Table 5: Photometric solutions of V861 Herculis, based on 2003 LC. For details see Sect. 4.2.
Parameter Value Error

L₁ / (L₁ +L₂ )

V 0.3736 $\pm$ 0.0033

R 0.3610 $\pm$ 0.0031

I 0.3519 $\pm$ 0.0028

x₁ = x₂

bolometric: 0.520

V 0.644

R 0.556

I 0.470

q = M₂ / M₁ 2.460 $\pm$ 0.017

i 66.17 $\pm$ 0.23

$\Phi_{{\rm sh}}$ -0.0306 $\pm$ 0.0004

A₁ = A₂ 0.50

g₁ = g₂ 0.32

$\Omega_1 = \Omega_2$ 5.8414 $\pm$ 0.0228

T₂ 5332K $\pm 220K$

$r_1{\rm (pole)}$ 0.2876 $\pm 0.0022$

$r_1{\rm (side)}$ 0.3004 $\pm 0.0027$

$r_1{\rm (back)}$ 0.3357 $\pm 0.0046$

$r_2{\rm (pole)}$ 0.4351 $\pm 0.0018$

$r_2{\rm (side)}$ 0.4650 $\pm 0.0024$

$r_2{\rm (back)}$ 0.4933 $\pm 0.0031$

$\Sigma w (l_{{\rm obs}} - l_{{\rm comp}})^2$ $2.22 \times 10^{-3}$

**Table 5:** Photometric solutions of V861 Herculis, based on 2003 LC. For details see Sect. 4.2.
Parameter	Value	Error
L₁ / (L₁ +L₂ )
V	0.3736	$\pm$ 0.0033
R	0.3610	$\pm$ 0.0031
I	0.3519	$\pm$ 0.0028
x₁ = x₂
bolometric:	0.520
V	0.644
R	0.556
I	0.470
q = M₂ / M₁	2.460	$\pm$ 0.017
i	66.17	$\pm$ 0.23
$\Phi_{{\rm sh}}$	-0.0306	$\pm$ 0.0004
A₁ = A₂	0.50
g₁ = g₂	0.32
$\Omega_1 = \Omega_2$	5.8414	$\pm$ 0.0228
T₂	5332K	$\pm 220K$
$r_1{\rm (pole)}$	0.2876	$\pm 0.0022$
$r_1{\rm (side)}$	0.3004	$\pm 0.0027$
$r_1{\rm (back)}$	0.3357	$\pm 0.0046$
$r_2{\rm (pole)}$	0.4351	$\pm 0.0018$
$r_2{\rm (side)}$	0.4650	$\pm 0.0024$
$r_2{\rm (back)}$	0.4933	$\pm 0.0031$
$\Sigma w (l_{{\rm obs}} - l_{{\rm comp}})^2$	$2.22 \times 10^{-3}$

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