Arjen van der Wel

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Ghent University

Belgium

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Arjen van der Wel is a Professor at Ghent University in Belgium. His research focuses on topics related to galaxy evolution, stellar properties, and observational astronomy, as evidenced by his recent publications on the evolution of galaxies up to redshift z = 2.5 and the analysis of UV-millimeter emissions in star-forming regions. He is actively involved in preparing for the Euclid space mission and has contributed to enhancing the understanding of the mass-dependent UVJ diagram and the properties of quiescent galaxies.

Recent Grants

Grant: Close

The Physics of Galaxies 7 Gyr Ago

Open Date: 2016-04-01

Close Date: 2021-03-31

Grant: Close

The Physical Properties of Galaxies 7 Billion Years Ago

Open Date: 2015-01-01

Close Date:

Arjen van der Wel

Research Interests

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About

Recent Grants

Articles (27)

Even redder than we knew: Color and AV evolution up to z = 2.5 from JWST/NIRCam photometry

Euclid preparation

More is better: Strong constraints on the stellar properties of LEGA-C z ∼ 1 galaxies with Prospector

The mass-dependent UVJ diagram at cosmic noon

Evolution of the Sérsic index up to z = 2.5 from JWST and HST

The hyperplane of early-type galaxies: using stellar population properties to increase the precision and accuracy of the fundamental plane as a distance indicator

The Size–Mass Relation at Rest-frame 1.5 μm from JWST/NIRCam in the COSMOS-WEB and PRIMER-COSMOS Fields

3D-DASH: The Evolution of Size, Shape, and Intrinsic Scatter in Populations of Young and Old Quiescent Galaxies at 0.5 < z < 3

The many colours of the TNG100 simulation

Bottom’s Dream and the Amplification of Filamentary Gas Structures and Stellar Spiral Arms

The TNG50-SKIRT Atlas: Post-processing methodology and first data release

A Census of Star Formation Histories of Massive Galaxies at 0.6 < z < 1 from Spectrophotometric Modeling Using Bagpipes and Prospector

Stellar Half-mass Radii of 0.5 z < 2.3 Galaxies: Comparison with JWST/NIRCam Half-light Radii

TODDLERS: A new UV-millimeter emission library for star-forming regions

JWST Reveals Bulge-dominated Star-forming Galaxies at Cosmic Noon

From Carbon to Cobalt: Chemical Compositions and Ages of z ∼ 0.7 Quiescent Galaxies

A Simple Spectroscopic Technique to Identify Rejuvenating Galaxies

The Gas and Stellar Content of a Metal-poor Galaxy at z = 8.496 as Revealed by JWST and ALMA

Different higher order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI, and LEGA-C surveys

Evolution in the orbital structure of quiescent galaxies from MAGPI, LEGA-C, and SAMI surveys: direct evidence for merger-driven growth over the last 7 Gyr

When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multiband Imaging Data

Rest-frame Near-infrared Radial Light Profiles up to z = 3 from JWST/NIRCam: Wavelength Dependence of the Sérsic Index

Stars, Gas, and Star Formation of Distant Post-starburst Galaxies

Galaxy And Mass Assembly (GAMA)

The Velocity Dispersion Function for Massive Quiescent and Star-forming Galaxies at 0.6 < z ≤ 1.0

The Mass Scale of High-redshift Galaxies: Virial Mass Estimates Calibrated with Stellar Dynamical Models from LEGA-C

Staring at the Shadows of Archaic Galaxies: Damped Lyα and Metal Absorbers Toward a Young z ∼ 6 Weak-line Quasar

Collaborators (21)

Matthew Colless

Amelia Fraser-McKelvie

Joel Leja

Katherine Whitaker

Sabine Thater

Peter Camps

Thomas R. Greve

David Sobral

Bunyo Hatsukade

Stijn Wuyts

Daniel Weisz

Antonio La Marca

Gabriel Brammer

Angus H Wright

Joss Bland-Hawthorn

Matt Owers

Gourav Khullar

Sharon Meidt

Angel Lopez-Sanchez

Steven Gillman

Aswin Vijayan

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