What is she best known for?
The fields of study she is best known for:
- Galaxy
- Astronomy
- Astrophysics
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 most cited work include:
- An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2 (946 citations)
- Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse* ** (747 citations)
- The Growth of Massive Galaxies Since z = 2 (736 citations)
What are the main themes of her work throughout her whole career to date?
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.
She most often published in these fields:
- Astrophysics (117.33%)
- Galaxy (107.22%)
- Redshift (68.23%)
What were the highlights of her more recent work (between 2017-2021)?
- Astrophysics (117.33%)
- Galaxy (107.22%)
- Redshift (68.23%)
In recent papers she was focusing on the following fields of study:
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.
Between 2017 and 2021, her most popular works were:
- The MOSDEF Survey: A Stellar Mass-SFR-Metallicity Relation Exists at z ∼ 2.3 (67 citations)
- The MOSDEF Survey: Direct Observational Constraints on the Ionizing Photon Production Efficiency, ξ ion, at z ∼ 2 (66 citations)
- COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation Since z~3 from new Wide Field WFC3 Imaging Combined with CANDELS/3DHST (45 citations)
In her most recent research, the most cited papers focused on:
- Galaxy
- Astronomy
- Milky Way
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.
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