Ghent University Academic Bibliography

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A nearby galaxy perspective on dust evolution : scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples

Frédéric Galliano, Angelos Nersesian (UGent) , Simone Bianchi, Ilse De Looze (UGent) , Sambit Roychowdhury, Maarten Baes (UGent) , Viviana Casasola, Letizia P. Cassará, Wouter Dobbels, Jacopo Fritz, et al.

(2021) ASTRONOMY & ASTROPHYSICS. 649.
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The case for thermalization as a contributor to the [CII] deficit

Jessica Sutter, Daniel A. Dale, Karin Sandstrom, J. D. T. Smith, Alberto Bolatto, Mederic Boquien, Daniela Calzetti, V Croxall, Kevin, Ilse De Looze (UGent) , Maud Galametz, et al.

(2021) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 503(1). p.911-919
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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, Jacopo Fritz, Maud Galametz, et al.

(2020) ASTRONOMY & ASTROPHYSICS. 641.
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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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Using [CII] 158 mu m emission from isolated ISM phases as a star-formation rate indicator

Jessica Sutter, Daniel A. Dale, Kevin V. Croxall, Eric W. Pelligrini, J. D. T. Smith, Phillip N. Appleton, Pedro Beirao, Alberto D. Bolatto, Daniela Calzetti, Alison Crocker, et al.

(2019) ASTROPHYSICAL JOURNAL. 886(1).
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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 applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types

Ilse De Looze (UGent) , Diane Cormier, Vianney Lebouteiller, Suzanne Madden, Maarten Baes (UGent) , George J Bendo, Médéric Boquien, Alessandro Boselli, David L Clements, Luca Cortese, et al.

(2014) ASTRONOMY & ASTROPHYSICS. 568.
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Dust and gas in the Magellanic clouds from the Heritage Herschel key project, II: gas-to-dust ratio variations across interstellar medium phases

Julia Roman-Duval, Karl Gordon (UGent) , Margaret Meixner, Caroline Bot, Alberto Bolatto, Annie Hughes, Tony Wong, Brian Babler, Jean-Philippe Bernard, Geoffrey C Clayton, et al.

(2014) ASTROPHYSICAL JOURNAL. 797(2).
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Dust and gas in the Magellanic clouds from the Heritage Herschel key project, I: dust properties and insights into the origin of the submillimeter excess emission

Karl Gordon (UGent) , Julia Roman-Duval, Caroline Bot, Margaret Meixner, Brian Babler, Jean-Philippe Bernard, Alberto Bolatto, Martha L Boyer, Geoffrey C Clayton, Charles Engelbracht, et al.

(2014) ASTROPHYSICAL JOURNAL. 797(2).
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Spatially resolved stellar, dust, and gas properties of the post-interacting Whirlpool galaxy system

Erin Mentuch Cooper, Christine D Wilson, Kelly Foyle, George Bendo, Jin Koda, Maarten Baes (UGent) , Médéric Boquien, Alessandro Boselli, Laure Ciesla, Asantha Cooray, et al.

(2012) ASTROPHYSICAL JOURNAL. 755(2).

Academic Bibliography

A nearby galaxy perspective on dust evolution : scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples

The case for thermalization as a contributor to the [CII] deficit

Nonparametric galaxy morphology from UV to submm wavelengths

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

Using [CII] 158 mu m emission from isolated ISM phases as a star-formation rate indicator

The spatially resolved [CII] cooling line deficit in galaxies

The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types

Dust and gas in the Magellanic clouds from the Heritage Herschel key project, II: gas-to-dust ratio variations across interstellar medium phases

Dust and gas in the Magellanic clouds from the Heritage Herschel key project, I: dust properties and insights into the origin of the submillimeter excess emission

Spatially resolved stellar, dust, and gas properties of the post-interacting Whirlpool galaxy system

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