Table 3: Spots configuration for IM Peg. The stellar parameters used in the solution are: unspotted effective temperature, $T_{\rm max}$ = 4666 K; limb-darkening coefficients at V and at 6200 Å, $\mu _{\rm V}$ = 0.80, $\mu _{6200}$ = 0.68; inclination, i = 60 $^{\circ }$ .
Model Radius Lon. Lat. $\frac{T_{\rm sp}}{T_{\rm ph}}$ $A_{\rm rel}$

Planck 27 $\hbox{$.\!\!^\circ$ }$ 2 123 $\hbox{$^\circ$ }$ 138 $\hbox{$^\circ$ }$ 0.873 $\pm$ 0.050 0.093 $\pm$ 0.025

" " 21 $\hbox{$.\!\!^\circ$ }$ 8 223 $\hbox{$^\circ$ }$ 149 $\hbox{$^\circ$ }$ 0.873 $\pm$ 0.050

Kurucz 28 $\hbox{$.\!\!^\circ$ }$ 5 123 $\hbox{$^\circ$ }$ 138 $\hbox{$^\circ$ }$ 0.904 $\pm$ 0.027 0.106 $\pm$ 0.020

" " 23 $\hbox{$.\!\!^\circ$ }$ 4 223 $\hbox{$^\circ$ }$ 149 $\hbox{$^\circ$ }$ 0.904 $\pm$ 0.027

NextG 30 $\hbox{$.\!\!^\circ$ }$ 0 123 $\hbox{$^\circ$ }$ 138 $\hbox{$^\circ$ }$ 0.915 $\pm$ 0.030 0.115 $\pm$ 0.030

" " 23 $\hbox{$.\!\!^\circ$ }$ 9 223 $\hbox{$^\circ$ }$ 149 $\hbox{$^\circ$ }$ 0.915 $\pm$ 0.030

**Table 3:** Spots configuration for IM Peg. The stellar parameters used in the solution are: unspotted effective temperature, $T_{\rm max}$ = 4666 K; limb-darkening coefficients at V and at 6200 Å, $\mu _{\rm V}$ = 0.80, $\mu _{6200}$ = 0.68; inclination, i = 60 $^{\circ }$ .
Model	Radius	Lon.	Lat.	$\frac{T_{\rm sp}}{T_{\rm ph}}$	$A_{\rm rel}$
Planck	27 $\hbox{$.\!\!^\circ$ }$ 2	123 $\hbox{$^\circ$ }$	138 $\hbox{$^\circ$ }$	0.873 $\pm$ 0.050	0.093 $\pm$ 0.025
" "	21 $\hbox{$.\!\!^\circ$ }$ 8	223 $\hbox{$^\circ$ }$	149 $\hbox{$^\circ$ }$	0.873 $\pm$ 0.050
Kurucz	28 $\hbox{$.\!\!^\circ$ }$ 5	123 $\hbox{$^\circ$ }$	138 $\hbox{$^\circ$ }$	0.904 $\pm$ 0.027	0.106 $\pm$ 0.020
" "	23 $\hbox{$.\!\!^\circ$ }$ 4	223 $\hbox{$^\circ$ }$	149 $\hbox{$^\circ$ }$	0.904 $\pm$ 0.027
NextG	30 $\hbox{$.\!\!^\circ$ }$ 0	123 $\hbox{$^\circ$ }$	138 $\hbox{$^\circ$ }$	0.915 $\pm$ 0.030	0.115 $\pm$ 0.030
" "	23 $\hbox{$.\!\!^\circ$ }$ 9	223 $\hbox{$^\circ$ }$	149 $\hbox{$^\circ$ }$	0.915 $\pm$ 0.030

Source LaTeX | All tables | In the text

	1 Introduction
	2 Targets selection and observations
	3 Data analysis
	4 The spot model
	5 Results
	6 Discussion
	7 Conclusion
	References
	Online Material
	Appendix A: The hemisphere-averaged temperature and luminosity