Chromospheric activity and rotation of FGK stars in the solar vicinity - An estimation of the radial velocity jitter

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Volume 520 (September-October 2010)

A&A, 520 (2010) A79

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Table 2:

Inactive stars used as references in the subtraction technique to measure chromospheric activity.
HIP	SpT	B-V	$v \sin{i}$	Obs.¹	$\log (F_{\rm H} + F_{\rm K})$	HIP	SpT	B-V	v $\sin{i}$	Obs.¹	$\log (F_{\rm H} + F_{\rm K})$
			(km s^-1)		(erg cm $^{\rm -2}$ s $^{\rm -1}$ )				(km s^-1)		(erg cm $^{\rm -2}$ s $^{\rm -1}$ )
37279	F5V	0.420	5.38	Mc	0.76^a	8102	G8V	0.730	8.00	Mc	0.15^a, 0.14^d
910	F5V	0.489	4.88	S	...	79492	G8V	0.756	2.68	FO	0.12^a, 0.11^d
78072	F6IV	0.480	11.42	FO	0.57^a	95319	G8V	0.805	0.60	FO	-0.05^a, 0.01^d
22449	F6V	0.475	19.22	Mc	0.71^a,d	101997	G8V	0.730	3.50	S	0.16^d
40035	F7V	0.495	11.26	S	...	47080	G8V	0.779	6.97	FO/S/Mc	0.30^a
27072	F7V	0.498	...	FE	...	63366	G9V	0.780	...	FE	0.12^a
17147	F9V	0.538	9.70	FO	0.48^d	74537	K0V	0.761	2.12	S	...
57757	F9V	0.558	3.41	Mc	0.44^d	40693	K0V	0.766	$\leq$ 6.79	Mc	0.09^d
16852	F9V	0.568	2.67	Mc	0.39^a, 0.37^d	84195	K0	0.940	8.58	FO	-0.20^d
1599	F9V	0.576	$\leq$ 3.23	FE	0.45^b	112190	K0	0.968	$\leq$ 3.35	FO	-0.12^d
64394	F9.5V	0.588	4.72	Mc	0.48^a,d	3093	K0.5V	0.853	9.38	FO/S/Mc	-0.05^a, -0.11^d
61317	G0V	0.589	2.00	Mc	0.43^a, 0.41^d	7981	K1V	0.834	6.50	FO/S/Mc	-0.01^a, -0.02^d
77257	G0IV	0.596	3.00	Mc	0.37^a,d	70016	K1V	0.867	8.15	S	-0.13^a, -0.07^d
14632	G0V	0.606	3.15	Mc	0.33^a, 0.32^d	79190	K1V	0.843	$\leq$ 3.97	FE	...
77801	G0V	0.624	...	FO/S	0.37^d	71681	K1V	0.900	$\leq$ 3.52	FE	...
1499	G0V	0.680	4.18	FO	0.21^d	3765	K2V	0.885	6.71	FO/S/Mc	-0.04^a
67904	G0V	0.697	...	FE	0.27^d	88 972	K2V	0.886	4.82	S	-0.11^a, -0.13^d
10 644	G0.5V	0.603	3.93	Mc	0.52^a, 0.50^d	105 152	K2V	1.028	3.69	FO	-0.33^a
29860	G0.5V	0.611	2.98	S	0.34^a,d	114886	K2V	0.898	$\leq$ 3.18	FO	-0.07^d
48113	G0.5IV	0.624	2.93	FO/S	0.23^a, 0.27^d	12114	K3V	0.918	6.45	S	-0.11^a, -0.04^d
15371	G1V	0.600	$\leq$ 2.64	FE	0.42^c	114 622	K3/K4 V	1.000	2.10	FO/S	-0.29^a
53721	G1V	0.613	2.80	Mc	0.31^a, 0.35^d	78843	K3/K4V	1.059	6.24	S	-0.38^d
24813	G1.5IV	0.613	2.00	Mc	0.31^a,d	73184	K4V	1.110	...	FE	-0.20^d
7918	G1.5V	0.620	2.10	FO/S/Mc	0.30^a	113718	K4V	0.948	6.22	FO	...
52369	G2/G3V	0.629	7.22	S	...	12929	K5	1.170	8.11	FO	0.01^a, -0.07^d
79672	G2Va	0.648	$\leq$ 4.07	Mc	0.31^a, 0.30^d	50125	K5V	1.122	2.85	S	...
27435	G4V	0.639	2.61	S	0.32^d	54651	K5V	1.089	$\leq$ 0.53	S	...
50505	G5	0.686	1.72	S	0.22^d	83591	K5V	1.120	3.70	FO/S	-0.20^d
64924	G5V	0.709	4.09	S	0.16^a, 0.15^d	93871	K5V	1.050	4.07	FO	...
171	G5V	0.660	3.00	Mc	0.30^a	104214	K5V	1.160	4.72	FO/S	-0.22^a
5336	G5V	0.700	8.00	Mc	0.19^a	80644	K6V	1.209	$\leq$ 3.68	FO	-0.25^a, -0.26^d
62523	G7V	0.706	10.60	S	0.42 $^{\rm d}$	104217	K7V	1.360	1.70	FO/S	-0.50^a
2941	G7V	0.717	5.54	S	0.23^a, 0.19^d	54646	K8V	1.345	5.83	S	-0.37^d
58576	G8IV-V	0.757	...	Mc	0.03^a, 0.11^d	60661	M0V	1.451	...	FO	...
14150	G8V	0.715	4.08	S	0.22^d

Notes. ⁽¹⁾ Spectrograph used: Mc: Mc Donald; S: SARG; FO: FOCES; FE: FEROS. ^(a) Duncan et al. (1991). ^(b) Henry et al. (1996). ^(c) Jenkins et al. (2006). ^(d) Wright et al. (2004).

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