Ghent University Academic Bibliography

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- Journal Article
Dust Attenuation Curves at z ∼ 0.8 from LEGA-C: Precise Constraints on the Slope and 2175Å Bump Strength

Ivana Barišić, Camilla Pacifici, Arjen van der Wel (UGent) , Caroline Straatman (UGent) , Eric F. Bell, Rachel Bezanson, Gabriel Brammer, Francesco D'Eugenio (UGent) , Marijn Franx, Josha van Houdt, et al.

(2020) The Astrophysical Journal.
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- A1
- open access
The CANDELS/SHARDS multiwavelength catalog in GOODS-N : photometry, photometric redshifts, stellar masses, emission-line fluxes, and star formation rates

Guillermo Barro, Pablo G Perez-Gonzalez, Antonio Cava, Gabriel Brammer, Viraj Pandya, Carmen Eliche Moral, Pilar Esquej, Helena Dominguez-Sanchez, Belen Alcalde Pampliega, Yicheng Guo, et al.

(2019) ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 243(2).
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Demographics of star-forming galaxies since z ∼ 2.5, I : the UVJ diagram in CANDELS

Jerome J Fang, SM Faber, David C Koo, Aldo Rodríguez-Puebla, Yicheng Guo, Guillermo Barro, Peter Behroozi, Gabriel Brammer, Zhu Chen, Avishai Dekel, et al.

(2018) ASTROPHYSICAL JOURNAL. 858(2).
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Predicting quiescence : the dependence of specific star formation rate on galaxy size and central density at 0.5 < z < 2.5

Katherine E Whitaker, Rachel Bezanson, Pieter G van Dokkum, Marijn Franx, Arjen van der Wel (UGent) , Gabriel Brammer, Natascha M Foerster-Schreiber, Mauro Giavalisco, Ivo Labbe, Ivelina G Momcheva, et al.

(2017) ASTROPHYSICAL JOURNAL. 838(1).
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Stellar dynamics and star formation histories of z ∼ 1 radio-loud galaxies

Ivana Barišić, Arjen van der Wel (UGent) , Rachel Bezanson, Camilla Pacifici, Kai Noeske, Juan C Muñoz-Mateos, Marijn Franx, Vernesa Smolčić, Eric F Bell, Gabriel Brammer, et al.

(2017) ASTROPHYSICAL JOURNAL. 847(1).
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- A1
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Not in our backyard : spectroscopic support for the CLASH z=11 candidate MACS 0647-JD

Nor Pirzkal, Dan Coe, Brenda L Frye, Gabriel Brammer, John Moustakas, Barry Rothberg, Thomas J Broadhurst, Rychard Bouwens, Larry Bradley, Arjen van der Wel (UGent) , et al.

(2015) ASTROPHYSICAL JOURNAL. 804(1).
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- A1
- open access
Forming compact massive galaxies

Pieter G van Dokkum, Erica June Nelson, Marijn Franx, Pascal Oesch, Ivelina Momcheva, Gabriel Brammer, Natascha M Foerster Schreiber, Rosalind E Skelton, Katherine E Whitaker, Arjen van der Wel (UGent) , et al.

(2015) ASTROPHYSICAL JOURNAL. 813(1).
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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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Dense cores in galaxies out to z=2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fields

Pieter G van Dokkum, Rachel Bezanson, Arjen van der Wel (UGent) , Erica June Nelson, Ivelina Momcheva, Rosalind E Skelton, Katherine E Whitaker, Gabriel Brammer, Charlie Conroy, Natascha M Foerster Schreiber, et al.

(2014) ASTROPHYSICAL JOURNAL. 791(1).
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Exploring the chemical link between local ellipticals and their high-redshift progenitors

Joel Leja, Pieter G. van Dokkum, Ivelina Momcheva, Gabriel Brammer, Rosalind E. Skelton, Katherine E. Whitaker, Brett H. Andrews, Marijn Franx, Mariska Kriek, Arjen van der Wel (UGent) , et al.

(2013) ASTROPHYSICAL JOURNAL LETTERS. 778(2).

Academic Bibliography

Dust Attenuation Curves at z ∼ 0.8 from LEGA-C: Precise Constraints on the Slope and 2175Å Bump Strength

The CANDELS/SHARDS multiwavelength catalog in GOODS-N : photometry, photometric redshifts, stellar masses, emission-line fluxes, and star formation rates

Demographics of star-forming galaxies since z ∼ 2.5, I : the UVJ diagram in CANDELS

Predicting quiescence : the dependence of specific star formation rate on galaxy size and central density at 0.5 < z < 2.5

Stellar dynamics and star formation histories of z ∼ 1 radio-loud galaxies

Not in our backyard : spectroscopic support for the CLASH z=11 candidate MACS 0647-JD

Forming compact massive galaxies

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

Dense cores in galaxies out to z=2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fields

Exploring the chemical link between local ellipticals and their high-redshift progenitors

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