Ghent University Academic Bibliography

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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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The spatially resolved correlation between [NII] 205 µm line emission and the 24 µm continuum in nearby galaxies

Thomas Hughes (UGent) , Maarten Baes (UGent) , MRP Schirm, TJ Parkin, R Wu, Ilse De Looze (UGent) , CD Wilson, Sébastien Viaene (UGent) , GJ Bendo, A Boselli, et al.

(2016) ASTRONOMY & ASTROPHYSICS. 587.
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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).
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The ionized gas in nearby galaxies as traced by the [NII] 122 and 205 µm transitions

R Herrera-Camus, A Bolatto, JD Smith, B Draine, E Pellegrini, M Wolfire, K Croxall, Ilse De Looze (UGent) , D Calzetti, R Kennicutt, et al.

(2016) ASTROPHYSICAL JOURNAL. 826(2).
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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 Herschel exploitation of local galaxy Andromeda (HELGA), VI : the distribution and properties of molecular cloud associations in M31

JM Kirk, WK Gear, Jacopo Fritz (UGent) , MWL Smith, G Ford, Maarten Baes (UGent) , GJ Bendo, Ilse De Looze (UGent) , SA Eales, Gianfranco Gentile (UGent) , et al.

(2015) ASTROPHYSICAL JOURNAL. 798(1).

Academic Bibliography

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

The spatially resolved correlation between [NII] 205 µm line emission and the 24 µm continuum in nearby galaxies

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

The ionized gas in nearby galaxies as traced by the [NII] 122 and 205 µm transitions

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 Herschel exploitation of local galaxy Andromeda (HELGA), VI : the distribution and properties of molecular cloud associations in M31

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