Ghent University Academic Bibliography

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Your filters: cql: author="Whitaker, Katherine" or (type any "bookEditor journalEditor issueEditor" and editor="Whit...

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COSMOS-DASH : the evolution of the galaxy size-mass relation since z ∼ 3 from new wide-field WFC3 imaging combined with CANDELS/3D-HST

Lamiya A Mowla, Pieter van Dokkum, Gabriel B Brammer, Ivelina Momcheva, Arjen van der Wel (UGent) , Katherine Whitaker, Erica Nelson, Rachel Bezanson, Adam Muzzin, Marijn Franx, et al.

(2019) ASTROPHYSICAL JOURNAL. 880(1).
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Molecular gas contents and scaling relations for massive, passive galaxies at intermediate redshifts from the LEGA-C Survey

Justin Spilker, Rachel Bezanson, Ivana Barisic, Eric Bell, Claudia del P Lagos, Michael Maseda, Adam Muzzin, Camilla Pacifici, David Sobral, Caroline Straatman (UGent) , et al.

(2018) ASTROPHYSICAL JOURNAL. 860(2).
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On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 < z < 2.8

Camilla Pacifici, Elisabete da Cunha, Stéphane Charlot, Hans-Walter Rix, Mattia Fumagalli, Arjen van der Wel (UGent) , Marijn Franx, Michael V. Maseda, Pieter G. van Dokkum, Gabriel B. Brammer, et al.

(2015) MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 447(1). p.786-805
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A massive galaxy in its core formation phase three billion years after the Big Bang

Erica Nelson, Pieter van Dokkum, Marijn Franx, Gabriel Brammer, Ivelina Momcheva, Natascha Foerster Schreiber, Elisabete da Cunha, Linda Tacconi, Rachel Bezanson, Allison Kirkpatrick, et al.

(2014) NATURE. 513(7518). p.394-+
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Large-scale star-formation-driven outflows at 1 < z < 2 in the 3D-HST Survey

Britt F Lundgren, Gabriel Brammer, Pieter van Dokkum, Rachel Bezanson, Marijn Franx, Mattia Fumagalli, Ivelina Momcheva, Erica Nelson, Rosalind E Skelton, David Wake, et al.

(2012) ASTROPHYSICAL JOURNAL. 760(1).

Academic Bibliography

COSMOS-DASH : the evolution of the galaxy size-mass relation since z ∼ 3 from new wide-field WFC3 imaging combined with CANDELS/3D-HST

Molecular gas contents and scaling relations for massive, passive galaxies at intermediate redshifts from the LEGA-C Survey

On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 < z < 2.8

A massive galaxy in its core formation phase three billion years after the Big Bang

Large-scale star-formation-driven outflows at 1 < z < 2 in the 3D-HST Survey

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