Table B1. Open in new tab Summary of the...

Star	Data	Rotation period	Decay time	Smoothing factor	Amplitude	White noise	Rms	\|$\chi ^2_{\rm r}$\|
Gl 905	c₁	\|$111.7^{+3.0}_{-3.2}$\|	\|$133^{+18}_{-22}$\|	\|$0.50^{+0.09}_{-0.07}$\|	\|$12.9^{+3.1}_{-2.1}$\|	\|$0.6^{+0.5}_{-0.4}$\|	3.8	0.79
Gl 905	B_ℓ	\|$114.4^{+3.5}_{-2.4}$\|	\|$130^{+25}_{-32}$\|	\|$0.44^{+0.12}_{-0.09}$\|	\|$14.1^{+3.5}_{-2.4}$\|	\|$1.2^{+1.1}_{-0.8}$\|	6.9	0.87
Gl 905	D23	114.3 ± 2.8	\|$129^{+25}_{-21}$\|	0.43 ± 0.09	\|$13.3^{+2.5}_{-2.1}$\|	\|$1.7^{+1.2}_{-0.7}$\|	6.2	0.84
GJ 1289	c₁	\|$75.62^{+0.85}_{-0.79}$\|	\|$129^{+26}_{-24}$\|	0.40 ± 0.05	\|$41.9^{+7.9}_{-6.0}$\|	\|$1.2^{+1.1}_{-0.8}$\|	6.9	0.72
GJ 1289	B_ℓ	\|$73.67^{+1.01}_{-0.91}$\|	\|$152^{+30}_{-28}$\|	0.48 ± 0.08	\|$53.3^{+11.7}_{-9.4}$\|	\|$3.2^{+2.4}_{-2.1}$\|	14.3	0.84
GJ 1289	D23	73.66 ± 0.92	\|$152^{+32}_{-27}$\|	0.48 ± 0.09	\|$53.2^{+12.4}_{-10.1}$\|	\|$4.2^{+2.7}_{-1.6}$\|	13.9	0.82
GJ 1151	c₁	\|$175.8^{+3.2}_{-3.4}$\|	300	\|$0.40^{+0.10}_{-0.09}$\|	\|$12.7^{+3.2}_{-2.4}$\|	3.3 ± 0.7	5.8	0.99
GJ 1151	B_ℓ	\|$176.1^{+3.6}_{-4.1}$\|	300	\|$0.42^{+0.10}_{-0.09}$\|	\|$14.6^{+3.4}_{-2.7}$\|	\|$1.1^{+1.1}_{-0.8}$\|	6.7	0.73
GJ 1151	D23	175.6 ± 4.9	300	0.43 ± 0.11	\|$14.9^{+4.2}_{-3.3}$\|	\|$1.6^{+1.3}_{-0.7}$\|	6.7	0.72
GJ 1286	c₁	\|$186.8^{+9.5}_{-5.8}$\|	300	\|$0.23^{+0.05}_{-0.04}$\|	\|$18.0^{+4.3}_{-3.1}$\|	\|$2.7^{+1.5}_{-1.7}$\|	7.5	1.02
GJ 1286	B_ℓ	\|$181^{+18}_{-13}$\|	300	\|$0.28^{+0.13}_{-0.07}$\|	\|$17.2^{+6.2}_{-3.6}$\|	\|$3.9^{+2.3}_{-2.4}$\|	12.0	1.03
GJ 1286	D23	178 ± 15	300	0.29 ± 0.09	\|$16.7^{+4.6}_{-3.6}$\|	\|$4.6^{+2.6}_{-1.6}$\|	10.1	1.02
Gl 617B	c₁	\|$37.8^{+8.5}_{-2.6}$\|	\|$35^{+8}_{-4}$\|	\|$0.47^{+0.09}_{-0.05}$\|	\|$5.9^{+1.2}_{-0.8}$\|	\|$0.7^{+0.6}_{-0.5}$\|	2.2	0.66
Gl 617B	B_ℓ	\|$40.6^{+2.1}_{-4.4}$\|	\|$82^{+45}_{-30}$\|	\|$0.58^{+0.13}_{-0.11}$\|	\|$5.5^{+1.3}_{-1.1}$\|	\|$1.3^{+1.0}_{-0.9}$\|	5.0	0.86
Gl 617B	D23	40.4 ± 3.0	\|$69^{+35}_{-23}$\|	0.60 ± 0.22	\|$5.4^{+1.3}_{-1.0}$\|	\|$1.7^{+1.1}_{-0.7}$\|	4.9	0.86
Gl 408	c₁	\|$175^{+12}_{-14}$\|	200	\|$0.18^{+0.10}_{-0.05}$\|	\|$4.2^{+0.9}_{-0.8}$\|	\|$2.2^{+0.5}_{-0.6}$\|	3.9	1.19
Gl 408	B_ℓ	\|$170.7^{+7.1}_{-9.8}$\|	200	\|$0.22^{+0.13}_{-0.08}$\|	\|$6.3^{+1.6}_{-1.2}$\|	\|$1.0^{+1.0}_{-0.7}$\|	6.9	0.72
Gl 408	D23	171.0 ± 8.4	200	0.21 ± 0.10	\|$6.3^{+1.5}_{-1.2}$\|	\|$1.5^{+1.2}_{-0.7}$\|	6.3	0.66

Star

Data

Rotation period

Decay time

Smoothing factor

Amplitude

White noise

Rms

|$\chi ^2_{\rm r}$|

P_rot (d)

l (d)

α (G)

σ (G)

(G)

Gl 905

c₁

|$111.7^{+3.0}_{-3.2}$|

|$133^{+18}_{-22}$|

|$0.50^{+0.09}_{-0.07}$|

|$12.9^{+3.1}_{-2.1}$|

|$0.6^{+0.5}_{-0.4}$|

3.8

0.79

Gl 905

B_ℓ

|$114.4^{+3.5}_{-2.4}$|

|$130^{+25}_{-32}$|

|$0.44^{+0.12}_{-0.09}$|

|$14.1^{+3.5}_{-2.4}$|

|$1.2^{+1.1}_{-0.8}$|

6.9

0.87

Gl 905

D23

114.3 ± 2.8

|$129^{+25}_{-21}$|

0.43 ± 0.09

|$13.3^{+2.5}_{-2.1}$|

|$1.7^{+1.2}_{-0.7}$|

6.2

0.84

GJ 1289

c₁

|$75.62^{+0.85}_{-0.79}$|

|$129^{+26}_{-24}$|

0.40 ± 0.05

|$41.9^{+7.9}_{-6.0}$|

|$1.2^{+1.1}_{-0.8}$|

6.9

0.72

GJ 1289

B_ℓ

|$73.67^{+1.01}_{-0.91}$|

|$152^{+30}_{-28}$|

0.48 ± 0.08

|$53.3^{+11.7}_{-9.4}$|

|$3.2^{+2.4}_{-2.1}$|

14.3

0.84

GJ 1289

D23

73.66 ± 0.92

|$152^{+32}_{-27}$|

0.48 ± 0.09

|$53.2^{+12.4}_{-10.1}$|

|$4.2^{+2.7}_{-1.6}$|

13.9

0.82

GJ 1151

c₁

|$175.8^{+3.2}_{-3.4}$|

300

|$0.40^{+0.10}_{-0.09}$|

|$12.7^{+3.2}_{-2.4}$|

3.3 ± 0.7

5.8

0.99

GJ 1151

B_ℓ

|$176.1^{+3.6}_{-4.1}$|

300

|$0.42^{+0.10}_{-0.09}$|

|$14.6^{+3.4}_{-2.7}$|

|$1.1^{+1.1}_{-0.8}$|

6.7

0.73

GJ 1151

D23

175.6 ± 4.9

300

0.43 ± 0.11

|$14.9^{+4.2}_{-3.3}$|

|$1.6^{+1.3}_{-0.7}$|

6.7

0.72

GJ 1286

c₁

|$186.8^{+9.5}_{-5.8}$|

300

|$0.23^{+0.05}_{-0.04}$|

|$18.0^{+4.3}_{-3.1}$|

|$2.7^{+1.5}_{-1.7}$|

7.5

1.02

GJ 1286

B_ℓ

|$181^{+18}_{-13}$|

300

|$0.28^{+0.13}_{-0.07}$|

|$17.2^{+6.2}_{-3.6}$|

|$3.9^{+2.3}_{-2.4}$|

12.0

1.03

GJ 1286

D23

178 ± 15

300

0.29 ± 0.09

|$16.7^{+4.6}_{-3.6}$|

|$4.6^{+2.6}_{-1.6}$|

10.1

1.02

Gl 617B

c₁

|$37.8^{+8.5}_{-2.6}$|

|$35^{+8}_{-4}$|

|$0.47^{+0.09}_{-0.05}$|

|$5.9^{+1.2}_{-0.8}$|

|$0.7^{+0.6}_{-0.5}$|

2.2

0.66

Gl 617B

B_ℓ

|$40.6^{+2.1}_{-4.4}$|

|$82^{+45}_{-30}$|

|$0.58^{+0.13}_{-0.11}$|

|$5.5^{+1.3}_{-1.1}$|

|$1.3^{+1.0}_{-0.9}$|

5.0

0.86

Gl 617B

D23

40.4 ± 3.0

|$69^{+35}_{-23}$|

0.60 ± 0.22

|$5.4^{+1.3}_{-1.0}$|

|$1.7^{+1.1}_{-0.7}$|

4.9

0.86

Gl 408

c₁

|$175^{+12}_{-14}$|

200

|$0.18^{+0.10}_{-0.05}$|

|$4.2^{+0.9}_{-0.8}$|

|$2.2^{+0.5}_{-0.6}$|

3.9

1.19

Gl 408

B_ℓ

|$170.7^{+7.1}_{-9.8}$|

200

|$0.22^{+0.13}_{-0.08}$|

|$6.3^{+1.6}_{-1.2}$|

|$1.0^{+1.0}_{-0.7}$|

6.9

0.72

Gl 408

D23

171.0 ± 8.4

200

0.21 ± 0.10

|$6.3^{+1.5}_{-1.2}$|

|$1.5^{+1.2}_{-0.7}$|

6.3

0.66

Star	Data	Rotation period	Decay time	Smoothing factor	Amplitude	White noise	Rms	\|$\chi ^2_{\rm r}$\|
Gl 905	c₁	\|$111.7^{+3.0}_{-3.2}$\|	\|$133^{+18}_{-22}$\|	\|$0.50^{+0.09}_{-0.07}$\|	\|$12.9^{+3.1}_{-2.1}$\|	\|$0.6^{+0.5}_{-0.4}$\|	3.8	0.79
Gl 905	B_ℓ	\|$114.4^{+3.5}_{-2.4}$\|	\|$130^{+25}_{-32}$\|	\|$0.44^{+0.12}_{-0.09}$\|	\|$14.1^{+3.5}_{-2.4}$\|	\|$1.2^{+1.1}_{-0.8}$\|	6.9	0.87
Gl 905	D23	114.3 ± 2.8	\|$129^{+25}_{-21}$\|	0.43 ± 0.09	\|$13.3^{+2.5}_{-2.1}$\|	\|$1.7^{+1.2}_{-0.7}$\|	6.2	0.84
GJ 1289	c₁	\|$75.62^{+0.85}_{-0.79}$\|	\|$129^{+26}_{-24}$\|	0.40 ± 0.05	\|$41.9^{+7.9}_{-6.0}$\|	\|$1.2^{+1.1}_{-0.8}$\|	6.9	0.72
GJ 1289	B_ℓ	\|$73.67^{+1.01}_{-0.91}$\|	\|$152^{+30}_{-28}$\|	0.48 ± 0.08	\|$53.3^{+11.7}_{-9.4}$\|	\|$3.2^{+2.4}_{-2.1}$\|	14.3	0.84
GJ 1289	D23	73.66 ± 0.92	\|$152^{+32}_{-27}$\|	0.48 ± 0.09	\|$53.2^{+12.4}_{-10.1}$\|	\|$4.2^{+2.7}_{-1.6}$\|	13.9	0.82
GJ 1151	c₁	\|$175.8^{+3.2}_{-3.4}$\|	300	\|$0.40^{+0.10}_{-0.09}$\|	\|$12.7^{+3.2}_{-2.4}$\|	3.3 ± 0.7	5.8	0.99
GJ 1151	B_ℓ	\|$176.1^{+3.6}_{-4.1}$\|	300	\|$0.42^{+0.10}_{-0.09}$\|	\|$14.6^{+3.4}_{-2.7}$\|	\|$1.1^{+1.1}_{-0.8}$\|	6.7	0.73
GJ 1151	D23	175.6 ± 4.9	300	0.43 ± 0.11	\|$14.9^{+4.2}_{-3.3}$\|	\|$1.6^{+1.3}_{-0.7}$\|	6.7	0.72
GJ 1286	c₁	\|$186.8^{+9.5}_{-5.8}$\|	300	\|$0.23^{+0.05}_{-0.04}$\|	\|$18.0^{+4.3}_{-3.1}$\|	\|$2.7^{+1.5}_{-1.7}$\|	7.5	1.02
GJ 1286	B_ℓ	\|$181^{+18}_{-13}$\|	300	\|$0.28^{+0.13}_{-0.07}$\|	\|$17.2^{+6.2}_{-3.6}$\|	\|$3.9^{+2.3}_{-2.4}$\|	12.0	1.03
GJ 1286	D23	178 ± 15	300	0.29 ± 0.09	\|$16.7^{+4.6}_{-3.6}$\|	\|$4.6^{+2.6}_{-1.6}$\|	10.1	1.02
Gl 617B	c₁	\|$37.8^{+8.5}_{-2.6}$\|	\|$35^{+8}_{-4}$\|	\|$0.47^{+0.09}_{-0.05}$\|	\|$5.9^{+1.2}_{-0.8}$\|	\|$0.7^{+0.6}_{-0.5}$\|	2.2	0.66
Gl 617B	B_ℓ	\|$40.6^{+2.1}_{-4.4}$\|	\|$82^{+45}_{-30}$\|	\|$0.58^{+0.13}_{-0.11}$\|	\|$5.5^{+1.3}_{-1.1}$\|	\|$1.3^{+1.0}_{-0.9}$\|	5.0	0.86
Gl 617B	D23	40.4 ± 3.0	\|$69^{+35}_{-23}$\|	0.60 ± 0.22	\|$5.4^{+1.3}_{-1.0}$\|	\|$1.7^{+1.1}_{-0.7}$\|	4.9	0.86
Gl 408	c₁	\|$175^{+12}_{-14}$\|	200	\|$0.18^{+0.10}_{-0.05}$\|	\|$4.2^{+0.9}_{-0.8}$\|	\|$2.2^{+0.5}_{-0.6}$\|	3.9	1.19
Gl 408	B_ℓ	\|$170.7^{+7.1}_{-9.8}$\|	200	\|$0.22^{+0.13}_{-0.08}$\|	\|$6.3^{+1.6}_{-1.2}$\|	\|$1.0^{+1.0}_{-0.7}$\|	6.9	0.72
Gl 408	D23	171.0 ± 8.4	200	0.21 ± 0.10	\|$6.3^{+1.5}_{-1.2}$\|	\|$1.5^{+1.2}_{-0.7}$\|	6.3	0.66

Table B1.

Open in new tab

Summary of the best-fitting parameters of the QP GPR fits applied to c₁ and B_ℓ for the six M dwarfs in our sample and the comparison with the corresponding GPR results for B_ℓ by D23 marked as D23 in the second column.

Star	Data	Rotation period	Decay time	Smoothing factor	Amplitude	White noise	Rms	\|$\chi ^2_{\rm r}$\|
		P_rot (d)	l (d)	β	α (G)	σ (G)	(G)
Gl 905	c₁	\|$111.7^{+3.0}_{-3.2}$\|	\|$133^{+18}_{-22}$\|	\|$0.50^{+0.09}_{-0.07}$\|	\|$12.9^{+3.1}_{-2.1}$\|	\|$0.6^{+0.5}_{-0.4}$\|	3.8	0.79
Gl 905	B_ℓ	\|$114.4^{+3.5}_{-2.4}$\|	\|$130^{+25}_{-32}$\|	\|$0.44^{+0.12}_{-0.09}$\|	\|$14.1^{+3.5}_{-2.4}$\|	\|$1.2^{+1.1}_{-0.8}$\|	6.9	0.87
Gl 905	D23	114.3 ± 2.8	\|$129^{+25}_{-21}$\|	0.43 ± 0.09	\|$13.3^{+2.5}_{-2.1}$\|	\|$1.7^{+1.2}_{-0.7}$\|	6.2	0.84
GJ 1289	c₁	\|$75.62^{+0.85}_{-0.79}$\|	\|$129^{+26}_{-24}$\|	0.40 ± 0.05	\|$41.9^{+7.9}_{-6.0}$\|	\|$1.2^{+1.1}_{-0.8}$\|	6.9	0.72
GJ 1289	B_ℓ	\|$73.67^{+1.01}_{-0.91}$\|	\|$152^{+30}_{-28}$\|	0.48 ± 0.08	\|$53.3^{+11.7}_{-9.4}$\|	\|$3.2^{+2.4}_{-2.1}$\|	14.3	0.84
GJ 1289	D23	73.66 ± 0.92	\|$152^{+32}_{-27}$\|	0.48 ± 0.09	\|$53.2^{+12.4}_{-10.1}$\|	\|$4.2^{+2.7}_{-1.6}$\|	13.9	0.82
GJ 1151	c₁	\|$175.8^{+3.2}_{-3.4}$\|	300	\|$0.40^{+0.10}_{-0.09}$\|	\|$12.7^{+3.2}_{-2.4}$\|	3.3 ± 0.7	5.8	0.99
GJ 1151	B_ℓ	\|$176.1^{+3.6}_{-4.1}$\|	300	\|$0.42^{+0.10}_{-0.09}$\|	\|$14.6^{+3.4}_{-2.7}$\|	\|$1.1^{+1.1}_{-0.8}$\|	6.7	0.73
GJ 1151	D23	175.6 ± 4.9	300	0.43 ± 0.11	\|$14.9^{+4.2}_{-3.3}$\|	\|$1.6^{+1.3}_{-0.7}$\|	6.7	0.72
GJ 1286	c₁	\|$186.8^{+9.5}_{-5.8}$\|	300	\|$0.23^{+0.05}_{-0.04}$\|	\|$18.0^{+4.3}_{-3.1}$\|	\|$2.7^{+1.5}_{-1.7}$\|	7.5	1.02
GJ 1286	B_ℓ	\|$181^{+18}_{-13}$\|	300	\|$0.28^{+0.13}_{-0.07}$\|	\|$17.2^{+6.2}_{-3.6}$\|	\|$3.9^{+2.3}_{-2.4}$\|	12.0	1.03
GJ 1286	D23	178 ± 15	300	0.29 ± 0.09	\|$16.7^{+4.6}_{-3.6}$\|	\|$4.6^{+2.6}_{-1.6}$\|	10.1	1.02
Gl 617B	c₁	\|$37.8^{+8.5}_{-2.6}$\|	\|$35^{+8}_{-4}$\|	\|$0.47^{+0.09}_{-0.05}$\|	\|$5.9^{+1.2}_{-0.8}$\|	\|$0.7^{+0.6}_{-0.5}$\|	2.2	0.66
Gl 617B	B_ℓ	\|$40.6^{+2.1}_{-4.4}$\|	\|$82^{+45}_{-30}$\|	\|$0.58^{+0.13}_{-0.11}$\|	\|$5.5^{+1.3}_{-1.1}$\|	\|$1.3^{+1.0}_{-0.9}$\|	5.0	0.86
Gl 617B	D23	40.4 ± 3.0	\|$69^{+35}_{-23}$\|	0.60 ± 0.22	\|$5.4^{+1.3}_{-1.0}$\|	\|$1.7^{+1.1}_{-0.7}$\|	4.9	0.86
Gl 408	c₁	\|$175^{+12}_{-14}$\|	200	\|$0.18^{+0.10}_{-0.05}$\|	\|$4.2^{+0.9}_{-0.8}$\|	\|$2.2^{+0.5}_{-0.6}$\|	3.9	1.19
Gl 408	B_ℓ	\|$170.7^{+7.1}_{-9.8}$\|	200	\|$0.22^{+0.13}_{-0.08}$\|	\|$6.3^{+1.6}_{-1.2}$\|	\|$1.0^{+1.0}_{-0.7}$\|	6.9	0.72
Gl 408	D23	171.0 ± 8.4	200	0.21 ± 0.10	\|$6.3^{+1.5}_{-1.2}$\|	\|$1.5^{+1.2}_{-0.7}$\|	6.3	0.66

Star	Data	Rotation period	Decay time	Smoothing factor	Amplitude	White noise	Rms	\|$\chi ^2_{\rm r}$\|
		P_rot (d)	l (d)	β	α (G)	σ (G)	(G)
Gl 905	c₁	\|$111.7^{+3.0}_{-3.2}$\|	\|$133^{+18}_{-22}$\|	\|$0.50^{+0.09}_{-0.07}$\|	\|$12.9^{+3.1}_{-2.1}$\|	\|$0.6^{+0.5}_{-0.4}$\|	3.8	0.79
Gl 905	B_ℓ	\|$114.4^{+3.5}_{-2.4}$\|	\|$130^{+25}_{-32}$\|	\|$0.44^{+0.12}_{-0.09}$\|	\|$14.1^{+3.5}_{-2.4}$\|	\|$1.2^{+1.1}_{-0.8}$\|	6.9	0.87
Gl 905	D23	114.3 ± 2.8	\|$129^{+25}_{-21}$\|	0.43 ± 0.09	\|$13.3^{+2.5}_{-2.1}$\|	\|$1.7^{+1.2}_{-0.7}$\|	6.2	0.84
GJ 1289	c₁	\|$75.62^{+0.85}_{-0.79}$\|	\|$129^{+26}_{-24}$\|	0.40 ± 0.05	\|$41.9^{+7.9}_{-6.0}$\|	\|$1.2^{+1.1}_{-0.8}$\|	6.9	0.72
GJ 1289	B_ℓ	\|$73.67^{+1.01}_{-0.91}$\|	\|$152^{+30}_{-28}$\|	0.48 ± 0.08	\|$53.3^{+11.7}_{-9.4}$\|	\|$3.2^{+2.4}_{-2.1}$\|	14.3	0.84
GJ 1289	D23	73.66 ± 0.92	\|$152^{+32}_{-27}$\|	0.48 ± 0.09	\|$53.2^{+12.4}_{-10.1}$\|	\|$4.2^{+2.7}_{-1.6}$\|	13.9	0.82
GJ 1151	c₁	\|$175.8^{+3.2}_{-3.4}$\|	300	\|$0.40^{+0.10}_{-0.09}$\|	\|$12.7^{+3.2}_{-2.4}$\|	3.3 ± 0.7	5.8	0.99
GJ 1151	B_ℓ	\|$176.1^{+3.6}_{-4.1}$\|	300	\|$0.42^{+0.10}_{-0.09}$\|	\|$14.6^{+3.4}_{-2.7}$\|	\|$1.1^{+1.1}_{-0.8}$\|	6.7	0.73
GJ 1151	D23	175.6 ± 4.9	300	0.43 ± 0.11	\|$14.9^{+4.2}_{-3.3}$\|	\|$1.6^{+1.3}_{-0.7}$\|	6.7	0.72
GJ 1286	c₁	\|$186.8^{+9.5}_{-5.8}$\|	300	\|$0.23^{+0.05}_{-0.04}$\|	\|$18.0^{+4.3}_{-3.1}$\|	\|$2.7^{+1.5}_{-1.7}$\|	7.5	1.02
GJ 1286	B_ℓ	\|$181^{+18}_{-13}$\|	300	\|$0.28^{+0.13}_{-0.07}$\|	\|$17.2^{+6.2}_{-3.6}$\|	\|$3.9^{+2.3}_{-2.4}$\|	12.0	1.03
GJ 1286	D23	178 ± 15	300	0.29 ± 0.09	\|$16.7^{+4.6}_{-3.6}$\|	\|$4.6^{+2.6}_{-1.6}$\|	10.1	1.02
Gl 617B	c₁	\|$37.8^{+8.5}_{-2.6}$\|	\|$35^{+8}_{-4}$\|	\|$0.47^{+0.09}_{-0.05}$\|	\|$5.9^{+1.2}_{-0.8}$\|	\|$0.7^{+0.6}_{-0.5}$\|	2.2	0.66
Gl 617B	B_ℓ	\|$40.6^{+2.1}_{-4.4}$\|	\|$82^{+45}_{-30}$\|	\|$0.58^{+0.13}_{-0.11}$\|	\|$5.5^{+1.3}_{-1.1}$\|	\|$1.3^{+1.0}_{-0.9}$\|	5.0	0.86
Gl 617B	D23	40.4 ± 3.0	\|$69^{+35}_{-23}$\|	0.60 ± 0.22	\|$5.4^{+1.3}_{-1.0}$\|	\|$1.7^{+1.1}_{-0.7}$\|	4.9	0.86
Gl 408	c₁	\|$175^{+12}_{-14}$\|	200	\|$0.18^{+0.10}_{-0.05}$\|	\|$4.2^{+0.9}_{-0.8}$\|	\|$2.2^{+0.5}_{-0.6}$\|	3.9	1.19
Gl 408	B_ℓ	\|$170.7^{+7.1}_{-9.8}$\|	200	\|$0.22^{+0.13}_{-0.08}$\|	\|$6.3^{+1.6}_{-1.2}$\|	\|$1.0^{+1.0}_{-0.7}$\|	6.9	0.72
Gl 408	D23	171.0 ± 8.4	200	0.21 ± 0.10	\|$6.3^{+1.5}_{-1.2}$\|	\|$1.5^{+1.2}_{-0.7}$\|	6.3	0.66

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