Table 2.

Families of solutions for the occulted star-spot.

SolutionsFractionx-positiony-positionRadiusΔTΔlog g
of models[|$\rm R_*$|][|$\rm R_*$|][|$\rm R_*$|][K][log10 cm s−2]
Most likely0.560.090 ± 0.0050.42 ± 0.050.116 ± 0.01493 ± 151.16 ± 0.19
Colder spot
Similar position0.180.092 ± 0.0030.41 ± 0.070.090 ± 0.004140 ± 201.8 ± 0.2
Higher position0.140.088 ± 0.0040.53 ± 0.030.125 ± 0.018180 ± 502.1 ± 0.4
Lower position0.120.091 ± 0.0050.24 ± 0.050.14 ± 0.03190 ± 802.2 ± 0.6
SolutionsFractionx-positiony-positionRadiusΔTΔlog g
of models[|$\rm R_*$|][|$\rm R_*$|][|$\rm R_*$|][K][log10 cm s−2]
Most likely0.560.090 ± 0.0050.42 ± 0.050.116 ± 0.01493 ± 151.16 ± 0.19
Colder spot
Similar position0.180.092 ± 0.0030.41 ± 0.070.090 ± 0.004140 ± 201.8 ± 0.2
Higher position0.140.088 ± 0.0040.53 ± 0.030.125 ± 0.018180 ± 502.1 ± 0.4
Lower position0.120.091 ± 0.0050.24 ± 0.050.14 ± 0.03190 ± 802.2 ± 0.6
Table 2.

Families of solutions for the occulted star-spot.

SolutionsFractionx-positiony-positionRadiusΔTΔlog g
of models[|$\rm R_*$|][|$\rm R_*$|][|$\rm R_*$|][K][log10 cm s−2]
Most likely0.560.090 ± 0.0050.42 ± 0.050.116 ± 0.01493 ± 151.16 ± 0.19
Colder spot
Similar position0.180.092 ± 0.0030.41 ± 0.070.090 ± 0.004140 ± 201.8 ± 0.2
Higher position0.140.088 ± 0.0040.53 ± 0.030.125 ± 0.018180 ± 502.1 ± 0.4
Lower position0.120.091 ± 0.0050.24 ± 0.050.14 ± 0.03190 ± 802.2 ± 0.6
SolutionsFractionx-positiony-positionRadiusΔTΔlog g
of models[|$\rm R_*$|][|$\rm R_*$|][|$\rm R_*$|][K][log10 cm s−2]
Most likely0.560.090 ± 0.0050.42 ± 0.050.116 ± 0.01493 ± 151.16 ± 0.19
Colder spot
Similar position0.180.092 ± 0.0030.41 ± 0.070.090 ± 0.004140 ± 201.8 ± 0.2
Higher position0.140.088 ± 0.0040.53 ± 0.030.125 ± 0.018180 ± 502.1 ± 0.4
Lower position0.120.091 ± 0.0050.24 ± 0.050.14 ± 0.03190 ± 802.2 ± 0.6
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