Table 1.
Characterization and validation of the 17 new planets from our TLS search, MCMC fitting, and vespa false-positive vetting pipeline.
| EPIC | K2 name | Ms (M⊙) |  |
P (d) | Rp/Rs | Rp (R⊕) | b | #tr (b) | SNR | SDETLS | ρ(″) | FPP | FPP2 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 201238110.02(d) |  |
 |
 |
 |
 |
 |
3 | 12.1 | 27.5 | 1.0 | 5.3 × 10−4 | 2.1 × 10−5 | |
| 201497682.03(d) |  |
 |
 |
 |
 |
 |
36 | 9.5 | 21.2 | 22.3 | 5.0 × 10−2 | 2.1 × 10−3 | |
| 201615463.02(i) | K2-166 |  |
 |
 |
 |
 |
 |
15 | 8.0 | 17.7 | 24.1 | 1.7 × 10−2 | 6.8 × 10−4 |
| 201754305.03(cde) | K2-16 |  |
 |
 |
 |
 |
 |
26 | 9.6 | 22.9 | 0.5 | 3.2 × 10−5 | 1.3 × 10−6 |
| 201833600.02(de) | K2-50 |  |
 |
 |
 |
 |
 |
18 | 8.0 | 12.7 | 10.0 | 8.3 × 10−3 | 3.3 × 10−4 |
| 201841433.02(d) |  |
 |
 |
 |
 |
 |
18 | 7.3 | 19.1 | 1.0 | 3.8 × 10−3 | 1.5 × 10−4 | |
| 205950854.02(di) | K2-168 |  |
 |
 |
 |
 |
 |
9 | 10.0 | 21.3 | 1.0 | 2.9 × 10−3 | 1.2 × 10−4 |
| 206024342.03(de) |  |
 |
 |
 |
 |
 |
13 | 11.3 | 25.1 | 27.0 | 2.4 × 10−2 | 9.7 × 10−4 | |
| 206032309.02(d) |  |
 |
 |
 |
 |
 |
24 | 11.9 | 20.7 | 1.0 | 8.1 × 10−3 | 3.3 × 10−4 | |
| 206042996.02(d) |  |
 |
 |
 |
 |
 |
12 | 9.7 | 19.7 | 1.0 | 8.4 × 10−4 | 3.4 × 10−5 | |
| 206215704.02(d) |  |
 |
 |
 |
 |
 |
29 | 12.4 | 22.5 | 1.0 | 1.1 × 10−1 | 5.0 × 10−3 | |
| 206317286.02(d) |  |
 |
 |
 |
 |
 |
42 | 10.2 | 25.2 | 1.0 | 1.1 × 10−2 | 4.6 × 10−4 | |
| 212297394.02(g) |  |
 |
 |
 |
 |
 |
33 | 11.1 | 24.2 | 1.0 | 4.4 × 10−3 | 1.8 × 10−4 | |
| 212424622.02(g) |  |
 |
 |
 |
 |
 |
4 | 8.5 | 19.0 | 1.0 | 2.2 × 10−2 | 9.2 × 10−4 | |
| 212499991.02(g) |  |
 |
 |
 |
 |
 |
2 | 9.1 | 11.9 | 11.1 | 2.0 × 10−1 | 9.9 × 10−3 | |
| 212587672.02(fgk) |  |
 |
 |
 |
 |
 |
5 | 8.6 | 18.5 | 23.5 | 1.3 × 10−1 | 6.1 × 10−3 | |
| 220554210.02(dk) | K2-282 |  |
 |
 |
 |
 |
 |
103 | 16.8 | 25.8 | 1.0 | 4.0 × 10−5 | 1.6 × 10−6 |
Notes. T0, P, Rp/Rs, and b obtained from MCMC fitting. #tr, S/N, and SDETLS obtained from TLS. FPP2 obtained with vespa and corrected for the multiplicity boost following Eq. (1). Rp [R⊕] derived from Rp/Rs as per TLS and literature values for the stellar radius. All stellar radii and masses from Huber et al. (2016), except for EPIC 201497682(l), EPIC 201615463(j), EPIC 201754305(d), EPIC 201841433(l), EPIC 205950854(j), EPIC 212297394(l), EPIC 212499991(l), EPIC 212587672(k), and EPIC 220554210(k). (a)T0 = BKJD − 2065 d with the Barycentric Kepler Julian Day BKJD = BJD − 2, 454, 833.0 d. (b)Number of transits detected with TLS that have data.
References. Planets or candidates have previously been found in these systems by (c) Montet et al. (2015), (d) Vanderburg et al. (2016), (e) Crossfield et al. (2016), (f) Barros et al. (2016), (g) Pope et al. (2016), (h) Dressing et al. (2017), (i) Mayo et al. (2018), (j) Livingston et al. (2018b), (k) Petigura et al. (2018). Gaia DR2 radii were computed by (l) Andrae et al. (2018).
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