Ghent University Academic Bibliography

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The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators : towards addressing the tension between observations and simulations

A. Katsianis, V. Gonzalez, Daniela Barrientos Acevedo (UGent) , X. Yang, C. D. P. Lagos, J. Schaye, Peter Camps (UGent) , Ana Trčka (UGent) , Maarten Baes (UGent) , Marko Stalevski (UGent) , et al.

(2020) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 492(4). p.5592-5606
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VALES V : a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z ∼ 0.03-0.35 using ALMA

J Molina, Edo Ibar, V Villanueva, A Escala, C Cheng, Maarten Baes (UGent) , H Messias, C Yang, FE Bauer, . van der Werf, et al.

(2019) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 482(2). p.1499-1524
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Rejuvenation in z ∼ 0.8 quiescent galaxies in LEGA-C

Priscilla Chauke, Arjen van der Wel (UGent) , Camilla Pacifici, Rachel Bezanson, Po-Feng Wu, Anna Gallazzi, Caroline Straatman (UGent) , Marijn Franx, Ivana Barisic, Eric F Bell, et al.

(2019) ASTROPHYSICAL JOURNAL. 877(1).
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HST/WFC3 grism observations of z ∼ 1 clusters : the cluster versus field stellar mass-size relation and evidence for size growth of quiescent galaxies from minor mergers

J Matharu, A Muzzin, GB Brammer, RFJ van der Burg, MW Auger, PC Hewett, Arjen van der Wel (UGent) , P van Dokkum, M Balogh, JCC Chan, et al.

(2019) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 484(1). p.595-617
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Dense gas is not enough : environmental variations in the star formation efficiency of dense molecular gas at 100 pc scales in M 51

M Querejeta, E Schinnerer, A Schruba, E Murphy, Sharon Meidt van der Wel (UGent) , A Usero, AK Leroy, J Pety, F Bigiel, M Chevance, et al.

(2019) ASTRONOMY & ASTROPHYSICS. 625.
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The spatial relation between young star clusters and molecular clouds in M51 with LEGUS

K Grasha, D Calzetti, A Adamo, RC Kennicutt, BG Elmegreen, M Messa, DA Dale, K Fedorenko, S Mahadevan, EK Grebel, et al.

(2019) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 483(4). p.4707-4723
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Comprehensive comparison of models for spectral energy distributions from 0.1 μm to 1 mm of nearby star-forming galaxies

LK Hunt, Ilse De Looze (UGent) , M Boquien, R Nikutta, A Rossi, S Bianchi, DA Dale, GL Granato, RC Kennicutt, L Silva, et al.

(2019) ASTRONOMY & ASTROPHYSICS. 621.
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First results from the TNG50 simulation : the evolution of stellar and gaseous discs across cosmic time

Annalisa Pillepich, Dylan Nelson, Volker Springel, Rüdiger Pakmor, Paul Torrey, Rainer Weinberger, Mark Vogelsberger, Federico Marinacci, Shy Genel, Arjen van der Wel (UGent) , et al.

(2019) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 490(3). p.3196-3233
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An evolving and mass-dependent σsSFR-M* relation for galaxies

Antonios Katsianis, Xianzhong Zheng, Valentino Gonzalez, Guillermo Blanc, Claudia del P Lagos, Luke JM Davies, Peter Camps (UGent) , Ana Trčka (UGent) , Maarten Baes (UGent) , Joop Schaye, et al.

(2019) ASTROPHYSICAL JOURNAL. 879(1).
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High-resolution radiative transfer modelling of M33

Thomas G Williams, Maarten Baes (UGent) , Ilse De Looze (UGent) , Monica Relaño, Matthew WL Smith, Sam Verstocken (UGent) and Sébastien Viaene (UGent)

(2019) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 487(2). p.2753-2770

Academic Bibliography

The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators : towards addressing the tension between observations and simulations

VALES V : a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z ∼ 0.03-0.35 using ALMA

Rejuvenation in z ∼ 0.8 quiescent galaxies in LEGA-C

HST/WFC3 grism observations of z ∼ 1 clusters : the cluster versus field stellar mass-size relation and evidence for size growth of quiescent galaxies from minor mergers

Dense gas is not enough : environmental variations in the star formation efficiency of dense molecular gas at 100 pc scales in M 51

The spatial relation between young star clusters and molecular clouds in M51 with LEGUS

Comprehensive comparison of models for spectral energy distributions from 0.1 μm to 1 mm of nearby star-forming galaxies

First results from the TNG50 simulation : the evolution of stellar and gaseous discs across cosmic time

An evolving and mass-dependent σsSFR-M* relation for galaxies

High-resolution radiative transfer modelling of M33

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