207.5897Comment: Submitted to ApJ Letters.The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , and 20 other author(s). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1507.03999Comment: Submitted to ApJ. Main results: Fig. 6 shows the scale lengths of ionized gas vs. stellar disks. Fig. 9 shows where Halpha in galaxies is enhanced above and suppressed below the star-forming main sequence. Data points for Halpha profiles are available upon request.Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4, , , , , , , , and . (2015)cite arxiv:1511.04443Comment: Submitted to ApJ Letters. Fig. 2. shows measured radial Balmer decrement profiles. Fig. 3 shows inferred dust gradients. Fig. 4 shows dust-corrected radial profiles of star formation and the likely growth of bulges in high mass galaxies through in-situ star formation.Shocked Superwinds from the z~2 Clumpy Star-forming Galaxy, ZC406690, , , , , , , , , and 13 other author(s). (2012)cite arxiv:1204.4727Comment: 21 pages, 7 figures, Accepted for publication in ApJ.Direct measurement of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates, , , , , , , , , and 5 other author(s). (2013)cite arxiv:1310.4177Comment: Submitted for publication in the Astrophysical Journal.Validation of the equilibrium model for galaxy evolution to z~3 through molecular gas and dust observations of lensed star-forming galaxies, , , , , , , , , and 4 other author(s). (2013)cite arxiv:1309.3281Comment: accepted for publication in ApJ.