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Table 1

Stellar parameters measured from the primaries, with the [Fe/H] of the M dwarf secondary inferred from the primary.

Primary Secondary T eff log g ξ t [Fe/H] [Fe/H] T eff
[K] [cm s-2] [km s-1] source source

Gl53.1A Gl53.1B 4705  ±  131 4.33  ±  0.26 0.76  ±  0.25 0.07  ±  0.12 B05
Gl56.3A Gl56.3B 5394  ±  47 0.00  ±  0.10 COR S08CAL
Gl81.1A Gl81.1B 5332  ±  22 3.90  ±  0.03 0.99  ±  0.02 0.08  ±  0.02 S08
Gl100A Gl100C 4804  ±  81 4.82  ±  0.24 1.25  ±  0.24 –0.28  ±  0.03 New
Gl105A Gl105B 4910  ±  65 4.55  ±  0.14 0.77  ±  0.18 –0.19  ±  0.04 New
Gl140.1A Gl140.1B 4671  ±  65 4.31  ±  0.15 0.54  ±  0.31 –0.41  ±  0.04 S08
Gl157A Gl157B 4854  ±  71 4.75  ±  0.19 1.31  ±  0.20 –0.16  ±  0.03 New
Gl173.1A Gl173.1B 4888  ±  72 4.72  ±  0.16 0.97  ±  0.21 –0.34  ±  0.03 New
Gl211 Gl212 5293  ±  109 4.50  ±  0.21 0.79  ±  0.17 0.04  ±  0.11 B05
Gl231.1A Gl231.1B 5951  ±  14 4.40  ±  0.03 1.19  ±  0.01 –0.01  ±  0.01 New
Gl250A Gl250B 4670  ±  80 4.41  ±  0.16 0.70  ±  0.19 –0.15  ±  0.09 B05
Gl297.2A Gl297.2B 6461  ±  14 4.65  ±  0.02 1.74  ±  0.01 0.03  ±  0.05 New
Gl324A Gl324B 5283  ±  59 4.36  ±  0.11 0.87  ±  0.08 0.32  ±  0.07 B05
Gl559A Gl551 5857  ±  24 4.38  ±  0.04 1.19  ±  0.03 0.23  ±  0.02 New
Gl611A Gl611B 5214  ±  44 4.71  ±  0.06 –0.69  ±  0.03 SPO
Gl653 Gl654 4723  ±  89 4.41  ±  0.24 0.52  ±  0.31 –0.62  ±  0.04 S08
Gl666A Gl666B 5274  ±  26 4.47  ±  0.04 0.74  ±  0.05 –0.34  ±  0.02 New
Gl783.2A Gl783.2B 5094  ±  66 4.31  ±  0.13 0.30  ±  0.19 –0.16  ±  0.08 B05
Gl797A Gl797B 5889  ±  32 4.59  ±  0.06 1.01  ±  0.06 –0.07  ±  0.04 B05
GJ3091A GJ3092B 4971  ±  79 4.48  ±  0.15 0.81  ±  0.22 0.02  ±  0.04 S08
GJ3194A GJ3195B 5860  ±  47 0.00  ±  0.10 SOP S08CAL
GJ3627A GJ3628B 5013  ±  47 –0.04  ±  0.10 SOP S08CAL
NLTT34353 NLTT34357 5489  ±  19 4.46  ±  0.03 0.91  ±  0.03 –0.18  ±  0.01 New

References. [B05] Bonfils et al. (2005); [COR] CCF [Fe/H] derived from spectra of the CORALIE Spectrograph; [S08CAL] Teff calibration from Sousa et al. (2008); [S08] Sousa et al. (2008); [New] This paper; [SPO] Valenti & Fischer (2005); [SOP] CCF [Fe/H] taken from spectra of the SOPHIE Spectrograph (Bouchy & The Sophie Team 2006).

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