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Table 2

Properties of the repeating flare sample.

Name Δt (days) Nflares pTHE Double THE Separate events (p) Other References
AT 2024pvu ~6535 2 ✓ (5.7 × 10−4) i
AT 2022exr ~110 (~35) 3 ? X (9.6 × 10−6) i
AT 2022dbl ~695 2 X (6.1 × 10−5) ii, iii
AT 2022agi ~3760 2 ✓ (3.3 × 10−4) iv
AT 2021uvz ~55 2 ? X (4.8 × 10−6) i
AT 2021mhg ~710 2 X X X (6.2 × 10−5) α v, vi
AT 2020vdq ~995 2 X (8.7 × 10−5) vi, vii, viii
AT 2020acka ~300 2 X (2.6 × 10−5) β ix, x
AT 2019azh ~5295 2 ✓ (4.6 × 10−4) xi, xii
AT 2019ehz ~300 2 X (2.6 × 10−5) β vii, x, xii
AT 2018fyk ~1350 2 X (1.2 × 10−4) xiii, xiv

Notes. Column 1: name of the TDE. Column 2: time separation between the peaks (the parenthesis for AT 2022exr is the time separation between the second and third flares). Column 3: number of flares. Column 4: partial TDE scenario. Column 5: disruption of a stellar binary scenario. Column 6: disruption of separate stars scenario. Column 7: other potential mechanism (α = TDE followed by SN, β = accretion disc fluctuation or a sudden influx of excess orbiting material from the disrupted star). Column 8: references, (i) this work, (ii) Lin et al. (2024), (iii) Makrygianni et al. (2025), (iv) Sun et al. (2024), (v) Munoz-Arancibia et al. (2023), (vi) Somalwar et al. (2025b), (vii) Yao et al. (2023), (viii) Charalampopoulos et al. (2023), (ix) Guo et al. (2025), (x) Zhong (2025), (xi) Hinkle et al. (2021), (xii) Hammerstein et al. (2023), (xiii) Wevers et al. (2019), (xiv) Wevers et al. (2023).

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