Auxiliary information for "LMC N132D: A mature supernova remnant with a power-law gamma-ray spectrum extending beyond 8 TeV" (published in Astronomy & Astrophysics in 2021)

Link to the paper:


The fits file corresponding to the H.E.S.S. excess map shown in Figure 1 of the paper


The fits file corresponding to the smoothed Fermi-LAT count map shown in Figure 2 of the paper


The H.E.S.S. and Fermi-LAT spectral points shown in Figures 3 and 4 of the paper

[1/ (cm2 s TeV)]
Flux Error_low
[1/ (cm2 s TeV)]
Flux Error_high
[1/ (cm2 s TeV)]

1.73e-3 4.25e-08 3.54e-08 3.54e-08
5.20e-3 6.30e-09 3.28e-09 3.28e-09
15.6e-3 1.41e-09 5.37e-10 5.37e-10
83.0e-3 4.12e-11 2.68e-11 2.68e-11
1.47 6.47e-14 2.67e-14 2.43e-14
2.35 1.27e-14 5.24e-15 4.97e-15
4.97 5.32e-15 1.46e-15 1.37e-15
15.17 1.87e-16 1.09e-16 9.89e-17

The 2-sigma and 3-sigma significance contours of the best-fit position as derived using the ON counts map, background map (Alpha map times OFF map), and exposure map, and the H.E.S.S. point spread function shown in Figure 6 of the paper