Ghent University Academic Bibliography

Your filters: cql: author="van de Ven, Glenn" or (type any "bookEditor issueEditor" and editor="van de Ven, Glenn")

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Dark matter fraction in disk-like galaxies over the past 10 Gyr

Gauri Sharma, Glenn van de Ven, Paolo Salucci and Marco Martorano (UGent)

(2025) ASTRONOMY & ASTROPHYSICS. 699.
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Stellar half-mass radii of 0.5 z < 2.3 galaxies : comparison with JWST/NIRCam half-light radii

Arjen van der Wel (UGent) , Marco Martorano (UGent) , Boris Häußler, Kalina V. Nedkova, Tim B. Miller, Gabriel B. Brammer, Glenn van de Ven, Joel Leja, Rachel S. Bezanson, Adam Muzzin, et al.

(2024) ASTROPHYSICAL JOURNAL. 960(1).
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The SAMI Galaxy Survey : the internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models

Giulia Santucci, Sarah Brough, Jesse van de Sande, Richard M. McDermid, Glenn van de Ven, Ling Zhu, Francesco D'Eugenio (UGent) , Joss Bland-Hawthorn, Stefania Barsanti, Julia J. Bryant, et al.

(2022) ASTROPHYSICAL JOURNAL. 930(2).
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Deprojecting sersic profiles for arbitrary triaxial shapes : robust measures of intrinsic and projected galaxy sizes

Glenn van de Ven and Arjen van der Wel (UGent)

(2021) ASTROPHYSICAL JOURNAL. 914(1).
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An absence of radio-loud active galactic nuclei in geometrically flat quiescent galaxies : implications for maintenance-mode feedback models

Ivana Barisic, Arjen van der Wel (UGent) , Josha van Houdt, Michael V Maseda, Eric F Bell, Rachel Bezanson, Yu-Yen Chang, Huub Rottgering, Glenn van de Ven and Po-Feng Wu

(2019) ASTROPHYSICAL JOURNAL LETTERS. 872(1).
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Orbital decomposition of CALIFA spiral galaxies

Ling Zhu, Remco van den Bosch, Glenn van de Ven, Mariya Lyubenova, Jesus Falcon-Barroso, Sharon Meidt van der Wel (UGent) , Marie Martig, Juntai Shen, Zhao-Yu Li, Akin Yildirim, et al.

(2018) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 473(3). p.3000-3018
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Being wise II : reducing the influence of star formation history on the mass-to-light ratio of quiescent galaxies

Mark A. Norris, Glenn Van de Ven, Eva Schinnerer, Robert A. Crain, Sharon Meidt van der Wel (UGent) , Brent Groves, Richard G. Bower, Michelle Furlong, Matthieu Schaller, Joop Schaye, et al.

(2016) ASTROPHYSICAL JOURNAL. 832(2).
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The Spitzer survey of stellar structure in galaxies (S⁴G) : precise stellar mass distributions from automated dust correction at 3.6 µm

Miguel Querejeta, Sharon Meidt van der Wel (UGent) , Eva Schinnerer, Mauricio Cisternas, Juan Carlos Munoz-Mateos, Kartik Sheth, Johan Knapen, Glenn Van de Ven, Mark A Norris, Reynier Peletier, et al.

(2015) ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 219(1).
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Being WISE, I : validating stellar population models and M*/L ratios at 3.4 and 4.6 µm

Mark A Norris, Sharon Meidt van der Wel (UGent) , Glenn Van de Ven, Eva Schinnerer, Brent Groves and Miguel Querejeta

(2014) ASTROPHYSICAL JOURNAL. 797(1).
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Reconstructing the stellar mass distributions of galaxies using S⁴G IRAC 3.6 and 4.5 µm images, II : the conversion from light to mass

Sharon Meidt van der Wel (UGent) , Eva Schinnerer, Glenn van de Ven, Dennis Zaritsky, Reynier Peletier, Johan H Knapen, Kartik Sheth, Michael Regan, Miguel Querejeta, Juan-Carlos Munoz-Mateos, et al.

(2014) ASTROPHYSICAL JOURNAL. 788(2).

Academic Bibliography

Dark matter fraction in disk-like galaxies over the past 10 Gyr

Stellar half-mass radii of 0.5 z < 2.3 galaxies : comparison with JWST/NIRCam half-light radii

The SAMI Galaxy Survey : the internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models

Deprojecting sersic profiles for arbitrary triaxial shapes : robust measures of intrinsic and projected galaxy sizes

An absence of radio-loud active galactic nuclei in geometrically flat quiescent galaxies : implications for maintenance-mode feedback models

Orbital decomposition of CALIFA spiral galaxies

Being wise II : reducing the influence of star formation history on the mass-to-light ratio of quiescent galaxies

The Spitzer survey of stellar structure in galaxies (S⁴G) : precise stellar mass distributions from automated dust correction at 3.6 µm

Being WISE, I : validating stellar population models and M*/L ratios at 3.4 and 4.6 µm

Reconstructing the stellar mass distributions of galaxies using S⁴G IRAC 3.6 and 4.5 µm images, II : the conversion from light to mass

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