Auxiliary information for "Evidence for gamma-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations" (published in Astronomy & Astrophysics in 2022)

Link to the paper: https://www.aanda.org/articles/aa/abs/2022/06/aa43096-22/aa43096-22.html

DOI: https://doi.org/10.1051/0004-6361/202243096

The fits files corresponding to the H.E.S.S. significance map shown in Figure 1a and to the Fermi-LAT test-statistic map shown in Figure 1b of the paper

H.E.S.S. significance map [FITS]

Fermi-LAT test-statistic map [FITS]

The H.E.S.S. spectral points shown in Figures 2a and 3 of the paper [TXT]

Frequency
[Hz] E^2 dN/dE
[erg/ (cm² s)] Uncertainty E² dN/dE
[erg/ (cm² s)]

1.0366e26 2.1754e-13 6.6517e-14

2.5655e26 1.4131e-13 3.9048e-14

7.1766e26 7.5649e-14 3.9913e-14

2.0347e27 1.2820e-13 5.2302e-14