The TDE AT2020vwl showed a third radio flare at the time a jet-wind collision was predicted from its first two flares, the first predicted-and-confirmed third flare.
Long-term AGN variability and the case of GSN 069
1 Pith paper cite this work, alongside 6 external citations. Polarity classification is still indexing.
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abstract
We report on a study of long-term flux variations in a sample of more than 1000 AGN observed with ROSAT and in the XMM-Newton slew survey. Over a period of 3-19 years, NLS1 galaxies as a class are found to be only slightly more variable than broad line Seyfert galaxies, despite the strong short term variability seen in some bright nearby NLS1s. Contrary to expectations, it is Seyfert II galaxies that exhibit the greatest flux volatility. One particular Sy II, which has brightened by a factor > 300 over 15 years, has been monitored in detail with Swift and XMM. The spectrum is extremely soft (kT \sim 60eV) consistent with pure thermal emission from an accretion disk and reminiscent of ROSAT observations of the NLS1,WPVS 007. We show that this is likely to be a "true" Sy II, without a BLR, and speculate that in its new high luminosity state we may be able to witness a BLR in formation.
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Triple radio flares from tidal disruption events: jet-wind collisions and the discovery of a third radio flare from AT2020vwl
The TDE AT2020vwl showed a third radio flare at the time a jet-wind collision was predicted from its first two flares, the first predicted-and-confirmed third flare.