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Disambiguation of "van Dokkum, Pieter G."

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Galaxy Structure as a Driver of the Star Formation Sequence Slope and Scatter

, , , , , , , , , , , , , , and . (2015)cite arxiv:1508.04771Comment: Accepted for publication in the Astrophysical Journal Letters.

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Cornelis Pieter ˜vanœ Andel

Pieter Van der Merwe

Frans G van Lynden

Pieter Ploumen

Pieter Dingeldey

 

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 Star-formation Mass Sequence out to z=2.5, , , and . (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 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 HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies, , , , , , , , , and 6 other author(s). (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$^3D$, , , , , , , , , and 20 other author(s). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.The number density and mass density of star-forming and quiescent galaxies at 0.4 &lt; z &lt; 2.2, , , , , , , , , and 2 other author(s). (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.Halpha and 4000 Angstrom Break Measurements for ~3500 K-selected Galaxies at 0.5&lt;z&lt;2.0, , , , , and . (2011)cite arxiv:1103.0279 Comment: Submitted to ApJ, high-resolution version can be downloaded at https://www.cfa.harvard.edu/~mkriek/papers/.First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5 < z < 2$ from KMOS, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1503.08831Comment: 6 pages, 5 figures, accepted for publication in ApJL.ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using CI and CO, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1703.05764Comment: Accepted for publication in A&A.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.