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Table 5

Main properties of the stars presented in Fig. 10.

Star Mass Radius [Fe/H] T eff Magnetic activity P orb vsini Ref.
name [M] [R] [dex] [K] (LX/Lbol) [day] [km s-1]

OGLE-TR 123 Bb 0.085 ± 0.011 0.133 ± 0.009 1.8039 1
SDSS 0857+03 Bc 0.090 ± 0.010 0.110 ± 0.004 0.06528 2
J1219-39 Bb 0.091 ± 0.002 − 0.21 6.7600 3
OGLE-TR 122 Bb 0.092 ± 0.009 + 0.15 7.2687 4
C4780 Bb 0.096 ± 0.011 + 0.20 20.6841 this work
NN Ser Bc 0.111 ± 0.004 0.149 ± 0.002 0.13008 5
GK Vir Bc 0.116 ± 0.003 0.155 ± 0.003 0.34433 6
OGLE-TR 106 Bb 0.116 ± 0.021 0.181 ± 0.013 2.5359 3.59 ± 0.26 7
GJ 551a 0.118 ± 0.012 0.141 ± 0.007 + 0.19 3054 2.73E− 4 ± 6.5E− 5 n/a 8, 9, 10, 11
HAT-TR-205-013 Bb 0.124 ± 0.010 0.1670 ± 0.0060 − 0.20 2.2307 12
SDSS 0138-00 Bc 0.132 ± 0.003 0.165 ± 0.001 0.07276 13
KIC 1571511 Bb + 0.37 14.0225 14
GJ 699a 0.146 ± 0.015 0.1869 ± 0.0012 − 0.39 3222 2.88E− 6 ± 3.3E− 7 n/a <2.8 8, 11, 15, 16
SDSS 1210+33 Bc 0.158 ± 0.006 0.200 ± 0.004 − 2.0 0.12449 17
SDSS 1548+40 Bc 0.173 ± 0.027 0.181 ± 0.015 0.185 18
RR Cae Bc 0.1825 ± 0.0131 0.2090 ± 0.0143 3100 0.304 19
2MASS 0446+19 Bb 0.190 ± 0.020 0.210 ± 0.010 2900 0.61879 20

Notes.

(a)

A single star for which the mass was inferred from a mass-luminosity relation.

(b)

An sb1 EB for which the mass estimation is model dependent.

(c)

An eclipsing white dwarf + M-dwarf binary for which the radius listed in the table is the volume-averaged one.

Reference. (1) Pont et al. (2006); (2) Parsons et al. (2012b); (3) Triaud et al. (2013); (4) Pont et al. (2005b); (5) Parsons et al. (2010); (6) Parsons et al. (2012c); (7) Pont et al. (2005a); (8) Boyajian et al. (2012); (9) Demory et al. (2009); (10) Edvardsson et al. (1993); (11) López-Morales (2007); (12) Beatty et al. (2007); (13) Parsons et al. (2012a); (14) Ofir et al. (2012); (15) Lane et al. (2001); (16) Rojas-Ayala et al. (2012); (17) Pyrzas et al. (2012); (18) Pyrzas et al. (2009); (19) Maxted et al. (2007); (20) Hebb et al. (2006).

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