Published November 21, 2024
| Version v1
Publication
CEERS: Forging the First Dust -- Transition from Stellar to ISM Grain Growth in the Early Universe
Creators
- Burgarella, Denis
- Buat, Véronique
- Theulé, Patrice
- Zavala, Jorge
- Haro, Pablo Arrabal
- Bagley, Micaela B
- Boquien, Médéric
- Cleri, Nikko
- Dewachter, Tim
- Dickinson, Mark
- Ferguson, Henry C
- Fernández, Vital
- Finkelstein, Steven L
- Fontana, Adriano
- Gawiser, Eric
- Grazian, Andrea
- Grogin, Norman
- Holwerda, Benne W
- Kartaltepe, Jeyhan S
- Kewley, Lisa
- Kirkpatrick, Allison
- Kocevski, Dale
- Koekemoer, Anton M
- Long, Arianna
- Lotz, Jennifer
- Lucas, Ray A
- Mobasher, Bahram
- Papovich, Casey
- Pérez-González, Pablo G
- Pirzkal, Nor
- Ravindranath, Swara
- Rodighiero, Giulia
- Roehlly, Yannick
- Rose, Caitlin
- Seillé, Lise-Marie
- Somerville, Rachel
- Wilkins, Steve
- Yang, Guang
- Yung, L.Y. Aaron
Contributors
Others:
- Laboratoire d'Astrophysique de Marseille (LAM) ; Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
- Joseph Louis LAGRANGE (LAGRANGE) ; Université Nice Sophia Antipolis (1965 - 2019) (UNS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur ; Université Côte d'Azur (UniCA)-Université Côte d'Azur (UniCA)-Centre National de la Recherche Scientifique (CNRS)
Description
We investigate the coevolution of metals and dust for 173 galaxies at 4.010 by JWST. Besides, we observe that the metallicity of galaxies at z>8 presents a metal-to-stellar mass ratio larger than a few 10^-3, above a floor. This suggests a very fast rise of metals at high redshift, impacting the tentative detections of population III objects.
Abstract
International audienceAdditional details
Identifiers
- URL
- https://hal.science/hal-04796168
- URN
- urn:oai:HAL:hal-04796168v1
Origin repository
- Origin repository
- UNICA