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 language | English |
|---|---|
| Number of pages | 19 |
| Journal | The Astrophysical Journal |
| Volume | 991 |
| Issue number | 1 |
| Early online date | 19 Sept 2025 |
| DOIs | |
| Publication status | Published - 20 Sept 2025 |
Keywords
- AGN host galaxies
- Active galaxies
- Supermassive black holes
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