AT2021aeuk was reported as a repeated nuclear transient (RNT) hosted by a narrow-line Seyfert 1 galaxy (Bao et al. 2024; Sun et al.2025). Two major flares were detected between 2018 and 2023, peaking at approximately MJD 58708 and 59995, respectively, along with a weak precursor prior to the first flare.
We recently detected a new rebrightening event of this target in the Wide Field Survey Telescope (WFST) survey on 61183.85, with u=19.13+/-0.03 and r=18.43+/-0.02. The rebrightening was further confirmed through cross-checking with ATLAS data. The newly detected flare, likely the third major flare, is still rising and has already surpassed the second flare in brightness. In addition, the time interval between the second and third flares is slightly shorter than that between the first and second flares. Therefore, AT2021aeuk joins the small sample of repeated nuclear transients with multiple flares. Multi-band follow-up observations have been triggered.
| Catalog | Name | Reported RA | Reported DEC | Reported Obj-Type | Reported Redshift | Host Name | Host Redshift | Remarks | TNS RA | TNS DEC | TNS Obj-Type | TNS Redshift |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| TNS | 2021aeuk | 16:12:59.842 | +42:19:40.25 | Other | 16:12:59.842 | +42:19:40.25 |


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