Ghent University Academic Bibliography

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The LEGA-C and SAMI galaxy surveys : quiescent stellar populations and the mass-size plane across 6 Gyr

Tania M. Barone, Francesco D'Eugenio (UGent) , Nicholas Scott, Matthew Colless, Sam P. Vaughan, Arjen van der Wel (UGent) , Amelia Fraser-McKelvie, Anna de Graaff, Jesse van de Sande, Po-Feng Wu, et al.

(2022) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 512(3). p.3828-3845
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Frequency and nature of central molecular outflows in nearby star-forming disk galaxies

Sophia K. Stuber, Toshiki Saito, Eva Schinnerer, Eric Emsellem, Miguel Querejeta, Thomas G. Williams, Ashley T. Barnes, Frank Bigiel, Guillermo Blanc, Daniel A. Dale, et al.

(2021) ASTRONOMY & ASTROPHYSICS. 653.
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Exploring the origin of ultra-diffuse galaxies in clusters from their primordial alignment

Yu Rong, Pavel E. Mancera Piña, Elmo Tempel, Thomas H. Puzia and Sven De Rijcke (UGent)

(2020) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 498(1). p.L72-L76
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Link between radio-loud AGNs and host-galaxy shape

X. C. Zheng, H. J. A. Röttgering, P. N. Best, Arjen van der Wel (UGent) , M. J. Hardcastle, W. L. Williams, M. Bonato, I. Prandoni, D. J. B. Smith and S. K. Leslie

(2020) ASTRONOMY & ASTROPHYSICS. 644.
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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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Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?

Viraj Pandya, Joel Primack, Peter Behroozi, Avishai Dekel, Haowen Zhang, Elliot Eckholm, Sandra M. Faber, Henry C. Ferguson, Mauro Giavalisco, Yicheng Guo, et al.

(2019) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 488(4). p.5580-5593
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Near infrared spectroscopy and star-formation histories of 3 ≤ z ≤ 4 quiescent galaxies

C Schreiber, K Glazebrook, T Nanayakkara, GG Kacprzak, I Labbe, P Oesch, T Yuan, K-V Tran, C Papovich, L Spitler, et al.

(2018) ASTRONOMY & ASTROPHYSICS. 618.
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The number density evolution of extreme emission line galaxies in 3D-HST : results from a novel automated line search technique for slitless spectroscopy

Michael V Maseda, Arjen van der Wel (UGent) , Hans-Walter Rix, Ivelina Momcheva, Gabriel B Brammer, Marijn Franx, Britt F Lundgren, Rosalind E Skelton and Katherine E Whitaker

(2018) ASTROPHYSICAL JOURNAL. 854(1).
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GAMA/H-ATLAS : the local dust mass function and cosmic density as a function of galaxy type : a benchmark for models of galaxy evolution

RA Beeston, AH Wright, S Maddox, HL Gomez, L Dunne, SP Driver, A Robotham, CJR Clark, K Vinsen, TT Takeuchi, et al.

(2018) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 479. p.1077-1099
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Satellite quenching and galactic conformity at 0.3 < z < 2.5

Lalitwadee Kawinwanichakij, Ryan F Quadri, Casey Papovich, Glenn G Kacprzak, Ivo Labbe, Lee R Spitler, Caroline Straatman (UGent) , Kim-Vy H Tran, Rebecca Allen, Peter Behroozi, et al.

(2016) ASTROPHYSICAL JOURNAL. 817(1).

Academic Bibliography

The LEGA-C and SAMI galaxy surveys : quiescent stellar populations and the mass-size plane across 6 Gyr

Frequency and nature of central molecular outflows in nearby star-forming disk galaxies

Exploring the origin of ultra-diffuse galaxies in clusters from their primordial alignment

Link between radio-loud AGNs and host-galaxy shape

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

Can intrinsic alignments of elongated low-mass galaxies be used to map the cosmic web at high redshift?

Near infrared spectroscopy and star-formation histories of 3 ≤ z ≤ 4 quiescent galaxies

The number density evolution of extreme emission line galaxies in 3D-HST : results from a novel automated line search technique for slitless spectroscopy

GAMA/H-ATLAS : the local dust mass function and cosmic density as a function of galaxy type : a benchmark for models of galaxy evolution

Satellite quenching and galactic conformity at 0.3 < z < 2.5

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