Table A.1
Targets 1–5 of our Warm Spitzer program.
| Star | BD-061339 | HD 1461 | HD 10180 | HD 13808 | HD 20003 |
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| d [parsec] | 20.3 ± 0.71 | 23.2 ± 0.31 | 39.0 ± 0.61 | 28.6 ± 0.51 | 43.8 ± 1.21 |
| V [mag] | 9.67 ± 0.042 | 6.46 ± 0.012 | 7.32 ± 0.0112 | 8.38 ± 0.012 | 8.37 ± 0.012 |
| K [mag] | 6.31 ± 0.023 | 4.90 ± 0.023 | 5.87 ± 0.023 | 6.25 ± 0.023 | 6.65 ± 0.023 |
| Spectral type | K7V/M0V4 | G3V7 | G1V13 | K2V13 | G8V16 |
| Teff [K]a | 4040 ± 505 | 5765 ± 508 | 5910 ± 5014 | 5035 ± 508 | 5495 ± 508 |
| [Fe/H] [dex] | −0.07 ± 0.105 | 0.19 ± 0.018 | 0.08 ± 0.0114 | −0.21 ± 0.028 | 0.04 ± 0.028 |
| M∗ [M⊙] | 0.63 ± 0.035 | 1.04 ± 0.078 | 1.06 ± 0.0514 | 0.77 ± 0.068 | 0.91 ± 0.078 |
| Bolometric correction | −1.07 ± 0.036 | −0.082 ± 0.0096 | −0.058 ± 0.0096 | −0.290 ± 0.0216 | −0.140 ± 0.0136 |
| R∗ [R⊙]b | 0.69 ± 0.02 | 1.10 ± 0.02 | 1.18 ± 0.02 | 0.81 ± 0.02 | 0.98 ± 0.02 |
| log g [cgs] | 4.56 ± 0.04 | 4.37 ± 0.04 | 4.32 ± 0.03 | 4.51 ± 0.05 | 4.41 ± 0.04 |
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| RV | |||||
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| Data | HARPS: 1024+10 | HARPS: 1679+8210+5 | HARPS: 19014+63 | HARPS: 1339+89 | HARPS: 1049+77 |
| PFS: 155 | Keck: 14411 | ||||
| Model | 2 Keplerians | 3 Keplerians | 6 Keplerians | 2 Keplerians | 4 Keplerians |
| + linear trend | + quadratic trend | + quadratic trend | |||
| +CCF function | +CCF function | ||||
| Jitter noise [m s-1] | HARPS: 2.7 | HARPS: 1.5 | 1.5 | 1.7 | 1.4 |
| PFS: 2.7 | Keck: 2.4 & 1.6e | ||||
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| Planet | BD-061339 b4 | HD 1461 b11 | HD 10180 c14 | HD 13808 b9,15 | HD 20003 b9,17 |
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| Mpsini [M⊕] | 6.93 ± 0.96 | 6.73 ± 0.47 | 13.11 ± 0.62 | 11.83 ± 0.88 | 11.79 ± 0.61 |
| Min. Rp [R⊕]c | 1.30 ± 0.05 | 1.29 ± 0.03 | 1.53 ± 0.02 | 1.50 ± 0.03 | 1.49 ± 0.02 |
| Min. (Rp/R∗)2 [ppm]c | 298 ± 29 | 115 ± 6 | 142 ± 6 | 286 ± 18 | 191 ± 9 |
| Teq [K]d | 796 ± 17 | 1154 ± 20 | 1223 ± 18 | 674 ± 14 | 836 ± 12 |
| T0-2 450 000 [BJDTDB] |
|
6549.30 ± 0.12 |
|
6537.49 ± 0.26 | 6538.34 ± 0.36 |
| P [d] | 3.87310 ± 0.00037 | 5.77198 ± 0.00030 | 5.75931 ± 0.00021 | 14.1853 ± 0.0019 | 11.8489 ± 0.0015 |
| Wb = 0 [min] | 139 ± 15 | 218 ± 11 | 238 ± 10 | 246 ± 13 | 388 ± 23 |
| K [m s-1] | 3.90 ± 0.52 | 2.34 ± 0.13 | 4.51 ± 0.15 | 3.73 ± 0.20 | 3.84 ± 0.20 |
| a [AU] | 0.04136 ± 0.00066 | 0.0638 ± 0.0015 | 0.0641 ± 0.0010 | 0.1050 ± 0.0028 | 0.09817 ± 0.00072 |
| e |
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0.377 ± 0.047 |
| ω [deg] |
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| Prior Ptransit [%] |
|
8.06 ± 0.38 |
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3.52 ± 0.18 | 3.43 ± 0.15 |
| Prior Poccultation [%] |
|
8.00 ± 0.38 |
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Notes. For each target, the table presents the assumed stellar parameters, the RV data and details of their analysis, and the parameters that we derived for the planet searched for transit from our RV analysis.
Assuming Mpsini = Mp. These minimum values correspond to a pure iron planet (Seager et al. 2007).
Assuming a null albedo and a heat distribution factor f′ = 1/4 (Seager 2010).
For the first and second Keck datasets presented in Rivera et al. (2010), respectively.
Reference. (1) Van Leeuwen (2007); (2) Kharchenko (2001); (3) Skrutskie et al. (2006); (4) Lo Curto et al. (2013); (5) Arriagada et al. (2013); (6) Flower (1996); (7) Gray et al. (2003); (8) Santos et al. (2013); (9) Mayor et al. (2011); (10) Díaz et al. (2016); (11) Rivera et al. (2010); (12) Hog et al. (2000); (13) Gray et al. (2006); (14) Lovis et al. (2011); (15) Queloz et al. (in prep.), (16) Houk & Cowley (1975); (17) Udry et al. (in prep.).
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