Details

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.

.pdfPDF - Presentation file, Download (3,72 MB)
MD5: 2CA30C0695F70CCB7C50AA7C301E0D4E
URLURL - Source URL, Visit https://iopscience.iop.org/article/10.3847/2041-8213/ae13a9 This link opens in a new window

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 This link opens in a new window
UDC:524.8
ISSN on article:2041-8213
DOI:10.3847/2041-8213/ae13a9 This link opens in a new window
COBISS.SI-ID:259572995 This link opens in a new window
Publication date in RUL:02.12.2025
Views:530
Downloads:273
Metadata:XML DC-XML DC-RDF
:
Copy citation
Share:Bookmark and Share

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 This link opens in a new window

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

Similar documents

Similar works from RUL:
Similar works from other Slovenian collections:

Back