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Disambiguierung von "Skelton, Rosalind E."

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Ages of massive galaxies at $0.5 < z < 2.0$ from 3D-HST rest-frame optical spectroscopy

, , , , , , , , , , , , und . (2016)cite arxiv:1603.02689Comment: 13 pages, 15 figures, accepted for publication in ApJ.

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Rosalind Eugenie Skelton

Rosalind Dépas

Rosalind Egg

Rosalind Elster

Rosalind Heine

 

Weitere Publikationen von Autoren mit dem selben Namen

The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy, , , , , , , , und . (2016)cite arxiv:1608.01674Comment: 14 pages, 11 Figures; Resubmitted to ApJ after addressing referee comments.The Assembly of Milky Way-like Galaxies Since z~2.5, , , , , , , , , und 9 andere Autor(en). (2013)cite arxiv:1304.2391Comment: Submitted to ApJ Letters. 7 pages, 5 figures.Ages of massive galaxies at $0.5 < z < 2.0$ from 3D-HST rest-frame optical spectroscopy, , , , , , , , , und 3 andere Autor(en). (2016)cite arxiv:1603.02689Comment: 13 pages, 15 figures, accepted for publication in ApJ.Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2, , , , , , , , , und 14 andere Autor(en). (2013)cite arxiv:1310.6358Comment: Accepted for publication in ApJL, 5 pages, 1 table, 4 figures.Direct measurement of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates, , , , , , , , , und 5 andere Autor(en). (2013)cite arxiv:1310.4177Comment: Submitted for publication in the Astrophysical Journal.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , und 10 andere Autor(en). (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, , , , , , , , und . (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.Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies, , , , , , , , , und 9 andere Autor(en). (2014)cite arxiv:1401.2984Comment: Submitted to ApJ.Halpha Equivalent Widths from the 3D-HST survey: evolution with redshift and dependence on stellar mass, , , , , , , , , und 5 andere Autor(en). (2012)cite arxiv:1206.2645Comment: Submitted to The Astrophysical Journal Letters.Galaxy Structure as a Driver of the Star Formation Sequence Slope and Scatter, , , , , , , , , und 5 andere Autor(en). (2015)cite arxiv:1508.04771Comment: Accepted for publication in the Astrophysical Journal Letters.