Table 3.
Not confirmed AGN candidates.
| Case | Number of objects |
|---|---|
| Transient in template | 30 |
| Transient | 2 |
| Weak transient | 7 |
| Bad subtraction | 15 |
| Other | 11 |
| Total | 65 |
Notes. Case names and number of selected candidates that were not confirmed from their optical spectra. The Transient cases correspond to nuclear variability. Bad subtraction cases are those with poor subtraction in the ZTF difference images. The Other cases denote light curves where the measured variability appears to be real, based on visual inspection.
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