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Table 1

Parameters used in modeling.

Symbol Quantity
t Time
   
tk, Time of lunar, planetary eclipse
   
T Observation duration
   
L Distance to the observer on Earth
   
S Star radius
   
α Binary inclination angle, w.r.t. orbital plane
   
s1, s2 Planet, moon radius
   
a1, a2 Planet, moon albedo
   
R1, R2 Planet, moon position vector
   
Binary c.m.-position vector
   
Reduced position vector
   
Arbitrary planet surface vector

θ Azimuth angle
   
z Vertical coordinate w.r.t. planet center
   
l Vertical displacement of shadow center
   
v Shadow velocity
   
τ(l) Eclipse duration
   
ϒ(l) Eclipse magnitude

ν Continuous frequency variable
   
ω Barycenter angular frequency, mean motion
   
ϑ = ωt Barycenter phase angle, mean anomaly
   
Ω Lunar orbital frequency
   
φ = Ωt Lunar phase

Observation direction
θo Observation inclination, polar angle
   
ϕo Phase at inferior conjunction, azimuth
   
I(t) Variable star luminosity
   
IT(ν) Fourier transform of star luminosity
   
I0 Average star luminosity
   
F(t) Observed reflection signal
   
FT(ν) Fourier transform of reflection signal
   
f(t) = f(ϑ, φ) Total reflected light curve
   
Fourier coefficient of light curve
   
g(ϑ) Time-integrated dip for lunar eclipse
   
gn Fourier coefficient of g
   
h(ϑ) Single-planet phase light curve
   
hn Fourier coefficient of h

i, j, k, Basis vectors for orbital plane
, , Basis vectors for lunar plane
N = ωT∕2π Number of orbits
k Eclipse index number
n, m Integer indices

Notes. Symbol and significance of the physical quantities used.

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