Table 4
Morphological properties of the dips.
| EPIC | Name | P | σP | W | W−σ | W+σ | A | p2p |
|---|---|---|---|---|---|---|---|---|
| [d] | [d] | [P] | [P] | [P] | [mag] | [mag] | ||
| 246929818(a) | Haro 6-37 | 10.63; | 0.72 | 0.59 | 0.65 | 0.50 | 0.75 | 1.03 |
| 246942563 | St 34 | 5.23; | 0.20 | 0.65(b) | 0.59 | 0.76 | 0.14 | 0.33 |
| 246989752 | … | 1.62 | 0.03 | 0.22 | 0.18 | 0.37 | 0.16 | 0.46 |
| 247103541 | HD 285893 | … | … | … | … | … | 0.05 | 0.13 |
| 247520207 | LkCa 15 | 5.78 | 0.20 | 0.64(c) | 0.47 | 0.62 | 0.54 | 1.05 |
| 247575958 | CFHT Tau 12 | 3.48 | 0.07 | 0.59 | 0.60 | 0.70 | 0.23 | 0.50 |
| 247589612 | JH 112 A | 2.21 | 0.07 | 0.20(c) | 0.18 | 0.34 | 0.11 | 0.53 |
| 247592463 | HP Tau | 4.33 | 0.17 | 0.55(c) | 0.51 | 0.64 | 0.24 | 0.65 |
| 247763883 | GH Tau | 2.49 | 0.06 | 0.44 | 0.54 | 0.48 | 0.37 | 0.74 |
| 247764745 | V807 Tau | 4.39 | 0.12 | 0.39 | 0.40 | 0.35 | 0.11 | 0.18 |
| 247791801 | GK Tau | 4.61 | 0.15 | 0.43 | 0.41 | 0.48 | 0.62 | 1.28 |
| 247792225 | GI Tau | 7.13 | 0.40 | 0.67(c) | 0.34 | 0.68 | 0.49 | 0.97 |
| 247799571 | HK Tau | 3.3 | 0.07 | 0.50 | 0.53 | 0.44 | 0.29 | 0.55 |
| 247805410 | FX Tau | … | … | … | … | … | 0.18 | 0.36 |
| 247820821 | … | 2.38 | 0.04 | 0.41 | 0.43 | 0.36 | 1.18 | 1.77 |
| 247885481 | … | 2.90(d) | 0.08 | 0.60(b) | 0.32 | 0.89 | 0.05 | 0.14 |
| 247935061 | GO Tau | … | … | … | … | … | 0.17 | 0.36 |
| 248006676(a) | JH 223 | 3.31 | 0.09 | 0.36 | 0.36 | 0.39 | 0.32 | 0.54 |
| 248015397 | ITG 34 | 3.91 | 0.17 | 0.51 | 0.46 | 0.58 | 0.53 | 1.22 |
| 248029373(a) | DK Tau | 7.69; | 0.45 | 0.57 | 0.65 | 0.35 | 1.08 | 1.91 |
| 248046139 | GM Tau | 2.67 | 0.05 | 0.44 | 0.49 | 0.40 | 1.30 | 2.00 |
| 248047443 | IS Tau | 7.58 | 0.41 | 0.54(c) | 0.68 | 0.43 | 0.13 | 0.24 |
Notes. Columns: the photometric period P, the uncertainty estimated from the Gaussian fitting of the periodogram peak σP, the dip width W measured as the FWHM of the folded and binned light curve in units of phase, the dip width estimated considering the binned light curve ± σ of the flux (W−σ, W+σ), the dip amplitude with the 90th and5th flux percentiles A, the peak-to-peak amplitude p2p. The stars are detrended before the width was determined, with the exception of those marked(a). (b)Value discarded because it was not representative of the real dip width. (c)Double-peaked dip. (d)The peak of the periodogram is at 2.99 d and is linked to a cold spot. A more thorough analysis is needed to retrieve the dipper period at 2.90 d.
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