Ivo Ferdinand Louis Labbé
Affiliations: | Leiden Observatory | Leiden University, Leiden, Netherlands |
Website:
https://local.strw.leidenuniv.nl/people/touchscreen2/persinline.php?id=54Google:
"Ivo Ferdinand Louis Labbé"Bio:
http://home.strw.leidenuniv.nl/~ivo/
http://www.astro.rug.nl/KAPTEYN_DB/blaauw_view.php?stage=2&id=439&auth=0
https://www.strw.leidenuniv.nl/events/phdtheses/labbe/
Parents
Sign in to add mentor| Marijn Franx | grad student | 2004 | Leiden | |
| (Deep infra-red studies of massive high redshift galaxies.) | ||||
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Publications
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| de Graaff A, Setton DJ, Brammer G, et al. (2024) Efficient formation of a massive quiescent galaxy at redshift 4.9. Nature Astronomy. 9: 280-292 |
| Xiao M, Oesch PA, Elbaz D, et al. (2024) Accelerated formation of ultra-massive galaxies in the first billion years. Nature. 635: 311-315 |
| Atek H, Labbé I, Furtak LJ, et al. (2024) Most of the photons that reionized the Universe came from dwarf galaxies. Nature. 626: 975-978 |
| 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 |
| Furtak LJ, Labbé I, Zitrin A, et al. (2024) A high black hole to host mass ratio in a lensed AGN in the early Universe. Nature |
| Glazebrook K, Nanayakkara T, Schreiber C, et al. (2024) A massive galaxy that formed its stars at z ~ 11. Nature |
| Labbé I, van Dokkum P, Nelson E, et al. (2023) A population of red candidate massive galaxies ~600 Myr after the Big Bang. Nature |
| Whitaker KE, Franx M, Leja J, et al. (2020) Erratum: “CONSTRAINING THE LOW-MASS SLOPE OF THE STAR FORMATION SEQUENCE AT 0.5 < z < 2.5” (2014, ApJ, 795, 104) The Astrophysical Journal. 896: 175 |
| Tran KH, Forrest B, Alcorn LY, et al. (2020) MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3 |
| Martis NS, Marchesini DM, Muzzin A, et al. (2019) Stellar and Dust Properties of a Complete Sample of Massive Dusty Galaxies at 1 ≤ z ≤ 4 from MAGPHYS Modeling of UltraVISTA DR3 and Herschel Photometry The Astrophysical Journal. 882: 65 |