Ghent University Academic Bibliography

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PHANGS–JWST first results : variations in PAH fraction as a function of ISM phase and metallicity

Jérémy Chastenet (UGent) , Jessica Sutter, Karin Sandstrom, Francesco Belfiore, Oleg V. Egorov, Kirsten L. Larson, Adam K. Leroy, Daizhong Liu, Erik Rosolowsky, David A. Thilker, et al.

(2023) ASTROPHYSICAL JOURNAL LETTERS. 944(2).
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Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo’s third observing run

R. Abbott, T. D. Abbott, S. Abraham, F. Acernese, K. Ackley, A. Adams, C. Adams, R. X. Adhikari, V. B. Adya, C. Affeldt, et al.

(2021) PHYSICAL REVIEW D. 104(2).
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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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Old and young stellar populations in DustPedia galaxies and their role in dust heating

Angelos Nersesian (UGent) , EM Xilouris, S Bianchi, F Galliano, AP Jones, Maarten Baes (UGent) , V Casasola, LP Cassara, CJR Clark, JI Davies, et al.

(2019) ASTRONOMY & ASTROPHYSICS. 624.
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SPICA and the chemical evolution of galaxies : the rise of metals and dust

JA Fernández-Ontiveros, L Armus, Maarten Baes (UGent) , J Bernard-Salas, AD Bolatto, J Braine, L Ciesla, Ilse De Looze (UGent) , E. Egami, J Fischer, et al.

(2017) PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA. 34.
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The origin of [C II] 157 μm emission in a five-component interstellar medium : the case of NGC 3184 and NGC 628

A Abdullah, BR Brandl, B Groves, M Wolfire, D Calzetti, K Croxall, Ilse De Looze (UGent) , RC Kennicutt, KM Sandstrom, L Armus, et al.

(2017) ASTROPHYSICAL JOURNAL. 842(1).
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A portrait of cold gas in galaxies at 60 pc resolution and a simple method to test hypotheses that link small-scale ISM structure to galaxy-scale processes

Adam K. Leroy, Annie Hughes, Andreas Schruba, Erik Rosolowsky, Guillermo A. Blanc, Alberto D. Bolatto, Dario Colombo, Andres Escala, Carsten Kramer, J. M. Diederik Kruijssen, et al.

(2016) ASTROPHYSICAL JOURNAL. 831(1).
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The bright end of the z ∼ 9 and z ∼ 10 UV luminosity functions using all five CANDELS fields

RJ Bouwens, PA Oesch, I Labbe, GD Illingworth, GG Fazio, D Coe, B Holwerda, R Smit, M Stefanon, PG van Dokkum, et al.

(2016) ASTROPHYSICAL JOURNAL. 830(2).
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UV to IR luminosities and dust attenuation determined from ∼4000 K-selected galaxies at 1 < z < 3 in the zFourGE survey

Ben Forrest, Kim-Vy H Tran, Adam R Tomczak, Adam Broussard, Ivo Labbe, Casey Papovich, Mariska Kriek, Rebecca J Allen, Michael Cowley, Mark Dickinson, et al.

(2016) ASTROPHYSICAL JOURNAL LETTERS. 818(2).
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The spatially resolved [CII] cooling line deficit in galaxies

JDT Smith, Kevin Croxall, Bruce Draine, Ilse De Looze (UGent) , Karin Sandstrom, Lee Armus, Pedro Beirão, Alberto Bolatto, Mederic Boquien, Bernhard Brandl, et al.

(2016) ASTROPHYSICAL JOURNAL. 834(1).

Academic Bibliography

PHANGS–JWST first results : variations in PAH fraction as a function of ISM phase and metallicity

Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo’s third observing run

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

Old and young stellar populations in DustPedia galaxies and their role in dust heating

SPICA and the chemical evolution of galaxies : the rise of metals and dust

The origin of [C II] 157 μm emission in a five-component interstellar medium : the case of NGC 3184 and NGC 628

A portrait of cold gas in galaxies at 60 pc resolution and a simple method to test hypotheses that link small-scale ISM structure to galaxy-scale processes

The bright end of the z ∼ 9 and z ∼ 10 UV luminosity functions using all five CANDELS fields

UV to IR luminosities and dust attenuation determined from ∼4000 K-selected galaxies at 1 < z < 3 in the zFourGE survey

The spatially resolved [CII] cooling line deficit in galaxies

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