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On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3

, , , , , , , , , , , , , , , , , , , , , , , , , и . (2011)cite arxiv:1106.5502Comment: Accepted for publication in The Astrophysical Journal, 19 pages, 15 figures.

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Natascha Schreiber

Natascha M Neugebauer

Tilmann M Schreiber

Natascha Schelero

Natascha Engel

 

Другие публикации лиц с тем же именем

Smooth(er) Stellar Mass Maps in CANDELS: Constraints on the Longevity of Clumps in High-redshift Star-forming Galaxies, , , , , , , , , и 15 other автор(ы). (2012)cite arxiv:1203.2611Comment: Submitted to The Astrophysical Journal, 25 pages, 1 table, 14 figures.On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3, , , , , , , , , и 16 other автор(ы). (2011)cite arxiv:1106.5502Comment: Accepted for publication in The Astrophysical Journal, 19 pages, 15 figures.Direct measurement of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates, , , , , , , , , и 5 other автор(ы). (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, , , , , , , , , и 4 other автор(ы). (2013)cite arxiv:1309.3281Comment: accepted for publication in ApJ.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , и 10 other автор(ы). (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.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , и 7 other автор(ы). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.Spatially-resolved dust maps from Balmer decrements in galaxies at z~1.4, , , , , , , , и . (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.The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , и 20 other автор(ы). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.Metallicity evolution at 0.8 < z < 2.6 from the LUCI, SINS/zC-SINF and KMOS-3D surveys, , , , , , , , , и 26 other автор(ы). (2014)cite arxiv:1405.6590Comment: 7 pages, 3 figures, submitted to ApJL.The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , и 21 other автор(ы). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.