“…Many astrophysical plasmas, such as the solar wind, are known for having hot non-thermal tails [13]. Laser-plasma interactions are also known for generating hot [14] or depleted tails [15,16]; the latter had the Weibel instability and its characteristics extensively studied in connection with fusion [17][18][19][20][21]. Non-Maxwellian distributions are rarely considered in the literature when performing kinetic analysis.…”