GA-NIFS: The cosmic evolution of AGN outflows up to z~3-6 with JWST NIRSpec

The period between z~3-6 is a crucial transitional phase in galaxy evolution, leading to "cosmic noon" (z~1-3). A key actor in this phase is expected to be AGN feedback acting through energetic radiation and fast gas outflows. However, little is known so far about AGN feedback at these redshifts. I will present our study of AGN outflows at z~3-6 from GOODS-S and COSMOS fields, the largest spatially resolved sample to date (16 targets), exploiting JWST NIRSpec IFU observations from the GA-NIFS GTO survey. We found an outflow incidence of ~80%, significantly higher than in most AGN samples at lower redshifts. By mapping the rest-optical ionised gas emission lines ([OIII], Ha…) at sub-kpc scales, we inferred the outflow properties (kinematics, energetics) and probed their relations with AGN luminosity and galaxy star formation rate, and compared them with literature studies at different redshifts and AGN luminosities. We find evidence for a cosmic evolution of the outflow properties, indicating that outflows were stronger in the early Universe than at later times, and more capable of affecting their host galaxy evolution.

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Zenodo (CERN European Organization for Nuclear Research)
Published
2026-10-29
DOI
https://doi.org/10.5281/zenodo.23775739
Primary Topic
Galaxies: Formation, Evolution, Phenomena
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article
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article

GA-NIFS: The cosmic evolution of AGN outflows up to z~3-6 with JWST NIRSpec

Nimisha Kumari, G. Cresci, Francesco D’Eugenio, E. Bertola et al.
7 links
Zenodo (CERN European Organization for Nuclear Research)
Galaxies: Formation, Evolution, Phenomena
article

GA-NIFS: The cosmic evolution of AGN outflows up to z~3-6 with JWST NIRSpec

Nimisha Kumari, G. Cresci, Francesco D’Eugenio, E. Bertola, Santiago Arribas, Bruno Rodríguez Del Pino, Michele Perna, R. Maiolino, Chiara Circosta, Stefano Carniani, Madeline A. Marshall, Gareth C. Jones, S. Charlot, Isabella Lamperti, Jan Scholtz, Giacomo Venturi, Eleonora Parlanti, Sandra Zamora, Torsten Böker, Gareth C. Jones, Francesco D'Eugenio, Andrew Bunker, Hannah Übler, Roberto Maiolino, Hannah Übler, Torsten Böker
article en

Abstract

The period between z~3-6 is a crucial transitional phase in galaxy evolution, leading to "cosmic noon" (z~1-3). A key actor in this phase is expected to be AGN feedback acting through energetic radiation and fast gas outflows. However, little is known so far about AGN feedback at these redshifts. I will present our study of AGN outflows at z~3-6 from GOODS-S and COSMOS fields, the largest spatially resolved sample to date (16 targets), exploiting JWST NIRSpec IFU observations from the GA-NIFS GTO survey. We found an outflow incidence of ~80%, significantly higher than in most AGN samples at lower redshifts. By mapping the rest-optical ionised gas emission lines ([OIII], Ha…) at sub-kpc scales, we inferred the outflow properties (kinematics, energetics) and probed their relations with AGN luminosity and galaxy star formation rate, and compared them with literature studies at different redshifts and AGN luminosities. We find evidence for a cosmic evolution of the outflow properties, indicating that outflows were stronger in the early Universe than at later times, and more capable of affecting their host galaxy evolution.

Zenodo (CERN European Organization for Nuclear Research)
Scuola Normale Superiore (IT)
Openalex Percentile: Top 15%
Galaxies: Formation, Evolution, Phenomena
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