Table 7.

Orbital parameter of exoplanets detected around HD 69830. The source of the values in the table (Ref) is given in the final column: 1.(Laliotis et al. 2023), 2. This study.

PlanetParameterBest fitRef
P(d)|$8.66897\pm 0.00028$|1
e|$0.128\pm 0.028$|1
HD 69830 bK(m s−1)|$3.4\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$10.1^{+0.38}_{-0.37}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.14^{+1.75}_{-0.34}$|2
Orbital distance (AU)|$0.079\pm 0.001$|2
P(d)|$31.6158\pm 0.0051$|1
e|$0.03\pm 0.03$|1
HD 69830 cK (m s−1)|$2.6\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$12.09^{+0.55}_{-0.54}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.17^{+2.12}_{-0.11}$|2
Orbital distance (AU)|$0.188\pm 0.001$|2
P (d)|$201.4\pm 0.4$|1
e|$0.08\pm 0.07$|1
HD 69830 dK (m s−1)|$1.5\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$12.26^{+0.89}_{-0.88}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.17^{+2.17}_{-0.11}$|2
Orbital distance (AU)|$0.644\pm 0.001$|2
PlanetParameterBest fitRef
P(d)|$8.66897\pm 0.00028$|1
e|$0.128\pm 0.028$|1
HD 69830 bK(m s−1)|$3.4\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$10.1^{+0.38}_{-0.37}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.14^{+1.75}_{-0.34}$|2
Orbital distance (AU)|$0.079\pm 0.001$|2
P(d)|$31.6158\pm 0.0051$|1
e|$0.03\pm 0.03$|1
HD 69830 cK (m s−1)|$2.6\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$12.09^{+0.55}_{-0.54}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.17^{+2.12}_{-0.11}$|2
Orbital distance (AU)|$0.188\pm 0.001$|2
P (d)|$201.4\pm 0.4$|1
e|$0.08\pm 0.07$|1
HD 69830 dK (m s−1)|$1.5\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$12.26^{+0.89}_{-0.88}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.17^{+2.17}_{-0.11}$|2
Orbital distance (AU)|$0.644\pm 0.001$|2
Table 7.

Orbital parameter of exoplanets detected around HD 69830. The source of the values in the table (Ref) is given in the final column: 1.(Laliotis et al. 2023), 2. This study.

PlanetParameterBest fitRef
P(d)|$8.66897\pm 0.00028$|1
e|$0.128\pm 0.028$|1
HD 69830 bK(m s−1)|$3.4\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$10.1^{+0.38}_{-0.37}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.14^{+1.75}_{-0.34}$|2
Orbital distance (AU)|$0.079\pm 0.001$|2
P(d)|$31.6158\pm 0.0051$|1
e|$0.03\pm 0.03$|1
HD 69830 cK (m s−1)|$2.6\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$12.09^{+0.55}_{-0.54}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.17^{+2.12}_{-0.11}$|2
Orbital distance (AU)|$0.188\pm 0.001$|2
P (d)|$201.4\pm 0.4$|1
e|$0.08\pm 0.07$|1
HD 69830 dK (m s−1)|$1.5\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$12.26^{+0.89}_{-0.88}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.17^{+2.17}_{-0.11}$|2
Orbital distance (AU)|$0.644\pm 0.001$|2
PlanetParameterBest fitRef
P(d)|$8.66897\pm 0.00028$|1
e|$0.128\pm 0.028$|1
HD 69830 bK(m s−1)|$3.4\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$10.1^{+0.38}_{-0.37}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.14^{+1.75}_{-0.34}$|2
Orbital distance (AU)|$0.079\pm 0.001$|2
P(d)|$31.6158\pm 0.0051$|1
e|$0.03\pm 0.03$|1
HD 69830 cK (m s−1)|$2.6\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$12.09^{+0.55}_{-0.54}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.17^{+2.12}_{-0.11}$|2
Orbital distance (AU)|$0.188\pm 0.001$|2
P (d)|$201.4\pm 0.4$|1
e|$0.08\pm 0.07$|1
HD 69830 dK (m s−1)|$1.5\pm 0.1$|1
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|⁠)|$12.26^{+0.89}_{-0.88}$|1
|$M_{\rm DA}$| (M|$_{\rm Jup}$|⁠)|$0.17^{+2.17}_{-0.11}$|2
Orbital distance (AU)|$0.644\pm 0.001$|2
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