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Disambiguation of "van Dokkum, Pieter"

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The Stellar Initial Mass Function in Early-Type Galaxies from Absorption Line Spectroscopy. III. Radial Gradients

, , , , and . (2016)cite arxiv:1611.09859Comment: Submitted to ApJ. Figure 12 shows the average IMF as a function of radius. Figure 16 compares our results to dynamical and lensing constraints.

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Cornelis Pieter ˜vanœ Andel

Pieter Van der Merwe

Pieter Ploumen

Pieter Dingeldey

Pieter Wolter

 

Other publications of authors with the same name

The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1411.0667Comment: 11 pages, 9 figures. Submitted to MNRAS, comments welcome. The official Illustris website can be found at http://www.illustris-project.org/.The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity, , , , , , , , , and 16 other author(s). (2014)cite arxiv:1406.6056Comment: 19 pages, 17 figures, Resubmitted to ApJ after responding to referee report. Information on ZFOURGE can be found at http://zfourge.tamu.edu.The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.The Initial Mass Function in the Nearest Strong Lenses from SNELLS: Assessing the Consistency of Lensing, Dynamical, and Spectroscopic Constraints, , , , and . (2016)cite arxiv:1612.00065Comment: Submitted to ApJ.Extensive Globular Cluster Systems Associated with Ultra Diffuse Galaxies in the Coma Cluster, , , , , , , , , and . (2017)cite arxiv:1705.08513Comment: Submitted to ApJ Letters. The black and white panels of Figure 1 make the key point of the paper, hopefully.Spatially Resolved Stellar Kinematics of the Ultra-Diffuse Galaxy Dragonfly 44: II. Constraints on Fuzzy Dark Matter, , , , , , , , , and 2 other author(s). (2019)cite arxiv:1905.10373Comment: 15 pages, 11 figures. Submitted to ApJ, comments are welcome!.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.A High Stellar Velocity Dispersion and ~100 Globular Clusters for the Ultra Diffuse Galaxy Dragonfly 44, , , , , , , , and . (2016)cite arxiv:1606.06291Comment: Submitted to ApJ Letters.Forty-Seven Milky Way-Sized, Extremely Diffuse Galaxies in the Coma Cluster, , , , , and . (2014)cite arxiv:1410.8141Comment: Submitted to ApJ Letters. To illustrate how big and fluffy these things are we made a graphic comparing the one with ACS imaging (Fig 4) to several well-known galaxies, if they were at the same distance: http://www.astro.yale.edu/dokkum/coma_udgs/sizes.jpg.The Size Evolution of Star-forming Galaxies Since z~7 Using ZFOURGE, , , , , , , , , and 3 other author(s). (2016)cite arxiv:1612.05262Comment: 7 pages, 4 figures, accepted to Apj letters.