KC
Karin Cescon
astro-ph.GAastro-ph.COastro-ph.IM
On Valency
published · living versionsW_unu28bt7published
Preprints & journals
10 papers in the corpus · 2025–2026The ALMA REBELS Survey: The [C II] Luminosity Function of UV-Selected Galaxies at 2610.27052v2 · Thomas Herard-Demanche, Pascal A. Oesch, Rychard Bouwens et al.2026 · 0 citationsarXiv
The dawn of the first galaxies2610.20733v2 · Livia Vallini, Tanio Diaz Santos, Belen Alcalde Pampliega et al.2026 · 0 citationsarXiv
What fuels the growth of stars and black holes in galaxies through cosmic time? The physics and chemistry of the interstellar medium in distant galaxies2610.20803v1 · Leindert A. Boogaard, Manuel Aravena, Matus Rybak et al.2026 · 0 citationsarXiv
REBELS-25: multi-phase morphology and kinematics at z = 7.312608.25982v1 · Lucie E. Rowland, Hiddo S. B. Algera, Jacqueline Hodge et al.2026 · 0 citationsarXiv
Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.152608.08015v1 · Gitanjali Rajulal, Hiddo S. B. Algera, Yuma Sugahara et al.2026 · 0 citationsarXiv
Direct detection of cool molecular gas in a star-forming galaxy at 2606.13393v1 · Karin Cescon, Jacqueline A. Hodge, Leindert A. Boogaard et al.2026 · 1 citationMNRAS, Volume 549, Issue 3, July 2026, stag924
A first systematic study of [OIII] 88m at : two luminous oxygen lines and a powerful ionized outflow in the first 600 million years2512.14486v2 · Hiddo S. B. Algera, John R. Weaver, Tom J. L. C. Bakx et al.2025 · 1 citationarXiv
How much gas and dust is in the Lyman Break Galaxy HZ10? An ALMA Band 10 to 4 and JWST/NIRSpec study of its interstellar medium2512.02320v1 · H. S. B. Algera, R. Herrera-Camus, M. Aravena et al.2025 · 1 citationarXiv
REBELS-IFU: on the origin of the elevated [OIII]/[CII] ratios in the early Universe2509.16071v1 · Hiddo Algera, Lucie Rowland, Renske Smit et al.2025 · 2 citationsarXiv
REBELS-IFU: Evidence for metal-rich massive galaxies at z~6-82501.10559v1 · Lucie E. Rowland, Mauro Stefanon, Rychard Bouwens et al.2025 · 17 citationsarXiv
Career total: 13 works. 10 are in this corpus.
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