Abstract
A fraction of active galactic nuclei (AGN) have double-peaked H$\alpha$, H$\beta$ 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 amongst 343 broad-line AGN with redshifts $0.004
| Original language | English |
|---|---|
| Journal | The Astrophysical Journal |
| Publication status | Submitted - 7 Jul 2025 |
Keywords
- astro-ph.GA
- astro-ph.HE
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