# Inferred constraints on the fraction of dark matter in the form of
# primordial black holes (PBHs) in the mass range 10^15--10^17 g from
# Mittal et al. (2021) [https://arxiv.org/abs/2107.02190]. This is for case II, in which X-ray heating is
# present. See figure 6 (red line) from the paper for a graphical
# representation. 
5.000000000000000358e-19 1.867518875340305291e-10
1.000000000000000072e-18 1.598424030286459998e-09
1.500000000000000107e-18 8.631315666101696167e-09
2.000000000000000143e-18 2.711777169001669106e-08
2.500000000000000179e-18 7.804246890122419145e-08
3.000000000000000215e-18 2.016823996474341435e-07
3.499999999999999865e-18 3.729812499115140448e-07
4.000000000000000286e-18 6.537007752296956841e-07
4.499999999999999937e-18 1.784604566757970476e-06
5.000000000000000358e-18 2.828883092443404599e-06
1.000000000000000072e-17 2.589637646878521703e-05
1.500000000000000030e-17 9.095006211413122295e-05
2.000000000000000143e-17 2.367200260800981474e-04
2.500000000000000256e-17 5.510411096603854255e-04
3.000000000000000061e-17 1.243526372074526794e-03
3.500000000000000173e-17 1.966962136744183302e-03
4.000000000000000286e-17 3.074956667167447807e-03
4.500000000000000399e-17 5.307634397692228417e-03
5.000000000000000512e-17 1.071119682946137554e-02
1.000000000000000102e-16 3.567524793115885440e-01
1.499999999999999969e-16 1.201212934563789192e+00
