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Table 1.
Sample of stars for which we consider asymmetry indicators and FWHM of the CCF.
Name | Teff[K] | log g [cm s−2] | [Fe/H] | υ sin i km s−1] |
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NRV | Δt [days] | Reference |
---|---|---|---|---|---|---|---|---|
HD 11506 | 6204 ± 50 | 4.44 | +0.36 | 5.0 ± 0.5 | −5.028 ± 0.017 | 37 | 678.32 | Santos et al. (2013) |
HD 13931 | 5830 ± 45 | 4.30 | +0.03 | 2.0 ± 0.5 | −5.043 ± 0.012 | 67 | 708.34 | Valenti & Fischer (2005) |
HD 23596 | 6110 ± 45 | 4.25 | +0.31 | 4.2 ± 0.5 | −5.039 ± 0.020 | 26 | 737.36 | Santos et al. (2013) |
HD 72659 | 5920 ± 45 | 4.24 | 0.0 | 2.2 ± 0.5 | −4.998 ± 0.019 | 23 | 737.35 | Valenti & Fischer (2005) |
HD 73534 | 5040 ± 65 | 3.78 | +0.23 | 0.5 ± 0.5 | −5.242 ± 0.028 | 31 | 737.38 | Valenti et al. (2009) |
HD 75898 | 6140 ± 50 | 4.31 | +0.30 | 4.5 ± 0.5 | −5.024 ± 0.032 | 34 | 737.47 | Santos et al. (2013) |
HD 89307 | 5900 ± 45 | 4.34 | −0.16 | 3.2 ± 0.5 | −4.970 ± 0.008 | 19 | 737.46 | Valenti & Fischer (2005) |
HD 99109 | 5270 ± 45 | 4.44 | +0.31 | 1.9 ± 0.5 | −5.139 ± 0.037 | 27 | 754.38 | Valenti & Fischer (2005) |
HD 106252 | 5870 ± 45 | 4.36 | −0.08 | 1.9 ± 0.5 | −5.003 ± 0.008 | 44 | 754.42 | Valenti & Fischer (2005) |
HD 108874 | 5585 ± 20 | 4.39 | +0.19 | 1.4 ± 0.3 | −5.050 ± 0.027 | 55 | 754.46 | Benatti et al. (2017) |
HD 155358 | 5900 ± 100 | 4.16 | −0.51 | ~2 | −4.965 ± 0.009 | 44 | 753.54 | Robertson et al. (2012) |
HD 188015 | 5745 ± 45 | 4.44 | +0.29 | ≤0.5 | −4.988 ± 0.027 | 22 | 737.76 | Valenti & Fischer (2005) |
HD 190228 | 5350 ± 45 | 3.98 | −0.18 | 1.9 ± 0.5 | −5.125 ± 0.012 | 44 | 553.42 | Valenti & Fischer (2005) |
HD 220773 | 5940 ± 100 | 4.24 | +0.09 | ~3 | −5.088 ± 0.010 | 46 | 653.30 | Robertson et al. (2012) |
XO-2S | 5395 ± 60 | 4.43 | +0.39 | 1.7 ± 0.4 | −5.053 ± 0.075 | 44 | 737.39 | Damasso et al. (2015b) |
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