Table 3
Name, distance d, spectral type, completeness C, and expected number of detectable exoplanets (planet yield) for the best targets.
Name | d [pc] | Spec. type | C | Planet yield |
|
||||
Gl 887 | 3.28 | M2V | 0.85 | 2.7 |
Gl 15 A | 3.59 | M1.0V | 0.85 | 2.6 |
Gl 411 | 2.55 | M1.5V | 0.82 | 2.5 |
Gl 1 | 4.34 | M2V | 0.79 | 2.5 |
Gl 725 A | 3.57 | M3.0V | 0.76 | 2.4 |
Gl 338 A | 6.14 | M0.0V | 0.76 | 2.3 |
Gl 832 | 4.95 | M2/3V | 0.76 | 2.3 |
Gl 784 | 6.20 | M0V | 0.74 | 2.3 |
Gl 526 | 5.39 | M3V | 0.72 | 2.3 |
Gl 628 | 4.29 | M3V | 0.73 | 2.3 |
|
||||
α Cen A | 1.32 | G2V | 1.00 | 1.4 |
α Cen B | 1.32 | K1V | 1.00 | 1.4 |
Sirius A | 2.64 | A1V | 1.00 | 0.8 |
Procyon A | 3.51 | F5IV-V | 1.00 | 0.8 |
Altair | 5.13 | A7Vn | 0.99 | 0.9 |
Fomalhaut | 7.70 | A4V | 0.99 | 0.8 |
δ Pav | 6.11 | G8IV | 0.99 | 1.4 |
η Cas A | 5.95 | F9V | 0.99 | 0.8 |
Vega | 7.68 | A0Va | 0.99 | 0.8 |
ζ Tuc | 8.59 | F9.5V | 0.98 | 0.8 |
Notes. The top half of the table shows the best 10 targets according to the left panel of Fig. 4 (highest planet yield), and the bottom half shows the best 10 targets according to the right panel of Fig. 4 (highest completeness). Spectral types taken from the SIMBAD Astronomical Database (http://simbad.u-strasbg.fr/simbad/).
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