Pieter G. van Dokkum
Yale University
400 Papers
9.8K Citations
Pieter G. van Dokkum is an academic researcher from Yale University. The author has contributed to research in topics: Galaxy & Stellar mass. The author has an hindex of 99, co-authored 318 publications. Previous affiliations of Pieter G. van Dokkum include Association of Universities for Research in Astronomy & California Institute of Technology.
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Papers
Evolution of Quiescent and Star-forming Galaxies since z ~ 1.5 as a Function of their Velocity Dispersions
TL;DR: In this article, the authors measured stellar masses and structural parameters for 5500 quiescent and 20,000 star-forming galaxies at 0.3 < z ≤ 1.5 in the Newfirm Medium Band Survey COSMOS and UKIDSS UDS fields.
Evidence of Absence of Tidal Features in the Outskirts of Ultra Diffuse Galaxies in the Coma Cluster
TL;DR: In this paper, the presence of tidal features associated with ultra diffuse galaxies (UDGs) in galaxy clusters is studied. But the authors focus on the Coma cluster and do not consider the other galaxies in the Yagi et al. 2016 catalog.
The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity
Lalitwadee Kawinwanichakij,Casey Papovich,Ryan Quadri,Kim-Vy Tran,Lee R. Spitler,Glenn G. Kacprzak,Glenn G. Kacprzak,Ivo Labbé,Caroline M. S. Straatman,Karl Glazebrook,Rebecca Allen,Michael J. Cowley,Romeel Davé,Romeel Davé,Avishai Dekel,Henry C. Ferguson,William G. Hartley,William G. Hartley,Anton M. Koekemoer,David C. Koo,Yu Lu,Nicola Mehrtens,Themiya Nanayakkara,S. Eric Persson,Glen Rees,Brett Salmon,Vithal Tilvi,Adam Tomczak,Pieter G. van Dokkum +28 more
TL;DR: In this paper, the authors study the statistical distribution of satellites around star-forming and quiescent central galaxies at 1 9$ at z 10.78 and find no statistical difference in the satellite distributions of intermediate-mass quiescents and starforming centrals.
Assessing the Predictive Power of Galaxy Formation Models: A Comparison of Predicted and Observed Rest-Frame Optical Luminosity Functions at 2.0 ≤ z ≤ 3.3
TL;DR: In this article, the authors compare the results of the Bower et al. model with the observed rest-frame V-band luminosity density of galaxies at redshifts 2.0 ≤ z ≤ 3.3 to predictions of semianalytic models.
Peer Review
The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization
Rachel Bezanson,Ivo Labbé,Katherine E. Whitaker,Joel Leja,Sedona H. Price,Marijn Franx,Gabriel B. Brammer,Danilo Marchesini,Adi Zitrin,Bingjie Wang,John R. Weaver,Lukas J. Furtak,Hakim Atek,Dan Coe,Sam Cutler,Pratika Dayal,Pieter G. van Dokkum,Robert Feldmann,N. M. Förster Schreiber,Seiji Fujimoto,Marla Geha,Karl Glazebrook,Anna de Graaff,Jenny E. Greene,Stéphanie Juneau,Susan A. Kassin,Mariska Kriek,G. Khullar,Michael V. Maseda,Lamiya Mowla,Adam Muzzin,Themiya Nanayakkara,Erica J. Nelson,Pascal Oesch,Camilla Pacifici,Richard Pan,Casey Papovich,David Setton,Alice E. Shapley,Renske Smit,Mauro Stefanon,Edward N. Taylor,D. C. Williams +42 more
- 08 Dec 2022
TL;DR: In this paper , the authors describe the survey design for the Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program, which executed its early imaging component in November 2022.