Table 5: MORO solutions of the light curve of the eclipsing system 2MASS J0516288+260738.
Parameter a b c d e f g h

q (=M₂/M₁) 0.085 0.094 0.110 0.122 0.156 0.181 0.182 0.184

i $75\fdg5$ $74\fdg3$ $74\fdg0$ $73\fdg9$ $73\fdg5$ $72\fdg4$ $72\fdg9$ $72\fdg3$

T₁/T₂ 1.67 1.72 1.74 1.73 1.77 1.63 1.83 1.88

r₁/r₂^a 1.11 0.89 0.85 0.87 0.85 0.67 0.73 0.64

$\Omega_1$ 5.138 5.350 5.510 5.520 5.598 6.123 6.001 6.220

$\Omega_2$ 1.961 1.943 1.997 2.055 2.182 2.197 2.236 2.198

L₁^b 0.998 0.998 0.999 0.998 0.999 0.993 0.999 0.999

x₁^c 0.60^* 0.60^* 0.50^* 0.50^* 0.60^* 0.60^* 0.488 0.60^*

x₂^c 0.50^* 0.50^* 0.50^* 0.50^* 0.50^* 0.50^* 0.527 0.50^*

l₃^d 0%^* 0%^* 0%^* 0%^* 0%^* 0%^* 1.5% 0%^*

$1\sigma$ deviation 0.00750 0.00750 0.00749 0.00749 0.00749 0.00755 0.00750 0.00749

^a Ratio of mean Roche radii.

^b Relative luminosity L₁/(L₁ + L₂); L₂ is not independently adjusted, but recomputed from r₂ and T₂.

^d Fraction of third light at maximum.

^* Fixed.

**Table 5:** MORO solutions of the light curve of the eclipsing system 2MASS J0516288+260738.
Parameter	a	b	c	d	e	f	g	h
q (=M₂/M₁)	0.085	0.094	0.110	0.122	0.156	0.181	0.182	0.184
i	$75\fdg5$	$74\fdg3$	$74\fdg0$	$73\fdg9$	$73\fdg5$	$72\fdg4$	$72\fdg9$	$72\fdg3$
T₁/T₂	1.67	1.72	1.74	1.73	1.77	1.63	1.83	1.88
r₁/r₂^a	1.11	0.89	0.85	0.87	0.85	0.67	0.73	0.64
$\Omega_1$	5.138	5.350	5.510	5.520	5.598	6.123	6.001	6.220
$\Omega_2$	1.961	1.943	1.997	2.055	2.182	2.197	2.236	2.198
L₁^b	0.998	0.998	0.999	0.998	0.999	0.993	0.999	0.999
x₁^c	0.60^*	0.60^*	0.50^*	0.50^*	0.60^*	0.60^*	0.488	0.60^*
x₂^c	0.50^*	0.50^*	0.50^*	0.50^*	0.50^*	0.50^*	0.527	0.50^*
l₃^d	0%^*	0%^*	0%^*	0%^*	0%^*	0%^*	1.5%	0%^*
$1\sigma$ deviation	0.00750	0.00750	0.00749	0.00749	0.00749	0.00755	0.00750	0.00749

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