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BASS. LII. The Prevalence of Double-peaked Broad Lines at Low Accretion Rates among Hard X-Ray Selected Active Galactic Nuclei

  • Charlotte Ward
  • , Michael J. Koss
  • , Michael Eracleous
  • , Benny Trakhtenbrot
  • , Franz E. Bauer
  • , Turgay Caglar
  • , Fiona Harrison
  • , Arghajit Jana
  • , Darshan Kakkad
  • , Macon Magno
  • , Ignacio del Moral-Castro
  • , Richard Mushotzky
  • , Kyuseok Oh
  • , Alessandro Peca
  • , Meredith C. Powell
  • , Claudio Ricci
  • , Alejandra Rojas
  • , Krista Lynne Smith
  • , Daniel Stern
  • , Ezequiel Treister
  • C. Megan Urry

Research output: Contribution to journalArticlepeer-review

2 Citations (Scopus)

Abstract

A fraction of active galactic nuclei (AGN) have double-peaked Hα, Hβ, and Mg II broad lines attributed to emission from rotating gas in the accretion disk. Using optical spectroscopy of a flux-limited sample of AGN selected via ultrahard X-rays from the BAT AGN Spectroscopic Survey (BASS), we systematically identify 71 double-peaked emitters (DPEs) among 343 broad-line AGN with redshifts 0.004 < z < 0.297 and X-ray luminosities of 40
Original languageEnglish
Number of pages19
JournalThe Astrophysical Journal
Volume991
Issue number1
Early online date19 Sept 2025
DOIs
Publication statusPublished - 20 Sept 2025

Keywords

  • AGN host galaxies
  • Active galaxies
  • Supermassive black holes

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