Table 3
Variable YSOs that are dipper candidates of lower quality.
| EPIC | 2MASS | Name | Type | Period | G |
|---|---|---|---|---|---|
| [d] | [mag] | ||||
| 210689083 | J04313747+1812244 | HH 30 | t | 7.51 | … |
| 210690735 | J04300399+1813493 | UX Tau A+C | t? | 3.6; | 11.29 |
| 210690913 | J04313843+1813576 | HL Tau | t? | … | … |
| 246923113 | J04470620+1658428 | DR Tau | Bd? | 14.71 | 11.65 |
| 247837468 | J04293008+2439550 | IRAS 04264+2433 | ? | 11.9 | … |
| 247923794 | J04423769+2515374 | DP Tau | t | 3.66; | 13.51 |
| 247992574 | J04392090+2545021 | GN Tau | t | 5.75; | 14.56 |
| 248017479 | J04410826+2556074 | ITG 33A | t | 6.6; | 17.60 |
| 248040905 | J04295156+2606448 | IQ Tau | t | … | 13.24 |
| 248055184 | J04335470+2613275 | IT Tau | t | 2.74 | … |
| 248058354 | J04334465+2615005 | … | ? | … | 16.50 |
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. Most objects in this list are dominated by a long-term trend. The brightness is obtained from the Gaia G band.
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