How Long Will the Quasar UV/Optical Flickering Be Damped?
The UV/optical light curves of Active Galactic Nuclei (AGNs) are commonly described by the Damped Random Walk (DRW) model. However, the physical interpretation of the damping timescale, a key parameter in the DRW model, remains unclear. Particularly, recent observations indicate a weak dependence of...
| Asıl Yazarlar: | , , , , , |
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| Materyal Türü: | Makale |
| Dil: | English |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2024-01-01
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| Seri Bilgileri: | The Astrophysical Journal |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/1538-4357/ad2fbc |