Table 5
Stellar properties of the dipper sample.
| EPIC | Name | L* | M* | R* | Rcor | Tcor | vsini | Ref. | i* | logṀacc | Refs. |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [L⊙] | [M⊙] | [R⊙] | [R*] | [K] | [km s−1] | [°] | [M⊙ yr−1] | ||||
| 246929818 | Haro 6-37 |  |
 |
 |
8.98 |  |
12.1 ± 1.2 | 1 | >47 | −7.00/−8.12 | 6,7,8 |
| 246942563 | St 34 |  |
 |
 |
6.38 |  |
… | … | … | … | … |
| 246989752 | … |  |
 |
 |
4.08 |  |
… | … | … | … | … |
| 247103541 | HD 285893 |  |
 |
 |
… | … | … | … | … | … | … |
| 247520207 | LkCa 15 |  |
 |
 |
8.69 |  |
13.9 ± 1.2 | 1 |  |
−8.83/−8.87/−9.17 | 8, 6, 9 |
| 247575958 | CFHT Tau 12 |  |
 |
 |
4.90 |  |
… | … | … | … | … |
| 247589612 | JH 112 A |  |
 |
 |
3.33 |  |
… | … | … | … | … |
| 247592463 | HP Tau |  |
 |
 |
4.00 |  |
15.4 ± 1.6 | 2 |  |
… | … |
| 247763883 | GH Tau |  |
 |
 |
2.46 |  |
30.3 ± 0.7 | 1 |  |
−7.92/−8.02/−8.90 | 7, 10, 6, 8 |
| 247764745 | V807 Tau |  |
 |
 |
3.81 |  |
13.6 ± 0.7 | 1 |  |
−8.40/<−8.68 | 8,10 |
| 247791801 | GK Tau |  |
 |
 |
4.98 |  |
18.7 ± 3.5 | 2 |  |
−8.19 | 6, 7, 8, 11 |
| 247792225 | GI Tau |  |
 |
 |
5.75 |  |
12.7 ± 1.9 | 1 |  |
−8.00/−8.02/−8.08 | 11, 6, 7, 8 |
| 247799571 | HK Tau |  |
 |
 |
4.47 |  |
21.8 ± 2.5 | 3 |  |
−7.65 | 12 |
| 247805410 | FX Tau |  |
 |
 |
… | … | 9.61 ± 0.19 | 1 | … | −8.65 | 6,7 |
| 247820821 | … |  |
 |
 |
3.70 |  |
18.4 ± 1.0 | 4 | >64 | … | … |
| 247885481 | … |  |
 |
 |
5.23 |  |
… | … | … | … | … |
| 247935061 | GO Tau |  |
 |
 |
… | … | 17.5 ± 9.7 | 2 | … | −7.93/−8.33/−8.42 | 6,9,8 |
| 248006676 | JH 223 |  |
 |
 |
4.52 |  |
… | … | … | … | … |
| 248015397 | ITG 34 |  |
 |
 |
6.23 |  |
… | … | … | … | … |
| 248029373 | DK Tau |  |
 |
 |
5.78 |  |
17.5 ± 1.2 | 1 | >60 | −7.42 | 6,7,11 |
| 248046139 | GM Tau |  |
 |
 |
4.49 |  |
9.0 ± 2.0 | 5 |  |
−8.60/−8.70 | 13, 14 |
| 248047443 | IS Tau |  |
 |
 |
6.93 |  |
… | … | … | −7.91/−8.01 | 10,8 |
Notes. Stellar inclinations reported as lower limits have sini > 1.
References. (1) Nguyen et al. (2012); (2) Güdel et al. (2007); (3) Hartmann et al. (1986); (4) Kraus et al. (2017); (5) Mohanty et al. (2005); (6) Hartmann et al. (1998); (7) Muzerolle et al. (1998); (8) White & Ghez (2001); (9) Isella et al. (2009); (10) Hartigan & Kenyon (2003); (11) Gullbring et al. (1998); (12) White & Hillenbrand (2004); (13) White & Basri (2003); (14) Herczeg & Hillenbrand (2008).
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