A Population of Red Galaxies with Very Strong Emission Lines at z > 5 Revealed by the NIRCam Medium Bands: “Classic” LRDs, Dusty Star-Forming Galaxies, and a Missing Population of LRDs

BibTeX Entry

@article{2026arXiv260606585W,
  author = {{Withers}, Sunna and {Muzzin}, Adam and {Ravindranath}, Swara and {Willott}, Chris J. and {Martis}, Nicholas S. and {Tripodi}, Roberta and {Asada}, Yoshihisa and {Brada{\v{c}}}, Maru{\v{s}}a and {Merchant}, Maya and {Mowla}, Lamiya and {Noirot}, Ga{\"e}l and {Sarrouh}, Ghassan T. E. and {Sawicki}, Marcin and {Antwi-Danso}, Jacqueline and {Harshan}, Anishya and {Jagga}, Naadiyah and {Marchesini}, Danilo and {Myers}, Katherine and {Sok}, Visal},
  title = {{A Population of Red Galaxies with Very Strong Emission Lines at $z > 5$ Revealed by the NIRCam Medium Bands: ``Classic'' LRDs, Dusty Star-Forming Galaxies, and a Missing Population of LRDs}},
  journal = {arXiv e-prints},
  keywords = {Astrophysics of Galaxies},
  year = {2026},
  month = jun,
  eid = {arXiv:2606.06585},
  pages = {arXiv:2606.06585},
  archiveprefix = {arXiv},
  eprint = {2606.06585},
  primaryclass = {astro-ph.GA},
  adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260606585W},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  dimensions = {true},
  lrdkeys = {early universe, emission lines, jwst, morphology, sample selection},
  month_numeric = {6}
}

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