# ---------------------------------------------------------------------------------------------------------------------------------------------------------------------------
# estimation of a possible Proxima Centauri event at 0.049 AU (TOA spectrum of Proxima Centauri b)
#
# based on Struminsky, Sadovski & Belov (2017) 
# problem: spectrum not known
# assumption: form of the Feb 1956 event
#
# E [MeV], dI/dE [protons/(cm^2 s sr MeV)]
#
#     energy    dI/dE upper limit  dI/dE lower limit
# ---------------------------------------------------------------------------------------------------------------------------------------------------------------------------

      456.757       28485.966       11394.387
      524.913       19609.077       7843.6310
      603.240       13278.179       5311.2715
      693.255       8821.2996       3528.5198
      796.702       5732.0778       2292.8311
      915.584       3630.2650       1452.1060
      1052.21       2231.6803       892.67213
      1209.22       1319.5733       527.82933
      1389.65       717.74339       287.09735
      1597.02       385.74586       154.29835
      1835.32       204.76287       81.905149
      2109.18       107.32338       42.929352
      2423.91       55.534646       22.213858
      2785.61       28.369834       11.347934
      3201.27       14.309516       5.7238063
      3678.96       7.1282522       2.8513009
      4227.93       3.5082337       1.4032935
      4858.81       1.7066823      0.68267291