Corentin Schreiber

Affiliations: 
2015 Université Paris-Saclay, Gif-sur-Yvette, Essonne, France 
Website:
https://www.universiteitleiden.nl/en/staffmembers/corentin-schreiber
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"Corentin Schreiber"
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Cross-listing: Astronomy Tree

Parents

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David Elbaz grad student 2015 Université Paris-Saclay
 (Étude statistique et multi-longueurs-d'onde de la formation d'étoiles dans les galaxies)
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Publications

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Nanayakkara T, Glazebrook K, Jacobs C, et al. (2024) A population of faint, old, and massive quiescent galaxies at [Formula: see text] revealed by JWST NIRSpec Spectroscopy. Scientific Reports. 14: 3724
Glazebrook K, Nanayakkara T, Schreiber C, et al. (2024) A massive galaxy that formed its stars at z ~ 11. Nature
Franco M, Elbaz D, Zhou L, et al. (2020) GOODS-ALMA: The slow downfall of star-formation in $z$ = 2-3 massive galaxies Astronomy and Astrophysics
Franco M, Elbaz D, Zhou L, et al. (2020) GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies Astronomy and Astrophysics
Zhou L, Elbaz D, Franco M, et al. (2020) GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5 Astronomy and Astrophysics
Ciesla L, Béthermin M, Daddi E, et al. (2020) A hyper luminous starburst at z = 4.72 magnified by a lensing galaxy pair at z = 1.48 Astronomy and Astrophysics. 635
Popesso P, Morselli L, Concas A, et al. (2019) The main sequence of star-forming galaxies – II. A non-evolving slope at the high-mass end Monthly Notices of the Royal Astronomical Society. 490: 5285-5299
Wang T, Elbaz D, Daddi E, et al. (2018) Revealing the Environmental Dependence of Molecular Gas Content in a Distant X-Ray Cluster at z = 2.51 The Astrophysical Journal. 867: L29
Popesso P, Concas A, Morselli L, et al. (2018) The main sequence of star-forming galaxies – I. The local relation and its bending Monthly Notices of the Royal Astronomical Society. 483: 3213-3226
McLure RJ, Pentericci L, Cimatti A, et al. (2018) The VANDELS ESO public spectroscopic survey Monthly Notices of the Royal Astronomical Society. 479: 25-42
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