The Astrophysical Journal (Jan 2025)

The Dual Nature of GHZ9: Coexisting Active Galactic Nuclei and Star Formation Activity in a Remote X-Ray Source at z = 10.145

  • Lorenzo Napolitano,
  • Marco Castellano,
  • Laura Pentericci,
  • Cristian Vignali,
  • Roberto Gilli,
  • Adriano Fontana,
  • Paola Santini,
  • Tommaso Treu,
  • Antonello Calabrò,
  • Mario Llerena,
  • Enrico Piconcelli,
  • Luca Zappacosta,
  • Sara Mascia,
  • Roberta Tripodi,
  • Pablo Arrabal Haro,
  • Pietro Bergamini,
  • Tom J. L. C. Bakx,
  • Mark Dickinson,
  • Karl Glazebrook,
  • Alaina Henry,
  • Nicha Leethochawalit,
  • Giovanni Mazzolari,
  • Emiliano Merlin,
  • Takahiro Morishita,
  • Themiya Nanayakkara,
  • Diego Paris,
  • Simonetta Puccetti,
  • Guido Roberts-Borsani,
  • Sofia Rojas Ruiz,
  • Piero Rosati,
  • Eros Vanzella,
  • Fabio Vito,
  • Benedetta Vulcani,
  • Xin Wang,
  • Ilsang Yoon,
  • Jorge A. Zavala

DOI
https://doi.org/10.3847/1538-4357/ade706
Journal volume & issue
Vol. 989, no. 1
p. 75

Abstract

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We present James Webb Space Telescope (JWST)/NIRSpec PRISM spectroscopic characterization of GHZ9 at z = 10.145 ± 0.010, currently the most distant source detected by the Chandra X-ray Observatory. The spectrum reveals several UV high-ionization lines, including C II , Si IV , N IV ], C IV , He II , O III ], N III ], and C III ]. The prominent rest-frame equivalent widths (EW(C IV ) ≃ 65 Å, EW(O III ]) ≃ 28 Å, and EW(C III ]) ≃ 48 Å) show the presence of a hard active galactic nucleus (AGN) radiation field, while line ratio diagnostics are consistent with either AGN or star formation as the dominant ionizing source. GHZ9 is nitrogen-enriched (6–9.5 (N/O) _⊙ ), carbon-poor (0.2–0.65 (C/O) _⊙ ), metal-poor ( Z = 0.01–0.1 Z _⊙ ), and compact (0.02, implies an accelerated growth of the BH mass with respect to the stellar mass. GHZ9 is the ideal target to constrain the early phases of AGN–galaxy coevolution with future multifrequency observations.

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