Variation of the stellar color in high-magnification and caustic-crossing microlensing events

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Table 4

Parameters of the light curves shown in Fig. 6.

	log₁₀ [u₀]	t_E	log₁₀ [ρ_*]	m_base, I	T_eff	a	T_p	i	b_I	q	d	ξ	Δχ²
		(days)		(mag)	(K)	(au)	(K)	(deg)				(deg)
6a	–2.35	8.7	–2.20	18.7	5846	0.01	2918	70	0.86	–	–	202	747
6b	–3.10	17.7	–2.55	18.1	5527	0.02	2175	43	1.0	–	–	76	876
6c	–2.02	82.4	–3.27	17.3	7480	0.02	3736	38	1.0	0.01	1.09	110	1875
6d	–0.63	31.9	–2.80	19.3	6055	0.01	2549	53	0.99	0.44	1.21	100	6

Notes. Here, a is the radius of the planet orbit,T_p is the planet temperature, and i is the inclination angle of the planetary orbit with respect to the sky plane.

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