Ghent University Academic Bibliography

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Evidence of dust grain evolution from extinction mapping in the IC 63 photodissociation region

Dries Van De Putte (UGent) , Karl Gordon (UGent) , Julia Roman-Duval, Benjamin F Williams, Maarten Baes (UGent) , Kirill Tchernyshyov, Brandon L Lawton and Heddy Arab

(2020) ASTROPHYSICAL JOURNAL. 888(1).
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SKIRT 9: Redesigning an advanced dust radiative transfer code to allow kinematics, line transfer and polarization by aligned dust grains

Peter Camps (UGent) and Maarten Baes (UGent)

(2020) ASTRONOMY AND COMPUTING. 31.
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High-resolution, 3D radiative transfer modelling. II : the early-type spiral galaxy M 81

Sam Verstocken, Angelos Nersesian (UGent) , Maarten Baes (UGent) , Sébastien Viaene (UGent) , Simone Bianchi, Viviana Casasola, Christopher J. R. Clark, Jonathan I. Davies, Ilse De Looze (UGent) , Pieter De Vis, et al.

(2020) ASTRONOMY & ASTROPHYSICS. 637.
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Reproducing the Universe : a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample

Ana Trčka (UGent) , Maarten Baes (UGent) , Peter Camps (UGent) , Sharon Meidt van der Wel (UGent) , James Trayford, Simone Bianchi, Viviana Casasola, Letizia P Cassarà, Ilse De Looze (UGent) , Pieter De Vis, et al.

(2020) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 494. p.2823-2838
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Infrared luminosity functions and dust mass functions in the EAGLE simulation

Maarten Baes (UGent) , Ana Trčka (UGent) , Peter Camps (UGent) , James Trayford, Antonios Katsianis, Lucia Marchetti, Tom Theuns, Mattia Vaccari and Bert Vandenbroucke (UGent)

(2020) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 494(2). p.2912-2924
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AlFoCS + Fornax3D : resolved star formation in the Fornax cluster with ALMA and MUSE

N Zabel, T A Davis, M Sarzi, Boris Nedelchev, M Chevance, J M Diederik Kruijssen, E Iodice, Maarten Baes (UGent) , G J Bendo, E Maria Corsini, et al.

(2020) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 496(2). p.2155-2182
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Nonparametric galaxy morphology from UV to submm wavelengths

Maarten Baes (UGent) , Angelos Nersesian (UGent) , Viviana Casasola, Simone Bianchi, Letizia P. Cassarà, Christopher J. R. Clark, Ilse De Looze (UGent) , Wouter Dobbels (UGent) , Jacopo Fritz, Maud Galametz, et al.

(2020) ASTRONOMY & ASTROPHYSICS. 641.
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VALES. VII. Molecular and ionized gas properties in the pressure balanced interstellar medium of starburst galaxies at z ∼ 0.15

Juan Molina, Edo Ibar, Nicolás Godoy, Andrés Escala, Tomonari Michiyama, Cheng Cheng, Thomas M. Hughes, Maarten Baes (UGent) , Yongquan Xue, Michał J. Michałowski, et al.

(2020) ASTRONOMY & ASTROPHYSICS. 643.
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High-resolution, 3D radiative transfer modelling : V. A detailed model of the M 51 interacting pair

Angelos Nersesian (UGent) , Sébastien Viaene (UGent) , Ilse De Looze (UGent) , Maarten Baes (UGent) , Emmanuel M. Xilouris, Matthew W. L. Smith, Simone Bianchi, Viviana Casasola, Letizia P. Cassarà, Christopher J. R. Clark, et al.

(2020) ASTRONOMY & ASTROPHYSICS. 643.
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CosTuuM : polarized thermal dust emission by magnetically oriented spheroidal grains

Bert Vandenbroucke (UGent) , Maarten Baes (UGent) and Peter Camps (UGent)

(2020) ASTRONOMICAL JOURNAL. 160(1).

Academic Bibliography

Evidence of dust grain evolution from extinction mapping in the IC 63 photodissociation region

SKIRT 9: Redesigning an advanced dust radiative transfer code to allow kinematics, line transfer and polarization by aligned dust grains

High-resolution, 3D radiative transfer modelling. II : the early-type spiral galaxy M 81

Reproducing the Universe : a comparison between the EAGLE simulations and the nearby DustPedia galaxy sample

Infrared luminosity functions and dust mass functions in the EAGLE simulation

AlFoCS + Fornax3D : resolved star formation in the Fornax cluster with ALMA and MUSE

Nonparametric galaxy morphology from UV to submm wavelengths

VALES. VII. Molecular and ionized gas properties in the pressure balanced interstellar medium of starburst galaxies at z ∼ 0.15

High-resolution, 3D radiative transfer modelling : V. A detailed model of the M 51 interacting pair

CosTuuM : polarized thermal dust emission by magnetically oriented spheroidal grains

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