#Below 1 M_sun, use LIGO's subsolar mass search: Fig. 2 in https://arxiv.org/abs/1904.08976
#Above 1 M_sun, use the bound from Fig. 11 of https://arxiv.org/abs/1805.09034
0.19780160103282196 0.15806044292293459
0.2184327602356321 0.13850434330244568
0.250359303278564 0.11583996564341904
0.2941586932679772 0.09319314885267727
0.3329980203821802 0.07978111196368196
0.38166963731122594 0.0672462071226684
0.4267382578583718 0.05756876600850738
0.4830827656645964 0.04890241851383388
0.5401265326563364 0.042191226047689975
0.6668949835553095 0.032145992037596584
0.8032438272286146 0.025265523425753743
1.0041424613860337 0.01880667049454468
1.000000000000000000e+01 4.128239741159375753e-03
2.000000000000000000e+01 2.359996338738551587e-03
4.000000000000000000e+01 1.366662670283457035e-03
1.000000000000000000e+02 7.743629278679708353e-04
2.000000000000000000e+02 1.740532545819348850e-03
3.000000000000000000e+02 4.412168318725404742e-03
