Table 3
Detectability at each spectral band of the exoplanets within 30 pc that are potential targets (Pdetect >25%) in at least one band with 3 h of integration time.
I | J | H | K | |||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
Planet | d | a | Mp | Pdetect | αobs | Pdetect | αobs | Pdetect | αobs | Pdetect | αobs | |
(pc) | (AU) | (MJ) | (%) | (deg) | (%) | (deg) | (%) | (deg) | (%) | (deg) | ||
VLTI | HD 62509 b | 10.34 | 1.62 | 2.74 | 100.00 | ![]() |
100.00 | ![]() |
99.90 | ![]() |
97.80 | ![]() |
eps Eri b | 3.20 | 3.53 | 0.68 | 100.00 | ![]() |
100.00 | ![]() |
100.00 | ![]() |
0.00 | – | |
alf Tau b | 20.44 | 1.47 | 7.44 | 100.00 | ![]() |
100.00 | ![]() |
49.70 | ![]() |
0.00 | – | |
alf Ari b | 20.21 | 1.20 | 2.13 | 100.00 | ![]() |
100.00 | ![]() |
0.00 | – | 0.00 | – | |
GJ 876 b | 4.68 | 0.21 | 2.28 | 100.00 | ![]() |
100.00 | ![]() |
0.00 | – | 0.00 | – | |
GJ 896 A b | 6.26 | 0.64 | 2.23 | 71.60 | ![]() |
99.90 | ![]() |
0.00 | – | 0.00 | – | |
GJ 876 c | 4.68 | 0.13 | 0.71 | 100.00 | ![]() |
0.00 | – | 0.00 | – | 0.00 | – | |
GJ 9066 c | 4.47 | 0.88 | 0.24 | 12.70 | ![]() |
47.60 | ![]() |
0.00 | – | 0.00 | – | |
Extended VLTI | HD 62509 b | 10.34 | 1.62 | 2.74 | 100.00 | ![]() |
100.00 | ![]() |
99.90 | ![]() |
99.30 | ![]() |
alf Tau b | 20.44 | 1.47 | 7.44 | 100.00 | ![]() |
100.00 | ![]() |
99.70 | ![]() |
43.50 | ![]() |
|
eps Eri b | 3.20 | 3.53 | 0.68 | 100.00 | ![]() |
100.00 | ![]() |
100.00 | ![]() |
0.00 | – | |
alf Ari b | 20.21 | 1.20 | 2.13 | 100.00 | ![]() |
100.00 | ![]() |
0.00 | – | 0.00 | – | |
GJ 876 c | 4.68 | 0.13 | 0.71 | 100.00 | ![]() |
100.00 | ![]() |
0.00 | – | 0.00 | – | |
GJ 876 b | 4.68 | 0.21 | 2.28 | 100.00 | ![]() |
100.00 | ![]() |
0.00 | – | 0.00 | – | |
GJ 896 A b | 6.26 | 0.64 | 2.23 | 67.00 | ![]() |
100.00 | ![]() |
0.00 | – | 0.00 | – | |
HD 27442 b | 18.27 | 1.27 | 1.81 | 7.20 | ![]() |
71.30 | ![]() |
0.00 | – | 0.00 | – | |
nu Oct A b | 21.15 | 1.25 | 2.34 | 30.60 | ![]() |
47.10 | ![]() |
0.00 | – | 0.00 | – | |
61 Vir d | 8.50 | 0.48 | 0.08 | 41.20 | ![]() |
26.60 | ![]() |
0.00 | – | 0.00 | – | |
GJ 9066 c | 4.47 | 0.88 | 0.24 | 4.90 | ![]() |
54.50 | ![]() |
0.00 | – | 0.00 | – | |
HD 26965 b | 5.04 | 0.22 | 0.03 | 29.70 | ![]() |
21.80 | ![]() |
1.20 | ![]() |
0.00 | – | |
HD 147513 b | 12.90 | 1.32 | 1.39 | 50.30 | ![]() |
0.00 | – | 0.00 | – | 0.00 | – | |
HD 3651 b | 11.13 | 0.30 | 0.27 | 42.70 | ![]() |
0.00 | – | 0.00 | – | 0.00 | – |
Notes. Both the configurations assuming 4 or 5 telescopes are shown. In all cases, we adopted a value of A𝑔=0.3 for bands I and J, and A𝑔=0.1 for H and K. The corresponding targets in 30 h of integration time are displayed in Tables D.1 and D.2.
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