The quest for high-redshift radio galaxies II. Discovery of the most powerful known radio galaxy at z=4.946

Abstract

As part of our quest for high-redshift radio galaxies (HzRGs), we present the results obtained from optical spectroscopy leading to the confirmation of one HzRG candidate selected using the Lyman break technique. The optical emission, associated with the radio source TXS 2354+015, exhibits a prominent drop in the r band, which is characteristic of sources at z~5. The optical spectrum shows a bright asymmetric emission line, with a large equivalent width of ~900 Angstrom. Its identification with the Lyα line is confirmed by the detection of the NVλ1640, leading to a redshift estimate of z=4.946. Its broadband radio spectrum is well reproduced using a power law with a slope of 0.94. The radio luminosity at the rest frame frequency of 500 MHz is 6.2e29 W/Hz. This result makes this source the most powerful radio galaxy currently known.

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BibTeX RIS

BibTeX

@misc{balmaverde2026quest,
  title = {{The quest for high-redshift radio galaxies II. Discovery of the most powerful known radio galaxy at z=4.946}},
  author = {B. Balmaverde and A. Capetti and M. Chiaberge and F. Massaro and M. Coloma Puga and A. Jimenez-Gallardo},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.28632},
  eprint = {2609.28632},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.28632},
  note = {CC BY 4.0},
}

RIS

TY  - UNPB
TI  - The quest for high-redshift radio galaxies II. Discovery of the most powerful known radio galaxy at z=4.946
AU  - B. Balmaverde
AU  - A. Capetti
AU  - M. Chiaberge
AU  - F. Massaro
AU  - M. Coloma Puga
AU  - A. Jimenez-Gallardo
PY  - 2026
DA  - 2026/09/23
PB  - arXiv
DO  - 10.48550/arxiv.2609.28632
UR  - https://arxiv.org/abs/2609.28632
AB  - As part of our quest for high-redshift radio galaxies (HzRGs), we present the results obtained from optical spectroscopy leading to the confirmation of one HzRG candidate selected using the Lyman break technique. The optical emission, associated with the radio source TXS 2354+015, exhibits a prominent drop in the r band, which is characteristic of sources at z~5. The optical spectrum shows a bright asymmetric emission line, with a large equivalent width of ~900 Angstrom. Its identification with the Lyα line is confirmed by the detection of the NVλ1640, leading to a redshift estimate of z=4.946. Its broadband radio spectrum is well reproduced using a power law with a slope of 0.94. The radio luminosity at the rest frame frequency of 500 MHz is 6.2e29 W/Hz. This result makes this source the most powerful radio galaxy currently known.
ER  -

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