Irony at z=6.68: a bright AGN with forbidden Fe emission and multi-component Balmer absorption

BibTeX Entry

@article{2025arXiv251000101D,
  author = {{D'Eugenio}, Francesco and {Nelson}, Erica and {Ji}, Xihan and {Baggen}, Josephine and {Greene}, Jenny and {Labb{\'e}}, Ivo and {Pezzulli}, Gabriele and {Brown}, Vanessa and {Maiolino}, Roberto and {Matthee}, Jorryt and {Terlevich}, Elena and {Terlevich}, Roberto and {Torralba}, Alberto and {Carniani}, Stefano},
  title = {{Irony at z=6.68: a bright AGN with forbidden Fe emission and multi-component Balmer absorption}},
  journal = {arXiv e-prints},
  keywords = {Astrophysics of Galaxies},
  year = {2025},
  month = sep,
  eid = {arXiv:2510.00101},
  pages = {arXiv:2510.00101},
  archiveprefix = {arXiv},
  eprint = {2510.00101},
  primaryclass = {astro-ph.GA},
  adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv251000101D},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  dimensions = {true},
  lrdkeys = {black hole mass, emission lines, jwst, kinematics, spectroscopy},
  month_numeric = {9}
}

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