Table A.1
Simulated light curves from Swift/XRT variable AGN searching for random TDE-like events.
| Source | TDE1 probab. | TDE3 probab. | Num. obs. | Variation | Type |
| (σ) | (σ) | ||||
|
|
|||||
| 1H 0707–495 | 4.11(4.95) | 4.06(4.84) | 101 | Δ = 114 | dip |
| Mkn 335 | >4.75 (7.93) | >4.75 (7.89) | 179 | Δ = 42 | flare |
| NGC 4395 | >4.75 (5.74) | 4.06(4.94) | 190 | Δ = 141 | flare |
| CGCG 229–015 | >4.75 (>8.31) | >4.75 (>8.31) | 44 | Δ = 56 | dip |
Notes. Probability of the first and third IC 3599 flares to be obtained by sampling the Swift/XRT light curves of highly variable AGNs. The first probability is obtained by requiring that the simulated light curve has a null-hypothesis probability higher than 5%. The second probability (in parenthesis) is obtained by weighting the best-fit light-curve probability with the number of simulations carried out.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.