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Disambiguierung von "van Dokkum, Pieter G."

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ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using CI and CO

, , , , , , , , , , , und . (2017)cite arxiv:1703.05764Comment: Accepted for publication in A&A.
DOI: 10.1051/0004-6361/201730391

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Cornelis Pieter ˜vanœ Andel

Pieter Van der Merwe

Frans G van Lynden

Pieter Wolter

Pieter Zwieten

 

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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 Star-formation Mass Sequence out to z=2.5, , , und . (2012)cite arxiv:1205.0547Comment: Submitted to the Astrophysical Journal Letters, 6 pages, 5 figures. NMBS IR+UV SFRs are now available at http://www.astro.yale.edu/nmbs/Data_Products.html.The number density and mass density of star-forming and quiescent galaxies at 0.4 &lt; z &lt; 2.2, , , , , , , , , und 2 andere Autor(en). (2011)cite arxiv:1104.2595 Comment: Submitted to the Astrophysical Journal. The release of EAZY v2.0 will accompany the publication of the manuscript in the journal.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 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.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.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.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , und 7 andere Autor(en). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.Halpha and 4000 Angstrom Break Measurements for ~3500 K-selected Galaxies at 0.5&lt;z&lt;2.0, , , , , und . (2011)cite arxiv:1103.0279 Comment: Submitted to ApJ, high-resolution version can be downloaded at https://www.cfa.harvard.edu/~mkriek/papers/.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.