# Sensitivity (projected 95% confidence limit) on photon-ALP coupling
# Derived from a potential core-collapse supernova of 10 solar mass progenitor
# in the galactic center, using the GMF model of Jansson & Farrar 2012
# ALP mass (eV) vs photon-ALP coupling (GeV^-1)
# Source: Meyer et al., arXiv:1609.02350
# 
1.00000e-10 1.87607e-13
1.49250e-10 1.87658e-13
2.22754e-10 1.87911e-13
3.32460e-10 1.89146e-13
4.96195e-10 1.94714e-13
7.40568e-10 2.13851e-13
1.10530e-09 2.54995e-13
1.64965e-09 3.16211e-13
2.46209e-09 4.28341e-13
3.67466e-09 6.86299e-13
5.48442e-09 1.02503e-12
8.18547e-09 1.53531e-12
1.22168e-08 2.37767e-12
1.82335e-08 3.49932e-12
2.72134e-08 5.13688e-12
4.06159e-08 7.65686e-12
6.06190e-08 1.11371e-11
9.04736e-08 1.62390e-11
1.35031e-07 2.44692e-11
2.01534e-07 3.90711e-11
3.00788e-07 5.75699e-11
4.48925e-07 8.24865e-11
6.70019e-07 1.00000e-10
1.00000e-06 1.00000e-10