  We present an analysis of survey observations of the trailing L5 Jupiter
Trojan swarm using the wide-field Hyper Suprime-Cam CCD camera on the 8.2 m
Subaru Telescope. We detected 189 L5 Trojans from our survey that covered about
15 deg^2 of sky with a detection limit of m_r = 24.1 mag, and selected an
unbiased sample consisting of 87 objects with absolute magnitude 14 < H_r < 17
corresponding to diameter 2 km < D < 10 km for analysis of size distribution.
We fit their differential magnitude distribution to a single-slope power-law
with an index \alpha = 0.37 +- 0.01, which corresponds to a cumulative size
distribution with an index of b = 1.85 +- 0.05. Combining our results with data
for known asteroids, we obtained the size distribution of L5 Jupiter Trojans
over the entire size range for 9 < H_V < 17, and found that the size
distributions of the L4 and L5 swarms agree well with each other for a wide
range of sizes. This is consistent with the scenario that asteroids in the two
swarms originated from the same primordial population. Based on the above
results, the ratio of the total number of asteroids with D > 2 km in the two
swarms is estimated to be N_L4/N_L5=1.40 +- 0.15, and the total number of L_5
Jupiter Trojans with D > 1 km is estimated to be 1.1 x 10^5 by extrapolating
the obtained distribution.
