Ghent University Academic Bibliography

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Your filters: cql: author="Santini, P" or (type any "bookEditor journalEditor issueEditor" and editor="Santini, P")

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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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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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Tracing the evolution of dust obscured star formation and accretion back to the reionisation epoch with SPICA

C Gruppioni, L Ciesla, E Hatziminaoglou, F Pozzi, G Rodighiero, P Santini, L Armus, Maarten Baes (UGent) , J Braine, V Charmandaris, et al.

(2017) PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA. 34.
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Galaxy evolution studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA) : the power of IR spectroscopy

L Spinoglio, A Alonso-Herrero, L Armus, Maarten Baes (UGent) , J Bernard-Salas, S Bianchi, M Bocchio, A Bolatto, C Bradford, J Braine, et al.

(2017) PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA. 34.
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- Journal Article
- A1
- open access
CANDELS+3D-HST : compact SFGs at z ∼ 2-3, the progenitors of the first quiescent galaxies

G Barro, SM Faber, PG Perez-Gonzalez, C Pacifici, JR Trump, DC Koo, S Wuyts, Y Guo, E Bell, A Dekel, et al.

(2014) ASTROPHYSICAL JOURNAL. 791(1).

Academic Bibliography

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

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

Tracing the evolution of dust obscured star formation and accretion back to the reionisation epoch with SPICA

Galaxy evolution studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA) : the power of IR spectroscopy

CANDELS+3D-HST : compact SFGs at z ∼ 2-3, the progenitors of the first quiescent galaxies

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