Metallicity of solar-type stars with debris discs and planets

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Table 1

The SWD and SWOD samples.

HIP	HD	SpType	V	Distance	log (Age)	[Fe/H]	Ref.
				(pc)	(yr)	(dex)

Stars with known debris discs
171	224930	G3V	5.80	12.17	9.60	–0.72^a	13
490	105	G0V	7.51	39.39	8.34	–0.03^b	2
544	166	K0V	6.07	13.67	9.16	0.15^a	5
682	377	G2V	7.59	39.08	8.34	0.12^b	6
1481	1466	F8/G0	7.46	41.55	8.34	–0.22^c	7
1598	1562	G0	6.97	24.80	9.79	–0.32^a	13
1599	1581	F9V	4.23	8.59	9.58	–0.29^a	9
2843	3296	F5	6.72	45.05		0.02^c	9

Notes. Only the first eight lines of the SWD sample and the references are presented here; the full version of the table is available at the CDS.

^(a)

This work;

^(b)

Valenti & Fischer (2005);

^(c)

Nordström et al. (2004);

(b) and (c) values are set into our metallicity scale as described in Sect. 3.2.

References. (1) Habing et al. (2001); (2) Spangler et al. (2001); (3) Chen et al. (2005); (4) Beichman et al. (2006); (5) Bryden et al. (2006); (6) Moór et al. (2006); (7) Smith et al. (2006); (8) Rhee et al. (2007); (9) Trilling et al. (2008); (10) Kóspál et al. (2009); (11) Plavchan et al. (2009); (12) Tanner et al. (2009); (13) Koerner et al. (2010); (14) Moór et al. (2011).

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