Ghent University Academic Bibliography

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

Marco Martorano (UGent) , Arjen van der Wel (UGent) , Maarten Baes (UGent) , E. F. Bell, G. Brammer, M. Franx, Andrea Gebek (UGent) , Sharon Meidt van der Wel (UGent) , T. B. Miller, E. Nelson, et al.

(2025) ASTRONOMY & ASTROPHYSICS. 694.
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Transforming Galaxies with EASE : widespread structural changes enabled by short-lived spirals

Arjen van der Wel (UGent) and Sharon Meidt van der Wel (UGent)

(2025) ASTRONOMY & ASTROPHYSICS. 704.
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JWST reveals bulge-dominated star-forming galaxies at cosmic noon

Chloë E. Benton, Erica J. Nelson, Tim B. Miller, Rachel Bezanson, Justus Gibson, Abigail I Hartley, Marco Martorano (UGent) , Sedona H. Price, Katherine A. Suess, Arjen van der Wel (UGent) , et al.

(2024) ASTROPHYSICAL JOURNAL LETTERS. 974(2).
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Rest-frame near-infrared radial light profiles up to z = 3 from JWST/NIRCam : wavelength dependence of the Sérsic index

Marco Martorano (UGent) , Arjen van der Wel (UGent) , Eric F. Bell, Marijn Franx, Katherine E. Whitaker, Angelos Nersesian (UGent) , Sedona H. Price, Maarten Baes (UGent) , Katherine A. Suess, Erica J. Nelson, et al.

(2023) ASTROPHYSICAL JOURNAL. 957(1).
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Galaxy kinematics and mass estimates at z ∼ 1 from ionized gas and stars

Junkai Zhang, Stijn Wuyts, Sam E. Cutler, Lamiya A. Mowla, Gabriel B. Brammer, Ivelina G. Momcheva, Katherine E. Whitaker, Pieter van Dokkum, Natascha M. Förster Schreiber, Erica J. Nelson, et al.

(2023) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 524(3). p.4128-4147
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Different higher order kinematics between star-forming and quiescent galaxies based on the SAMI, MAGPI, and LEGA-C surveys

Francesco D'Eugenio (UGent) , Arjen van der Wel (UGent) , Caro Derkenne, Josha van Houdt, Rachel Bezanson, Edward N Taylor, Jesse van de Sande, William M Baker, Eric F Bell, Joss Bland-Hawthorn, et al.

(2023) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 525(2). p.2765-2788
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The multiwavelength properties of red QSOs : evidence for dusty winds as the origin of QSO reddening

G. Calistro Rivera, D. M. Alexander, D. J. Rosario, C. M. Harrison, Marko Stalevski (UGent) , S. Rakshit, V. A. Fawcett, L. K. Morabito, L. Klindt, P. N. Best, et al.

(2021) ASTRONOMY & ASTROPHYSICS. 649.
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ZFIRE :3D modeling of rotation, dispersion, and angular momentum of star-forming galaxies at z ∼ 2

Leo Y Alcorn, Kim-Vy Tran, Karl Glazebrook, Caroline Straatman (UGent) , Michael Cowley, Ben Forrest, Glenn G Kacprzak, Lisa J Kewley, Ivo Labbe, Themiya Nanayakkara, et al.

(2018) ASTROPHYSICAL JOURNAL. 858(1).
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ZFIRE : the evolution of the stellar mass Tully-Fisher relation to redshift ∼ 2.2

Caroline Straatman (UGent) , Karl Glazebrook, Glenn G Kacprzak, Ivo Labbe, Themiya Nanayakkara, Leo Alcorn, Michael Cowley, Lisa J Kewley, Lee R Spitler, Kim-Vy H Tran, et al.

(2017) ASTROPHYSICAL JOURNAL. 839(1).
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Predicting quiescence : the dependence of specific star formation rate on galaxy size and central density at 0.5 < z < 2.5

Katherine E Whitaker, Rachel Bezanson, Pieter G van Dokkum, Marijn Franx, Arjen van der Wel (UGent) , Gabriel Brammer, Natascha M Foerster-Schreiber, Mauro Giavalisco, Ivo Labbe, Ivelina G Momcheva, et al.

(2017) ASTROPHYSICAL JOURNAL. 838(1).

Academic Bibliography

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

Transforming Galaxies with EASE : widespread structural changes enabled by short-lived spirals

JWST reveals bulge-dominated star-forming galaxies at cosmic noon

Rest-frame near-infrared radial light profiles up to z = 3 from JWST/NIRCam : wavelength dependence of the Sérsic index

Galaxy kinematics and mass estimates at z ∼ 1 from ionized gas and stars

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

The multiwavelength properties of red QSOs : evidence for dusty winds as the origin of QSO reddening

ZFIRE :3D modeling of rotation, dispersion, and angular momentum of star-forming galaxies at z ∼ 2

ZFIRE : the evolution of the stellar mass Tully-Fisher relation to redshift ∼ 2.2

Predicting quiescence : the dependence of specific star formation rate on galaxy size and central density at 0.5 < z < 2.5

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