Seven wonders of Cosmic Dawn: JWST confirms a high abundance of galaxies and AGN at z ≃ 9-11 in the GLASS field
Artikel i vetenskaplig tidskrift, 2025
We present the JWST/NIRSpec PRISM follow-up of candidate galaxies at z ≈ 9-11 selected from deep JWST/NIRCam photometry in GLASSJWST Early Release Science data. We spectroscopically confirm six sources with secure redshifts at z = 9.52-10.43, each showing multiple emission lines. An additional object is likely at z ≈ 10.66, based on its Lya-break and a single emission feature, while one source is a lowerredshift interloper. The sample includes the first JWST-detected candidate at z ∼ 10, GHZ1/GLASS-z10, which we confirm at z = 9.875, and the X-ray detected active galactic nucleus (AGN) GHZ9 at z = 10.145. Three objects, including GHZ9, have EW(CIII]λ1908) > 20 Å and occupy a region compatible with AGN emission in the EW(CIII]) vs CIV/CIII] diagram. The spectroscopic sample confirms a high abundance of galaxies at z > 9. We measure a number density of z ∼ 10 galaxies in the GLASS-JWST ERS field that is a factor of >3 higher than other JWST-based estimates at demagnified rest-frame magnitudes of -21 ≤ MUV ≤ -19. We find that the positions of these galaxies in redshift and angular space are not consistent with all of them being part of a single progenitor of present-day galaxy clusters. The high density of objects in the GLASS region can be explained either by clustering on large scales or by a superposition of different forming structures of which we observe only the brightest members. By considering all the spectroscopic z ∼ 10 sources in the Abell-2744 field, we identify two potential galaxy proto-clusters centered around GHZ9 and JD1, with relative separations between their members of ≈1-2 pMpc. The potential AGN nature of three of the sources in our sample lends support to a scenario in which the high abundance of bright sources determined by JWST surveys at cosmic dawn may be affected by AGN contribution to their UV luminosity.
Reionization
Galaxies: active
First stars
Galaxies: high-redshift
Dark ages
Författare
Lorenzo Napolitano
Osservatorio Astronomico di Roma
Sapienza Università di Roma
M. Castellano
Osservatorio Astronomico di Roma
L. Pentericci
Osservatorio Astronomico di Roma
Pablo Arrabal Haro
NSF's National Optical-Infrared Astronomy Research Laboratory (NOIRLab)
A. Fontana
Osservatorio Astronomico di Roma
Tommaso Treu
University of California
Pietro Bergamini
Universita' degli Studi di Milano
Istituto nazionale di astrofisica (INAF)
Antonello Calabrò
Osservatorio Astronomico di Roma
Sara Mascia
Osservatorio Astronomico di Roma
Universita degli Studi di Roma Tor Vergata
Takahiro Morishita
California Institute of Technology (Caltech)
Guido Roberts-Borsani
Université de Genève
P. Santini
Osservatorio Astronomico di Roma
Eros Vanzella
University of Ferrara
B. Vulcani
Istituto nazionale di astrofisica (INAF)
D. Zakharova
Università di Padova
Istituto nazionale di astrofisica (INAF)
Tom Bakx
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Mark Dickinson
NSF's National Optical-Infrared Astronomy Research Laboratory (NOIRLab)
Claudio Grillo
Universita' degli Studi di Milano
N. Leethochawalit
National Astronomical Research Institute of Thailand
Mario Llerena
Osservatorio Astronomico di Roma
E. Merlin
Osservatorio Astronomico di Roma
Diego Paris
Osservatorio Astronomico di Roma
S. Rojas-Ruiz
University of California
Piero Rosati
University of Ferrara
Istituto nazionale di astrofisica (INAF)
Xin Wang
Chinese Academy of Sciences
Beijing Normal University
I. Yoon
National Radio Astronomy Observatory
J. A. Zavala
National Astronomical Observatory of Japan
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 693 A50Ämneskategorier (SSIF 2025)
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/202452090