M
Mariska Kriek
Researcher at University of California, Berkeley
Publications - 271
Citations - 27298
Mariska Kriek is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 89, co-authored 248 publications receiving 24462 citations. Previous affiliations of Mariska Kriek include Harvard University & Yale University.
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Journal ArticleDOI
An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
Mariska Kriek,Pieter G. van Dokkum,Ivo Labbé,Marijn Franx,Garth D. Illingworth,Danilo Marchesini,Ryan Quadri +6 more
TL;DR: In this paper, the spectrum of a typical quiescent, ultra-dense galaxy at z = 2.1865 with the Gemini Near-Infrared Spectrograph was obtained.
Journal ArticleDOI
3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
Rosalind E. Skelton,Katherine E. Whitaker,Ivelina Momcheva,Gabriel B. Brammer,Pieter G. van Dokkum,Ivo Labbé,Marijn Franx,Arjen van der Wel,Rachel Bezanson,Rachel Bezanson,Elisabete da Cunha,Mattia Fumagalli,Natascha M. Förster Schreiber,Mariska Kriek,Joel Leja,Britt Lundgren,Daniel Magee,Danilo Marchesini,Michael V. Maseda,Erica J. Nelson,Pascal Oesch,Camilla Pacifici,Shannon G. Patel,Sedona H. Price,Hans-Walter Rix,Tomer Tal,David A. Wake,David A. Wake,Stijn Wuyts +28 more
TL;DR: In this paper, a photometric analysis of the CANDELS and 3D-HST HST imaging and the ancillary imaging data at wavelengths 0.3-8 μm is presented, where objects were selected in the WFC3 near-IR bands and their spectral energy distributions were determined by carefully taking the effects of the point-spread function in each observation into account.
Journal ArticleDOI
The Growth of Massive Galaxies Since z = 2
Pieter G. van Dokkum,Pieter G. van Dokkum,Katherine E. Whitaker,Katherine E. Whitaker,Gabriel B. Brammer,Gabriel B. Brammer,Marijn Franx,Mariska Kriek,Mariska Kriek,Ivo Labbé,Ivo Labbé,Danilo Marchesini,Danilo Marchesini,Ryan Quadri,Ryan Quadri,Rachel Bezanson,Garth D. Illingworth,Adam Muzzin,Gregory Rudnick,Gregory Rudnick,Tomer Tal,David A. Wake,David A. Wake +22 more
TL;DR: In this article, the authors study the growth of massive galaxies from z = 2 to the present using data from the NOAO/Yale NewFIRM Medium Band Survey.
Journal ArticleDOI
Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse* **
Pieter G. van Dokkum,Marijn Franx,Mariska Kriek,Bradford P. Holden,Garth D. Illingworth,Daniel Magee,Rychard Bouwens,Danilo Marchesini,Ryan Quadri,Greg Rudnick,Edward N. Taylor,Sune Toft +11 more
TL;DR: In this paper, the authors determined the sizes of these quiescent galaxies using deep, high-resolution images obtained with HST/NIC2 and laser guide star (LGS) assisted Keck/adaptive optics (AO).
Journal ArticleDOI
3D-HST: a wide-field grism spectroscopic survey with the Hubble Space Telescope
Gabriel B. Brammer,Pieter G. van Dokkum,Marijn Franx,Mattia Fumagalli,Shannon G. Patel,Hans-Walter Rix,Rosalind E. Skelton,Mariska Kriek,Erica J. Nelson,Kasper B. Schmidt,Rachel Bezanson,Elisabete da Cunha,Dawn K. Erb,Xiaohui Fan,Natascha M. Förster Schreiber,Garth D. Illingworth,Ivo Labbé,Joel Leja,Britt Lundgren,Dan Magee,Danilo Marchesini,Patrick J. McCarthy,Ivelina Momcheva,Ivelina Momcheva,Adam Muzzin,Ryan Quadri,Charles C. Steidel,Tomer Tal,David Wake,Katherine E. Whitaker,Anna Williams +30 more
TL;DR: 3D-HST as discussed by the authors is a near-infrared spectroscopic Treasury program with the Hubble Space Telescope for studying the physical processes that shape galaxies in the distant universe.