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Disambiguierung von "Nelson, Erica J."

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Confirmation of Small Dynamical and Stellar Masses for Extreme Emission Line Galaxies at z~2

, , , , , , , , , , , , , , , , , , , , , , , und . (2013)cite arxiv:1310.6358Comment: Accepted for publication in ApJL, 5 pages, 1 table, 4 figures.

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Erica Werther

Erica Meyer

Erica Schirmer

Erica Reicherzer

Erica Wünsche

 

Weitere Publikationen von Autoren mit dem selben Namen

Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2, , , , , , , , , und 3 andere Autor(en). (2013)cite arxiv:1305.1943Comment: 6 pages, 4 figures, resubmitted to the Astrophysical Journal Letters after minor revisions.The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , und 21 andere Autor(en). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.First spectroscopic observations of the galaxies that reionized the Universe, , , , , , , , , und 23 andere Autor(en). (2023)cite arxiv:2308.08540Comment: 29 pages, 7 figures, 2 tables.Metallicity evolution at 0.8 < z < 2.6 from the LUCI, SINS/zC-SINF and KMOS-3D surveys, , , , , , , , , und 26 andere Autor(en). (2014)cite arxiv:1405.6590Comment: 7 pages, 3 figures, submitted to ApJL.The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies, , , , , , , , , und 6 andere Autor(en). (2017)cite arxiv:1705.09302Comment: 22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal.The Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , und 20 andere Autor(en). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.Two Remarkably Luminous Galaxy Candidates at $z\approx11-13$ Revealed by JWST, , , , , , , , , und 14 andere Autor(en). (2022)cite arxiv:2207.09434Comment: Submitted to ApJL. Figs. 1 and 2 summarize the candidates, Fig. 3 places the brightness of these systems in context, Fig. 4 shows the morphology, Fig. 5 explores implications for the UVLF. Comments warmly welcomed.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.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.KMOS-3D Reveals Low-Level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7, , , , , , , , , und 16 andere Autor(en). (2017)cite arxiv:1703.07778Comment: 7 pages, 5 figures, submitted to ApJ Letters.