2014 - Hellman Fellow
Her primary scientific interests are in Astrophysics, Galaxy, Redshift, Astronomy and Galaxy formation and evolution. Her study in the field of Luminous infrared galaxy, Elliptical galaxy, Radio galaxy and Velocity dispersion is also linked to topics like Spectral density. Her research integrates issues of Stars and Emission spectrum in her study of Galaxy.
Her Redshift study combines topics from a wide range of disciplines, such as Number density, Spectral line and Photometry. Her biological study spans a wide range of topics, including Luminosity and Mass–luminosity relation. Her Star formation study incorporates themes from Doubly ionized oxygen and Surface brightness.
Her main research concerns Astrophysics, Galaxy, Redshift, Star formation and Stellar mass. Astrophysics connects with themes related to Astronomy in her study. Her work focuses on many connections between Galaxy and other disciplines, such as Balmer series, that overlap with her field of interest in Equivalent width.
In her study, Infrared is inextricably linked to Photometry, which falls within the broad field of Redshift. Her work investigates the relationship between Star formation and topics such as Effective radius that intersect with problems in Radius. Her Stellar mass research is multidisciplinary, relying on both Baryon, Active galactic nucleus, Luminosity, Surface brightness and Sigma.
Mariska Kriek mostly deals with Astrophysics, Galaxy, Redshift, Metallicity and Stellar mass. Her Astrophysics study frequently draws connections between related disciplines such as Spectral line. Mariska Kriek interconnects Ionization and Balmer series in the investigation of issues within Galaxy.
The concepts of her Redshift study are interwoven with issues in Star, Spectroscopy, Interstellar medium, Spitzer Space Telescope and Sigma. As part of one scientific family, Mariska Kriek deals mainly with the area of Stellar mass, narrowing it down to issues related to the Submillimeter Array, and often Hubble Ultra-Deep Field. Galaxy formation and evolution is the subject of her research, which falls under Astronomy.
Her scientific interests lie mostly in Galaxy, Astrophysics, Redshift, Metallicity and Star formation. Her work on Stellar population as part of general Galaxy research is often related to Context, thus linking different fields of science. Her Astrophysics study often links to related topics such as Emission spectrum.
Her study in Redshift is interdisciplinary in nature, drawing from both Star, Spectral line, Ionization, Interstellar medium and Stellar mass. Her Stellar mass research incorporates themes from Baryon and Optical spectra. Her Metallicity research includes themes of X-ray binary, Luminosity, Hubble Deep Field and Reionization.
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
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.
The Astrophysical Journal (2009)
The Growth of Massive Galaxies Since z = 2
Pieter G. van Dokkum;Pieter G. van Dokkum;Katherine E. Whitaker;Katherine E. Whitaker;Gabriel Brammer;Gabriel Brammer;Marijn Franx.
The Astrophysical Journal (2010)
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 Holden.
The Astrophysical Journal (2008)
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 G. Momcheva;Gabriel B. Brammer.
Astrophysical Journal Supplement Series (2014)
The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxies
Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. van Dokkum;Rosalind E. Skelton.
arXiv: Astrophysics of Galaxies (2015)
3D-HST: a wide-field grism spectroscopic survey with the Hubble Space Telescope
Gabriel B. Brammer;Pieter G. Van Dokkum;Marijn Franx;Mattia Fumagalli.
Astrophysical Journal Supplement Series (2012)
THE 3D-HST SURVEY: HUBBLE SPACE TELESCOPE WFC3/G141 GRISM SPECTRA, REDSHIFTS, AND EMISSION LINE MEASUREMENTS FOR ∼100,000 GALAXIES
Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. Van Dokkum;Rosalind E. Skelton.
Astrophysical Journal Supplement Series (2016)
The number density and mass density of star-forming and quiescent galaxies at 0.4 < z < 2.2
Gabriel B. Brammer;Katherine E. Whitaker;Pieter G. van Dokkum;Danilo Marchesini.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
THE RELATION BETWEEN COMPACT, QUIESCENT HIGH-REDSHIFT GALAXIES AND MASSIVE NEARBY ELLIPTICAL GALAXIES: EVIDENCE FOR HIERARCHICAL, INSIDE-OUT GROWTH
Rachel Bezanson;Pieter G. van Dokkum;Tomer Tal;Danilo Marchesini.
The Astrophysical Journal (2009)
THE NEWFIRM MEDIUM-BAND SURVEY: PHOTOMETRIC CATALOGS, REDSHIFTS, AND THE BIMODAL COLOR DISTRIBUTION OF GALAXIES OUT TO z ∼ 3
Katherine E. Whitaker;Katherine E. Whitaker;Ivo Labbé;Ivo Labbé;Pieter G. van Dokkum;Pieter G. van Dokkum;Gabriel Brammer;Gabriel Brammer;Gabriel Brammer.
The Astrophysical Journal (2011)
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