To observe cosmic-origin antiparticles, it is crucial to mitigate the astrophysical background.
One approach involved searching for background-free antideuterons/antihelium; however, no viable candidates were identified.
Consequently, we extended our antiproton observations to the lower-energy region below 0.2 GeV, where the contribution from secondary particles is minimized, and explored the potential signatures of dark matter in the $4.7 \times 10^{9}$ cosmic ray events recorded by BESS-Polar II during the solar activity minimum in 2007.
We modified the trigger conditions to utilize the middle time-of-flight (TOF), effectively reducing the amount of passing material by half.
We will report the details of the analysis and the lower-energy antiproton flux measured by BESS-Polar II.