The rest-ultraviolet to infrared spectral energy distributions of heavily reddened quasars are ’V-shaped’ and hot-dust poor

BibTeX Entry

@article{2026MNRAS.546ag191S,
  author = {{Stepney}, Matthew and {Banerji}, Manda and {Tang}, Shenli and {Temple}, Matthew J. and {Hewett}, Paul C.},
  title = {{The rest-ultraviolet to infrared spectral energy distributions of heavily reddened quasars are 'V-shaped' and hot-dust poor}},
  journal = {\mnras},
  keywords = {galaxies: evolution, galaxies: photometry, quasars: general},
  year = {2026},
  month = mar,
  volume = {546},
  number = {4},
  eid = {stag191},
  pages = {stag191},
  doi = {10.1093/mnras/stag191},
  adsurl = {https://ui.adsabs.harvard.edu/abs/2026MNRAS.546ag191S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System},
  dimensions = {true},
  lrdkeys = {agn-dominated, dust-reddened, multi-wavelength, obscuration, sed},
  eprint = {2601.17416},
  archiveprefix = {arXiv},
  primaryclass = {astro-ph.GA},
  month_numeric = {3}
}

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