( en | de | ru )

 

Disambiguation of "Skelton, Rosalind"

Author of the publication

copydeleteadd this publication to your clipboard
The Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST Survey

, , , , , , , , , , , , , , , , , , and . (2013)cite arxiv:1301.0320Comment: Accepted for publication in ApJ Letters.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed. You can also use the button next to the name to display some publications already assigned to the person.

Rosalind Eugenie Skelton

Rosalind Dépas

Rosalind Egg

Rosalind Elster

Rosalind Heine

 

Other publications of authors with the same name

Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2, , , , , , , , , and 3 other author(s). (2013)cite arxiv:1305.1943Comment: 6 pages, 4 figures, resubmitted to the Astrophysical Journal Letters after minor revisions.The Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST Survey, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1301.0320Comment: Accepted for publication in ApJ Letters.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 Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy, , , , , , , , and . (2016)cite arxiv:1608.01674Comment: 14 pages, 11 Figures; Resubmitted to ApJ after addressing referee comments.Ages of massive galaxies at $0.5 < z < 2.0$ from 3D-HST rest-frame optical spectroscopy, , , , , , , , , and 3 other author(s). (2016)cite arxiv:1603.02689Comment: 13 pages, 15 figures, 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, , , , , , , , , 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.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.Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2, , , , , , , , , and 14 other author(s). (2013)cite arxiv:1310.6358Comment: Accepted for publication in ApJL, 5 pages, 1 table, 4 figures.Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies, , , , , , , , , and 9 other author(s). (2014)cite arxiv:1401.2984Comment: Submitted to ApJ.