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A deep dive down the broad-line region: permitted O I, Ca II, and Fe II emission in an active galactic nucleus little red dot at z = 5.3
ID
Tripodi, Roberta
(
Author
),
ID
Bradač, Maruša
(
Author
),
ID
Martis, Nicholas S.
(
Author
),
ID
Rihtaršič, Gregor
(
Author
),
ID
Felicioni, Giordano
(
Author
),
ID
Harshan, Anishya
(
Author
),
ID
Judež, Jon
(
Author
),
ID
Markov, Vladan
(
Author
), et al.
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https://iopscience.iop.org/article/10.3847/2041-8213/ae13a9
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Abstract
We present a spectroscopic analysis of a broad-line active galactic nucleus (AGN) selected as a little red dot (LRD) at z = 5.3 behind the Bullet cluster (Bz5.3) based on JWST/NIRCam and NIRSpec data. The detection of strong Fe II, O I, and Ca II triplet emission lines, along with the evidence of broad Balmer lines, provides strong evidence of a broad-line region (BLR) and an accreting supermassive black hole. Notably, we report the first detection of the λ1304 bump (i.e., a blend of O I λ1304 and Si II) at high redshift, a feature commonly seen in local AGNs but not yet reported in the early Universe. The O I λ1304/λ8446 photon ratio provides an independent measurement of dust attenuation in galaxies. In Bz5.3, this ratio is highly suppressed (0.1–0.3), implying significant internal dust extinction, with estimated dust attenuation A$_V$ ~ 0.4–1.0. We identify Lyβ fluorescence as the dominant excitation mechanism of the low-ionization lines, with additional contributions from collisional excitation. High O I λ8446 equivalent width and weak O I λ7774 support this interpretation. The detection of iron emission, whether from broad permitted or narrow forbidden lines, supports the presence of a stratified BLR, as also recently proposed in local LRDs. Photoionization modeling of O I λ8446 and Ca II further suggests the coexistence of multiple gas phases with distinct densities and ionization states, highlighting the complexity of the BLR. Bz5.3 thus offers a rare window into early AGN activity and BLR physics at early times.
Language:
English
Keywords:
astrophysics
,
galaxies
,
spectroscopy
,
active galactic nucleus
Work type:
Article
Typology:
1.01 - Original Scientific Article
Organization:
FMF - Faculty of Mathematics and Physics
Publication status:
Published
Publication version:
Version of Record
Year:
2025
Number of pages:
12 str.
Numbering:
Vol. 994, no. 1
PID:
20.500.12556/RUL-176489
UDC:
524.8
ISSN on article:
2041-8213
DOI:
10.3847/2041-8213/ae13a9
COBISS.SI-ID:
259572995
Publication date in RUL:
02.12.2025
Views:
530
Downloads:
273
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Record is a part of a journal
Title:
The Astrophysical journal. Letters
Shortened title:
Astrophys. J. Lett.
Publisher:
American Astronomical Society
ISSN:
2041-8213
COBISS.SI-ID:
367233
Licences
License:
CC BY 4.0, Creative Commons Attribution 4.0 International
Link:
http://creativecommons.org/licenses/by/4.0/
Description:
This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.
Secondary language
Language:
Slovenian
Keywords:
astrofizika
,
galaksije
,
spektroskopija
,
aktivna galaktična jedra
Projects
Funder:
EC - European Commission
Project number:
101053208
Name:
Exploring Cosmic Dawn with James Webb Space Telescope
Acronym:
FIRSTLIGHT
Funder:
ARIS - Slovenian Research and Innovation Agency
Project number:
N1-0238-2022
Name:
Raziskave kozmične zore z James Webb vesoljskim teleskopom
Funder:
ARIS - Slovenian Research and Innovation Agency
Project number:
P1-0188-2022
Name:
Astrofizika in fizika atmosfere
Funder:
European Union
Funding programme:
European Union - NextGenerationEU
Project number:
2022CB3PJ3
Name:
First Light And Galaxy aSsembly
Acronym:
FLAGS
Funder:
ESA - European Space Agency
Project number:
4000146646
Funder:
CSA - Canadian Space Agency
Project number:
18JWST-GTO1
Funder:
Natural Sciences and Engineering Research Council of Canada
Funding programme:
Discovery Grants
Funder:
NASA - National Aeronautics and Space Administration
Project number:
NAS5-03127
Funder:
NASA - National Aeronautics and Space Administration
Project number:
4598
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