Hidden magnetic fields of young suns | Astronomy & Astrophysics (A&A)

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Table 4.

Parameters of target stars.

HD	Name	Sp. type⁽¹⁾	T_eff ⁽²⁾	log g⁽²⁾	Age⁽⁷⁾	P_rot ⁽¹⁰⁾	Ro	v_e sin i	log L_X/L_bol ⁽⁷⁾	⁽¹⁴⁾
			(K)		(Myr)	(d)		(km s⁻¹)
1835	BE Cet	G3 V	5837	4.47	600⁽⁸⁾	7.78⁽¹¹⁾	0.659	6.3	−4.43⁽¹¹⁾	−4.43
20630	κ¹ Cet	G5 V	5742	4.49	600	9.3	0.696	4.7	−4.71	−4.40
29615		G3 V	5866⁽³⁾	4.41⁽⁶⁾	27	2.34	0.207	20.1	−3.62⁽¹³⁾
39587	χ¹ Ori	G0 V	5882	4.34	500	4.83	0.437	9.4	−4.64	−4.37
56124		G0 V	5848	4.46	4500	18	1.549	0.6	−5.23⁽¹³⁾	−4.78
72905	π¹ UMa	G1.5 V	5873⁽⁴⁾	4.44	500	4.9	0.437	9.6	−4.64	−4.33
73350	V401 Hya	G5 V	5802	4.48	510	12.3	0.993	3.2	−4.80	−4.50
76151		G3 V	5790	4.55	3600⁽²⁾	20.5	1.629	0.0	−5.12⁽¹³⁾	−4.66
82558	LQ Hya	K1 V	5000⁽⁵⁾	4.00⁽⁵⁾	50	1.601⁽⁵⁾	0.067	28.3	−3.06	−3.97
129333	EK Dra	G1.5 V	5845	4.47	120	2.606⁽¹²⁾	0.223	17.0	−3.60	−4.09
131156A	ξ Boo A	G7 V	5570	4.65	200⁽⁹⁾	6.4	0.400	4.9	−4.44	−4.32
166435		G1 IV	5843	4.44	3800	3.43	0.293	7.6	−4.08	−4.26
175726		G0 V	5998	4.41	500	3.92	0.434	12.4	−4.58	−4.38
190771		G2 V	5834	4.44	2700	8.8	0.742	3.4	−4.45	−4.39
206860	HN Peg	G0 V	5974	4.47	260	4.55	0.481	10.1	−4.65	−4.37

References. (1) Turon et al. (1993); (2) Valenti & Fischer (2005); (3) McDonald et al. (2012); (4) Gonzalez et al. (2010); (5) Cole et al. (2015); (6) Allende Prieto & Lambert (1999); (7) Vidotto et al. (2014); (8) Rosén et al. (2016); (9) Oláh et al. (2016); (10) See et al. (2019); (11) Wright et al. (2011); (12) Järvinen et al. (2018); (13) Boller et al. (2016); (14) Boro Saikia et al. (2018).

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