STEPARSYN: A Bayesian code to infer stellar atmospheric parameters using spectral synthesis

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Volume 657 (January 2022)

A&A, 657 (2022) A66

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Table A.2.

Reference stellar atmospheric parameters for the stars analysed in this work.

Name	SpT	T_eff	log g	Ref.^a	[Fe/H]	Ref.^b	v sin i	Ref.^c
		[K]	[dex]		[dex]		[km s⁻¹]
Sun	G2 V	5771 ± 1	4.44 ± 0.01	Hei15	0.03 ± 0.05	Jof14	1.6	Vf05
HD 4628	K2 V	4950 ± 14	4.64 ± 0.01	Boy12b^d	−0.27 ± 0.04	Pastel	2.0	Mar14
η Cas A	G0 V	6003 ± 24	4.39 ± 0.01	Boy12a^d	−0.27 ± 0.07	Pastel	5.4	Luc17
μ Cas	G5 Vb	5308 ± 29	4.41 ± 0.06	Hei15	−0.81 ± 0.03	Jof14	1.1	Hal94
τ Cet	G8.5 V	5414 ± 21	4.49 ± 0.03	Hei15	−0.49 ± 0.03	Jof14	1.6	Jen11
HD 16160	K3 V	4662 ± 17	4.52 ± 0.01	Boy12b^d	−0.13 ± 0.06	Pastel	1.3	Que98
θ Per A	F7 V	6157 ± 37	4.26 ± 0.01	Boy12a^d	0.00 ± 0.08	Pastel	10.2	Luc17
α Cet	M1.5 IIIa	3796 ± 65	0.68 ± 0.23	Hei15	−0.45 ± 0.47	Jof14	6.9	Mas08
ϵ Eri	K2 V	5076 ± 30	4.61 ± 0.03	Hei15	−0.09 ± 0.06	Jof14	6.2	Bud19
HD 22879	F9 V	5868 ± 89	4.27 ± 0.04	Hei15	−0.86 ± 0.05	Jof14	4.2	Bud19
δ Eri	K1 III-IV	4954 ± 30	3.76 ± 0.02	Hei15	0.06 ± 0.05	Jof14	3.2	Sot18
Aldebaran	K5 III	3927 ± 40	1.11 ± 0.19	Hei15	−0.37 ± 0.17	Jof14	4.3	Mas08
π³ Ori	F6 V	6516 ± 19	4.31 ± 0.01	Boy12a^d	0.05 ± 0.07	Pastel	18.5	Luc17
HD 49933	F2 V	6635 ± 91	4.20 ± 0.03	Hei15	−0.41 ± 0.08	Jof14	5.0	Tak05
Procyon	F5 IV-V	6554 ± 84	4.00 ± 0.02	Hei15	0.01 ± 0.08	Jof14	7.4	Luc17
β Gem	K0 IIIb	4858 ± 60	2.90 ± 0.08	Hei15	0.13 ± 0.16	Jof14	2.8	Mas08
μ Leo	K2 III	4474 ± 60	2.51 ± 0.11	Hei15	0.25 ± 0.15	Jof14	4.5	Mas08
20 LMi	G3 V	5612 ± 52	4.26 ± 0.03	Boy12a^d	0.18 ± 0.12	Pastel	4.7	Luc17
36 UMa	F8 V	6233 ± 68	4.41 ± 0.03	Boy12a^d	−0.13 ± 0.05	Pastel	5.3	Luc17
β Vir	F9 V	6083 ± 41	4.10 ± 0.02	Hei15	0.24 ± 0.07	Jof14	6.4	Luc17
Gmb 1830	G8 Vp	4827 ± 55	4.60 ± 0.03	Hei15	−1.46 ± 0.39	Jof14	0.0	Lat02
HD107328	K0 IIIb	4496 ± 59	2.09 ± 0.13	Hei15	−0.33 ± 0.16	Jof14	1.9	Mas08
ϵ Vir	G8 III	4983 ± 61	2.77 ± 0.02	Hei15	0.15 ± 0.16	Jof14	1.4	Jof15
β Com	G0 V	5936 ± 33	4.37 ± 0.01	Boy12a^d	0.07 ± 0.09	Pastel	6.6	Luc17
η Boo	G0 IV	6099 ± 28	3.79 ± 0.02	Hei15	0.32 ± 0.08	Jof14	14.4	Luc17
Arcturus	K1.5 III	4286 ± 35	1.60 ± 0.20	Hei15	−0.52 ± 0.08	Jof14	4.2	Mas08
θ Boo A	F7 V	6265 ± 41	4.05 ± 0.04	Boy12a^d	−0.03 ± 0.03	Pastel	30.4	Luc17
18 Sco	G2 Va	5810 ± 80	4.44 ± 0.03	Hei15	0.03 ± 0.03	Jof14	4.4	Luc17
γ Sge	M0 III	3807 ± 49	1.05 ± 0.32	Hei15	−0.17 ± 0.39	Jof14	5.8	Mas08
HD 189733	K2 V	4875 ± 43	4.56 ± 0.03	Boy15^d	−0.02 ± 0.04	Pastel	4.5	Luc17
61 Cyg A	K5 V	4374 ± 22	4.63 ± 0.04	Hei15	−0.33 ± 0.38	Jof14	1.9	Que98
61 Cyg B	K7 V	4044 ± 32	4.67 ± 0.04	Hei15	−0.38 ± 0.03	Jof14	0.7	Que98
HD 209458	F9 V	6092 ± 103	4.28 ± 0.10	Boy15^d	0.03 ± 0.05	Pastel	3.9	Sot18
ξ Peg	F7 V	6168 ± 36	3.95 ± 0.01	Boy12a^d	−0.27 ± 0.08	Pastel	9.7	Luc17
HD 220009	K2 III	4217 ± 60	1.43 ± 0.12	Hei15	−0.74 ± 0.13	Jof14	1.2	Med99

Notes.

T_eff and log g reference. Hei15: Heiter et al. (2015a); Boy12a: Boyajian et al. (2012a); Boy12b: Boyajian et al. (2012b); Boy15: Boyajian et al. (2015).

[Fe/H] reference. Jof14: Jofré et al. (2014); Pastel: Literature average computed from the PASTEL catalogue (Soubiran et al. 2016).

v sin i reference. Hal94: Hale (1994); Que98: Queloz et al. (1998); Med99: de Medeiros & Mayor (1999); Lat02: Latham et al. (2002); Tak05: Takeda et al. (2005); Vf05: Valenti & Fischer (2005); Mas08: Massarotti et al. (2008); Jen11: Jenkins et al. (2011); Mar14: Marsden et al. (2014); Jof15: Jofré et al. (2015); Luc17: Luck (2017); Sot18: Soto & Jenkins (2018); Bud19: Buder et al. (2019).

log g values were computed from the corresponding literature values of mass and radius.

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