Table 2
Additional dippers that exhibit dips in their light curves as secondary variability.
| EPIC | 2MASS | Name | Type | Period | G |
|---|---|---|---|---|---|
| [d] | [mag] | ||||
| 210725857 | J04285053+1844361 | … | Sd | 2.06 | 15.19 |
| 246859790(*) | J04440164+1621324 | … | Sd | 2.16 | 17.30 |
| 247575425 | J04331907+2246342 | IRAS 04303+2240 | Td | 7.5 | 16.09 |
| 247584113 | J04335200+2250301 | CI Tau | db | 8.5; | 12.15 |
| 247585465 | J04322415+2251083 | … | Bd? | 2.48 | 15.25 |
| 247788960 | J04323058+2419572 | FY Tau | B?d | 6.94; | 13.77 |
| 247810494 | J04345542+2428531 | AA Tau | d? | … | 14.49 |
| 247827638(*) | J04293606+2435556 | XEST 13-010 | Sd | 3.9 | 14.85 |
| 247915927 | J04442713+2512164 | IRAS 04414+2506 | S?d | 4.42 | 15.48 |
| 248009353 | J04324282+2552314 | UZ Tau | Bd | … | 12.39 |
| 248018164(*) | J04413882+2556267 | Haro 6-33 | Td? | … | 15.94 |
| 248030407(*) | J04394488+2601527 | ITG 15 | S?d | 3.45 | 15.00 |
Notes. The variability type has to be interpreted as: capital letter = dominant variability; d = dipper; s = spot; b = burster; t = long-term trend. The periods are derived with the CLEAN periodogram, and the listed value is the dominant period of the light curve, i.e., of the spot, when present. Only CI Tau and EPIC 247585465 exhibit quasiperiodic dips. The brightness is obtained from the Gaia G band. (*)Star reported as a dipper by Rebull et al. (2020).
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