Table 1. Open in new tab Literature...

Parameter

IRAS 04125+2902

K2-33

TOI-1227

HIP 67522

AU Mic

V1298 Tau

K2-136

2MASS

J04154278|$+$|2909597

J16101473–1919095

J12270432–7227064

J13500627–4050090

J20450949–3120266

J04051959|$+$|2009256

J04293897|$+$|2252579

RA (J2000)|$^{a}$| (h:m:s)

04:15:42.80

16:10:14.73

12:27:04.16

13:50:06.24

20:45:09.88

04:05:19.60

04:29:39.09

DEC (J2000) (d:m:s)

+29:09:59.54

–19:19:09.79

–72:27:06.67

–40:50:09.24

–31:20:33.00

+20:09:25.31

+22:52:57.22

Age (Myr)

|$3.3^{+0.6}_{-0.5}$|

|$9.3^{+1.1}_{-1.3}$|

|$11 \pm 2$|

|$17 \pm 2$|

|$22 \pm 3$|

|$23 \pm 4$|

|$\simeq$|800

Prior

Age (Myr)

|$3 \pm 1$|

|$11 \pm 3$|

|$11 \pm 2$|

|$17 \pm 2$|

|$22 \pm 3$|

|$23 \pm 4$|

|$725 \pm 100$|

|$T_{\mathrm{eff}}$| (K)

|$3922 \pm 111$|

|$3450 \pm 70$|

|$5675 \pm 75$|

|$3700 \pm 100$|

|$4970 \pm 120$|

|$4499 \pm 50$|

|$A_V$| (mag)

|$2.253 \pm 0.128$|

|$0.64 \pm 0.08$|

|$0.21 \pm 0.1$|

DSEP Magnetic

|$M_{\star }$| (⁠|$\rm M_{\odot }$|⁠)

|$0.90^{+0.06}_{-0.06}$|

|$0.47^{+0.04}_{-0.04}$|

|$0.16^{+0.01}_{-0.01}$|

|$1.24^{+0.05}_{-0.04}$|

|$0.65^{+0.02}_{-0.02}$|

|$1.07^{+0.02}_{-0.02}$|

|$0.79^{+0.01}_{-0.01}$|

|$R_{\star }$| (⁠|$R_{\odot }$|⁠)

|$1.64^{+0.07}_{-0.05}$|

|$1.00^{+0.04}_{-0.04}$|

|$0.55^{+0.01}_{-0.01}$|

|$1.57^{+0.08}_{-0.06}$|

|$0.85^{+0.02}_{-0.02}$|

|$1.30^{+0.03}_{-0.03}$|

|$0.80^{+0.01}_{-0.01}$|

|$\rho _{\star }$| (⁠|$\rho _{\odot }$|⁠)

|$0.21^{+0.03}_{-0.03}$|

|$0.47^{+0.10}_{-0.07}$|

|$0.97^{+0.08}_{-0.08}$|

|$0.32^{+0.03}_{-0.03}$|

|$1.04^{+0.08}_{-0.09}$|

|$0.49^{+0.03}_{-0.03}$|

|$1.52^{+0.02}_{-0.02}$|

DSEP Non-Magnetic

|$M_{\star }$| (⁠|$\rm M_{\odot }$|⁠)

|$0.63^{+0.05}_{-0.04}$|

|$0.37^{+0.03}_{-0.03}$|

|$0.12^{+0.01}_{-0.01}$|

|$1.19^{+0.03}_{-0.03}$|

|$0.64^{+0.03}_{-0.03}$|

|$1.16^{+0.02}_{-0.02}$|

|$0.72^{+0.01}_{-0.01}$|

|$R_{\star }$| (⁠|$R_{\odot }$|⁠)

|$1.43^{+0.05}_{-0.05}$|

|$0.96^{+0.04}_{-0.05}$|

|$0.54^{+0.01}_{-0.01}$|

|$1.33^{+0.04}_{-0.04}$|

|$0.79^{+0.02}_{-0.02}$|

|$1.26^{+0.03}_{-0.03}$|

|$0.66^{+0.01}_{-0.01}$|

|$\rho _{\star }$| (⁠|$\rho _{\odot }$|⁠)

|$0.21^{+0.04}_{-0.03}$|

|$0.42^{+0.11}_{-0.07}$|

|$0.77^{+0.14}_{-0.09}$|

|$0.51^{+0.03}_{-0.04}$|

|$1.29^{+0.10}_{-0.10}$|

|$0.58^{+0.04}_{-0.03}$|

|$2.50^{+0.04}_{-0.05}$|

PARSEC

|$M_{\star }$| (⁠|$\rm M_{\odot }$|⁠)

|$0.67^{+0.02}_{-0.02}$|

|$0.51^{+0.03}_{-0.03}$|

|$0.22^{+0.01}_{-0.01}$|

|$1.18^{+0.03}_{-0.03}$|

|$0.68^{+0.02}_{-0.01}$|

|$1.15^{+0.01}_{-0.02}$|

|$R_{\star }$| (⁠|$R_{\odot }$|⁠)

|$1.46^{+0.01}_{-0.01}$|

|$1.02^{+0.04}_{-0.04}$|

|$0.65^{+0.03}_{-0.03}$|

|$1.31^{+0.04}_{-0.04}$|

|$0.83^{+0.02}_{-0.02}$|

|$1.24^{+0.02}_{-0.03}$|

|$\rho _{\star }$| (⁠|$\rho _{\odot }$|⁠)

|$0.214^{+0.001}_{-0.001}$|

|$0.46^{+0.10}_{-0.06}$|

|$0.79^{+0.12}_{-0.12}$|

|$0.53^{+0.03}_{-0.03}$|

|$1.17^{+0.08}_{-0.09}$|

|$0.61^{+0.03}_{-0.02}$|

Empirical (Literature)|$^{b}$|

|$M_{\star }$| (⁠|$\rm M_{\odot }$|⁠)

|$0.70 \pm 0.04$|

|$0.56^{+0.09}_{-0.09}$|

|$0.170 \pm 0.015$|

|$1.22 \pm 0.05$|

|$0.50 \pm 0.03$|

|$1.10 \pm 0.05$|

|$0.74 \pm 0.02$|

|$R_{\star }$| (⁠|$R_{\odot }$|⁠)

|$1.45 \pm 0.10$|

|$1.05^{+0.07}_{-0.07}$|

|$0.56 \pm 0.03$|

|$1.38 \pm 0.06$|

|$0.75 \pm 0.03$|

|$1.305 \pm 0.070$|

|$0.66 \pm 0.02$|

|$\rho _{\star }$| (⁠|$\rho _{\odot }$|⁠)

|$0.22 \pm 0.03$|

|$0.51^{+0.04}_{-0.07}$|

|$0.94 \pm 0.18$|

|$0.46 \pm 0.06$|

|$1.18 \pm 0.16$|

|$0.46 \pm 0.08$|

|$2.50^{+0.13}_{-0.12}$|

Ref.|$^{c}$|

7, 8

Parameter

IRAS 04125+2902

K2-33

TOI-1227

HIP 67522

AU Mic

V1298 Tau

K2-136

2MASS

J04154278|$+$|2909597

J16101473–1919095

J12270432–7227064

J13500627–4050090

J20450949–3120266

J04051959|$+$|2009256

J04293897|$+$|2252579

RA (J2000)|$^{a}$| (h:m:s)

04:15:42.80

16:10:14.73

12:27:04.16

13:50:06.24

20:45:09.88

04:05:19.60

04:29:39.09

DEC (J2000) (d:m:s)

+29:09:59.54

–19:19:09.79

–72:27:06.67

–40:50:09.24

–31:20:33.00

+20:09:25.31

+22:52:57.22

Age (Myr)

|$3.3^{+0.6}_{-0.5}$|

|$9.3^{+1.1}_{-1.3}$|

|$11 \pm 2$|

|$17 \pm 2$|

|$22 \pm 3$|

|$23 \pm 4$|

|$\simeq$|800

Prior

Age (Myr)

|$3 \pm 1$|

|$11 \pm 3$|

|$11 \pm 2$|

|$17 \pm 2$|

|$22 \pm 3$|

|$23 \pm 4$|

|$725 \pm 100$|

|$T_{\mathrm{eff}}$| (K)

|$3922 \pm 111$|

|$3450 \pm 70$|

|$5675 \pm 75$|

|$3700 \pm 100$|

|$4970 \pm 120$|

|$4499 \pm 50$|

|$A_V$| (mag)

|$2.253 \pm 0.128$|

|$0.64 \pm 0.08$|

|$0.21 \pm 0.1$|

DSEP Magnetic

|$M_{\star }$| (⁠|$\rm M_{\odot }$|⁠)

|$0.90^{+0.06}_{-0.06}$|

|$0.47^{+0.04}_{-0.04}$|

|$0.16^{+0.01}_{-0.01}$|

|$1.24^{+0.05}_{-0.04}$|

|$0.65^{+0.02}_{-0.02}$|

|$1.07^{+0.02}_{-0.02}$|

|$0.79^{+0.01}_{-0.01}$|

|$R_{\star }$| (⁠|$R_{\odot }$|⁠)

|$1.64^{+0.07}_{-0.05}$|

|$1.00^{+0.04}_{-0.04}$|

|$0.55^{+0.01}_{-0.01}$|

|$1.57^{+0.08}_{-0.06}$|

|$0.85^{+0.02}_{-0.02}$|

|$1.30^{+0.03}_{-0.03}$|

|$0.80^{+0.01}_{-0.01}$|

|$\rho _{\star }$| (⁠|$\rho _{\odot }$|⁠)

|$0.21^{+0.03}_{-0.03}$|

|$0.47^{+0.10}_{-0.07}$|

|$0.97^{+0.08}_{-0.08}$|

|$0.32^{+0.03}_{-0.03}$|

|$1.04^{+0.08}_{-0.09}$|

|$0.49^{+0.03}_{-0.03}$|

|$1.52^{+0.02}_{-0.02}$|

DSEP Non-Magnetic

|$M_{\star }$| (⁠|$\rm M_{\odot }$|⁠)

|$0.63^{+0.05}_{-0.04}$|

|$0.37^{+0.03}_{-0.03}$|

|$0.12^{+0.01}_{-0.01}$|

|$1.19^{+0.03}_{-0.03}$|

|$0.64^{+0.03}_{-0.03}$|

|$1.16^{+0.02}_{-0.02}$|

|$0.72^{+0.01}_{-0.01}$|

|$R_{\star }$| (⁠|$R_{\odot }$|⁠)

|$1.43^{+0.05}_{-0.05}$|

|$0.96^{+0.04}_{-0.05}$|

|$0.54^{+0.01}_{-0.01}$|

|$1.33^{+0.04}_{-0.04}$|

|$0.79^{+0.02}_{-0.02}$|

|$1.26^{+0.03}_{-0.03}$|

|$0.66^{+0.01}_{-0.01}$|

|$\rho _{\star }$| (⁠|$\rho _{\odot }$|⁠)

|$0.21^{+0.04}_{-0.03}$|

|$0.42^{+0.11}_{-0.07}$|

|$0.77^{+0.14}_{-0.09}$|

|$0.51^{+0.03}_{-0.04}$|

|$1.29^{+0.10}_{-0.10}$|

|$0.58^{+0.04}_{-0.03}$|

|$2.50^{+0.04}_{-0.05}$|

PARSEC

|$M_{\star }$| (⁠|$\rm M_{\odot }$|⁠)

|$0.67^{+0.02}_{-0.02}$|

|$0.51^{+0.03}_{-0.03}$|

|$0.22^{+0.01}_{-0.01}$|

|$1.18^{+0.03}_{-0.03}$|

|$0.68^{+0.02}_{-0.01}$|

|$1.15^{+0.01}_{-0.02}$|

|$R_{\star }$| (⁠|$R_{\odot }$|⁠)

|$1.46^{+0.01}_{-0.01}$|

|$1.02^{+0.04}_{-0.04}$|

|$0.65^{+0.03}_{-0.03}$|

|$1.31^{+0.04}_{-0.04}$|

|$0.83^{+0.02}_{-0.02}$|

|$1.24^{+0.02}_{-0.03}$|

|$\rho _{\star }$| (⁠|$\rho _{\odot }$|⁠)

|$0.214^{+0.001}_{-0.001}$|

|$0.46^{+0.10}_{-0.06}$|

|$0.79^{+0.12}_{-0.12}$|

|$0.53^{+0.03}_{-0.03}$|

|$1.17^{+0.08}_{-0.09}$|

|$0.61^{+0.03}_{-0.02}$|

Empirical (Literature)|$^{b}$|

|$M_{\star }$| (⁠|$\rm M_{\odot }$|⁠)

|$0.70 \pm 0.04$|

|$0.56^{+0.09}_{-0.09}$|

|$0.170 \pm 0.015$|

|$1.22 \pm 0.05$|

|$0.50 \pm 0.03$|

|$1.10 \pm 0.05$|

|$0.74 \pm 0.02$|

|$R_{\star }$| (⁠|$R_{\odot }$|⁠)

|$1.45 \pm 0.10$|

|$1.05^{+0.07}_{-0.07}$|

|$0.56 \pm 0.03$|

|$1.38 \pm 0.06$|

|$0.75 \pm 0.03$|

|$1.305 \pm 0.070$|

|$0.66 \pm 0.02$|

|$\rho _{\star }$| (⁠|$\rho _{\odot }$|⁠)

|$0.22 \pm 0.03$|

|$0.51^{+0.04}_{-0.07}$|

|$0.94 \pm 0.18$|

|$0.46 \pm 0.06$|

|$1.18 \pm 0.16$|

|$0.46 \pm 0.08$|

|$2.50^{+0.13}_{-0.12}$|

Ref.|$^{c}$|

7, 8

Table 1.

Open in new tab

Literature information and estimated stellar parameters for the sample of young planet hosts.

Parameter	IRAS 04125+2902	K2-33	TOI-1227	HIP 67522	AU Mic	V1298 Tau	K2-136
2MASS	J04154278\|$+$\|2909597	J16101473–1919095	J12270432–7227064	J13500627–4050090	J20450949–3120266	J04051959\|$+$\|2009256	J04293897\|$+$\|2252579
RA (J2000)\|$^{a}$\| (h:m:s)	04:15:42.80	16:10:14.73	12:27:04.16	13:50:06.24	20:45:09.88	04:05:19.60	04:29:39.09
DEC (J2000) (d:m:s)	+29:09:59.54	–19:19:09.79	–72:27:06.67	–40:50:09.24	–31:20:33.00	+20:09:25.31	+22:52:57.22
Age (Myr)	\|$3.3^{+0.6}_{-0.5}$\|	\|$9.3^{+1.1}_{-1.3}$\|	\|$11 \pm 2$\|	\|$17 \pm 2$\|	\|$22 \pm 3$\|	\|$23 \pm 4$\|	\|$\simeq$\|800
Prior
Age (Myr)	\|$3 \pm 1$\|	\|$11 \pm 3$\|	\|$11 \pm 2$\|	\|$17 \pm 2$\|	\|$22 \pm 3$\|	\|$23 \pm 4$\|	\|$725 \pm 100$\|
\|$T_{\mathrm{eff}}$\| (K)	\|$3922 \pm 111$\|	\|$3450 \pm 70$\|		\|$5675 \pm 75$\|	\|$3700 \pm 100$\|	\|$4970 \pm 120$\|	\|$4499 \pm 50$\|
\|$A_V$\| (mag)	\|$2.253 \pm 0.128$\|	\|$0.64 \pm 0.08$\|	\|$0.21 \pm 0.1$\|
DSEP Magnetic
\|$M_{\star }$\| (⁠\|$\rm M_{\odot }$\|⁠)	\|$0.90^{+0.06}_{-0.06}$\|	\|$0.47^{+0.04}_{-0.04}$\|	\|$0.16^{+0.01}_{-0.01}$\|	\|$1.24^{+0.05}_{-0.04}$\|	\|$0.65^{+0.02}_{-0.02}$\|	\|$1.07^{+0.02}_{-0.02}$\|	\|$0.79^{+0.01}_{-0.01}$\|
\|$R_{\star }$\| (⁠\|$R_{\odot }$\|⁠)	\|$1.64^{+0.07}_{-0.05}$\|	\|$1.00^{+0.04}_{-0.04}$\|	\|$0.55^{+0.01}_{-0.01}$\|	\|$1.57^{+0.08}_{-0.06}$\|	\|$0.85^{+0.02}_{-0.02}$\|	\|$1.30^{+0.03}_{-0.03}$\|	\|$0.80^{+0.01}_{-0.01}$\|
\|$\rho _{\star }$\| (⁠\|$\rho _{\odot }$\|⁠)	\|$0.21^{+0.03}_{-0.03}$\|	\|$0.47^{+0.10}_{-0.07}$\|	\|$0.97^{+0.08}_{-0.08}$\|	\|$0.32^{+0.03}_{-0.03}$\|	\|$1.04^{+0.08}_{-0.09}$\|	\|$0.49^{+0.03}_{-0.03}$\|	\|$1.52^{+0.02}_{-0.02}$\|
DSEP Non-Magnetic
\|$M_{\star }$\| (⁠\|$\rm M_{\odot }$\|⁠)	\|$0.63^{+0.05}_{-0.04}$\|	\|$0.37^{+0.03}_{-0.03}$\|	\|$0.12^{+0.01}_{-0.01}$\|	\|$1.19^{+0.03}_{-0.03}$\|	\|$0.64^{+0.03}_{-0.03}$\|	\|$1.16^{+0.02}_{-0.02}$\|	\|$0.72^{+0.01}_{-0.01}$\|
\|$R_{\star }$\| (⁠\|$R_{\odot }$\|⁠)	\|$1.43^{+0.05}_{-0.05}$\|	\|$0.96^{+0.04}_{-0.05}$\|	\|$0.54^{+0.01}_{-0.01}$\|	\|$1.33^{+0.04}_{-0.04}$\|	\|$0.79^{+0.02}_{-0.02}$\|	\|$1.26^{+0.03}_{-0.03}$\|	\|$0.66^{+0.01}_{-0.01}$\|
\|$\rho _{\star }$\| (⁠\|$\rho _{\odot }$\|⁠)	\|$0.21^{+0.04}_{-0.03}$\|	\|$0.42^{+0.11}_{-0.07}$\|	\|$0.77^{+0.14}_{-0.09}$\|	\|$0.51^{+0.03}_{-0.04}$\|	\|$1.29^{+0.10}_{-0.10}$\|	\|$0.58^{+0.04}_{-0.03}$\|	\|$2.50^{+0.04}_{-0.05}$\|
PARSEC
\|$M_{\star }$\| (⁠\|$\rm M_{\odot }$\|⁠)	\|$0.67^{+0.02}_{-0.02}$\|	\|$0.51^{+0.03}_{-0.03}$\|	\|$0.22^{+0.01}_{-0.01}$\|	\|$1.18^{+0.03}_{-0.03}$\|	\|$0.68^{+0.02}_{-0.01}$\|	\|$1.15^{+0.01}_{-0.02}$\|
\|$R_{\star }$\| (⁠\|$R_{\odot }$\|⁠)	\|$1.46^{+0.01}_{-0.01}$\|	\|$1.02^{+0.04}_{-0.04}$\|	\|$0.65^{+0.03}_{-0.03}$\|	\|$1.31^{+0.04}_{-0.04}$\|	\|$0.83^{+0.02}_{-0.02}$\|	\|$1.24^{+0.02}_{-0.03}$\|
\|$\rho _{\star }$\| (⁠\|$\rho _{\odot }$\|⁠)	\|$0.214^{+0.001}_{-0.001}$\|	\|$0.46^{+0.10}_{-0.06}$\|	\|$0.79^{+0.12}_{-0.12}$\|	\|$0.53^{+0.03}_{-0.03}$\|	\|$1.17^{+0.08}_{-0.09}$\|	\|$0.61^{+0.03}_{-0.02}$\|
Empirical (Literature)\|$^{b}$\|
\|$M_{\star }$\| (⁠\|$\rm M_{\odot }$\|⁠)	\|$0.70 \pm 0.04$\|	\|$0.56^{+0.09}_{-0.09}$\|	\|$0.170 \pm 0.015$\|	\|$1.22 \pm 0.05$\|	\|$0.50 \pm 0.03$\|	\|$1.10 \pm 0.05$\|	\|$0.74 \pm 0.02$\|
\|$R_{\star }$\| (⁠\|$R_{\odot }$\|⁠)	\|$1.45 \pm 0.10$\|	\|$1.05^{+0.07}_{-0.07}$\|	\|$0.56 \pm 0.03$\|	\|$1.38 \pm 0.06$\|	\|$0.75 \pm 0.03$\|	\|$1.305 \pm 0.070$\|	\|$0.66 \pm 0.02$\|
\|$\rho _{\star }$\| (⁠\|$\rho _{\odot }$\|⁠)	\|$0.22 \pm 0.03$\|	\|$0.51^{+0.04}_{-0.07}$\|	\|$0.94 \pm 0.18$\|	\|$0.46 \pm 0.06$\|	\|$1.18 \pm 0.16$\|	\|$0.46 \pm 0.08$\|	\|$2.50^{+0.13}_{-0.12}$\|
Ref.\|$^{c}$\|	1	2	3	4	5	6	7, 8

Parameter	IRAS 04125+2902	K2-33	TOI-1227	HIP 67522	AU Mic	V1298 Tau	K2-136
2MASS	J04154278\|$+$\|2909597	J16101473–1919095	J12270432–7227064	J13500627–4050090	J20450949–3120266	J04051959\|$+$\|2009256	J04293897\|$+$\|2252579
RA (J2000)\|$^{a}$\| (h:m:s)	04:15:42.80	16:10:14.73	12:27:04.16	13:50:06.24	20:45:09.88	04:05:19.60	04:29:39.09
DEC (J2000) (d:m:s)	+29:09:59.54	–19:19:09.79	–72:27:06.67	–40:50:09.24	–31:20:33.00	+20:09:25.31	+22:52:57.22
Age (Myr)	\|$3.3^{+0.6}_{-0.5}$\|	\|$9.3^{+1.1}_{-1.3}$\|	\|$11 \pm 2$\|	\|$17 \pm 2$\|	\|$22 \pm 3$\|	\|$23 \pm 4$\|	\|$\simeq$\|800
Prior
Age (Myr)	\|$3 \pm 1$\|	\|$11 \pm 3$\|	\|$11 \pm 2$\|	\|$17 \pm 2$\|	\|$22 \pm 3$\|	\|$23 \pm 4$\|	\|$725 \pm 100$\|
\|$T_{\mathrm{eff}}$\| (K)	\|$3922 \pm 111$\|	\|$3450 \pm 70$\|		\|$5675 \pm 75$\|	\|$3700 \pm 100$\|	\|$4970 \pm 120$\|	\|$4499 \pm 50$\|
\|$A_V$\| (mag)	\|$2.253 \pm 0.128$\|	\|$0.64 \pm 0.08$\|	\|$0.21 \pm 0.1$\|
DSEP Magnetic
\|$M_{\star }$\| (⁠\|$\rm M_{\odot }$\|⁠)	\|$0.90^{+0.06}_{-0.06}$\|	\|$0.47^{+0.04}_{-0.04}$\|	\|$0.16^{+0.01}_{-0.01}$\|	\|$1.24^{+0.05}_{-0.04}$\|	\|$0.65^{+0.02}_{-0.02}$\|	\|$1.07^{+0.02}_{-0.02}$\|	\|$0.79^{+0.01}_{-0.01}$\|
\|$R_{\star }$\| (⁠\|$R_{\odot }$\|⁠)	\|$1.64^{+0.07}_{-0.05}$\|	\|$1.00^{+0.04}_{-0.04}$\|	\|$0.55^{+0.01}_{-0.01}$\|	\|$1.57^{+0.08}_{-0.06}$\|	\|$0.85^{+0.02}_{-0.02}$\|	\|$1.30^{+0.03}_{-0.03}$\|	\|$0.80^{+0.01}_{-0.01}$\|
\|$\rho _{\star }$\| (⁠\|$\rho _{\odot }$\|⁠)	\|$0.21^{+0.03}_{-0.03}$\|	\|$0.47^{+0.10}_{-0.07}$\|	\|$0.97^{+0.08}_{-0.08}$\|	\|$0.32^{+0.03}_{-0.03}$\|	\|$1.04^{+0.08}_{-0.09}$\|	\|$0.49^{+0.03}_{-0.03}$\|	\|$1.52^{+0.02}_{-0.02}$\|
DSEP Non-Magnetic
\|$M_{\star }$\| (⁠\|$\rm M_{\odot }$\|⁠)	\|$0.63^{+0.05}_{-0.04}$\|	\|$0.37^{+0.03}_{-0.03}$\|	\|$0.12^{+0.01}_{-0.01}$\|	\|$1.19^{+0.03}_{-0.03}$\|	\|$0.64^{+0.03}_{-0.03}$\|	\|$1.16^{+0.02}_{-0.02}$\|	\|$0.72^{+0.01}_{-0.01}$\|
\|$R_{\star }$\| (⁠\|$R_{\odot }$\|⁠)	\|$1.43^{+0.05}_{-0.05}$\|	\|$0.96^{+0.04}_{-0.05}$\|	\|$0.54^{+0.01}_{-0.01}$\|	\|$1.33^{+0.04}_{-0.04}$\|	\|$0.79^{+0.02}_{-0.02}$\|	\|$1.26^{+0.03}_{-0.03}$\|	\|$0.66^{+0.01}_{-0.01}$\|
\|$\rho _{\star }$\| (⁠\|$\rho _{\odot }$\|⁠)	\|$0.21^{+0.04}_{-0.03}$\|	\|$0.42^{+0.11}_{-0.07}$\|	\|$0.77^{+0.14}_{-0.09}$\|	\|$0.51^{+0.03}_{-0.04}$\|	\|$1.29^{+0.10}_{-0.10}$\|	\|$0.58^{+0.04}_{-0.03}$\|	\|$2.50^{+0.04}_{-0.05}$\|
PARSEC
\|$M_{\star }$\| (⁠\|$\rm M_{\odot }$\|⁠)	\|$0.67^{+0.02}_{-0.02}$\|	\|$0.51^{+0.03}_{-0.03}$\|	\|$0.22^{+0.01}_{-0.01}$\|	\|$1.18^{+0.03}_{-0.03}$\|	\|$0.68^{+0.02}_{-0.01}$\|	\|$1.15^{+0.01}_{-0.02}$\|
\|$R_{\star }$\| (⁠\|$R_{\odot }$\|⁠)	\|$1.46^{+0.01}_{-0.01}$\|	\|$1.02^{+0.04}_{-0.04}$\|	\|$0.65^{+0.03}_{-0.03}$\|	\|$1.31^{+0.04}_{-0.04}$\|	\|$0.83^{+0.02}_{-0.02}$\|	\|$1.24^{+0.02}_{-0.03}$\|
\|$\rho _{\star }$\| (⁠\|$\rho _{\odot }$\|⁠)	\|$0.214^{+0.001}_{-0.001}$\|	\|$0.46^{+0.10}_{-0.06}$\|	\|$0.79^{+0.12}_{-0.12}$\|	\|$0.53^{+0.03}_{-0.03}$\|	\|$1.17^{+0.08}_{-0.09}$\|	\|$0.61^{+0.03}_{-0.02}$\|
Empirical (Literature)\|$^{b}$\|
\|$M_{\star }$\| (⁠\|$\rm M_{\odot }$\|⁠)	\|$0.70 \pm 0.04$\|	\|$0.56^{+0.09}_{-0.09}$\|	\|$0.170 \pm 0.015$\|	\|$1.22 \pm 0.05$\|	\|$0.50 \pm 0.03$\|	\|$1.10 \pm 0.05$\|	\|$0.74 \pm 0.02$\|
\|$R_{\star }$\| (⁠\|$R_{\odot }$\|⁠)	\|$1.45 \pm 0.10$\|	\|$1.05^{+0.07}_{-0.07}$\|	\|$0.56 \pm 0.03$\|	\|$1.38 \pm 0.06$\|	\|$0.75 \pm 0.03$\|	\|$1.305 \pm 0.070$\|	\|$0.66 \pm 0.02$\|
\|$\rho _{\star }$\| (⁠\|$\rho _{\odot }$\|⁠)	\|$0.22 \pm 0.03$\|	\|$0.51^{+0.04}_{-0.07}$\|	\|$0.94 \pm 0.18$\|	\|$0.46 \pm 0.06$\|	\|$1.18 \pm 0.16$\|	\|$0.46 \pm 0.08$\|	\|$2.50^{+0.13}_{-0.12}$\|
Ref.\|$^{c}$\|	1	2	3	4	5	6	7, 8

|$^{a}$| RA and DEC values from Gaia DR3.

|$^{b}$| Barber et al. (2024a) and Mann et al. (2022) used an ensemble of techniques to derive |$M_{\star }$| and |$R_{\star }$| for IRAS 04125+2902 and TOI-1227, respectively, which included stelpar.

|$^{c}$| Literature references: [1] Barber et al. (2024a), [2] Mann et al. (2016), [3] Mann et al. (2022), [4] Rizzuto et al. (2020), [5] Plavchan et al. (2020), [6] David et al. (2019a), [7] Brandt & Huang (2015), and [8] Mann et al. (2018).

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