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Table H.1.

Spectral points obtained from the 3D analysis with gammapy (Sect. 2.1.2).

Spectral points of HESS J1702-420A

e_ref e_min e_max sqrt_ts counts dnde dnde_ul dnde_errp dnde_errn
[TeV] [TeV] [TeV] [TeV−1 cm−2 s−1] [TeV−1 cm−2 s−1] [TeV−1 cm−2 s−1] [TeV−1 cm−2 s−1]
3.19 2.08 4.90 3.36 40973 4.08e−14 8.35e−14 1.33e−14 1.27e−14
8.66 4.90 15.32 3.15 15812 4.42e−15 7.01e−15 1.59e−15 1.50e−15
23.50 15.32 36.04 5.29 3363 1.42e−15 2.00e−15 3.64e−16 3.33e−16
47.94 36.04 63.76 4.83 835 4.73e−16 1.02e−15 1.52e−16 1.33e−16
84.80 63.76 112.78 4.00 454 1.89e−16 4.91e−16 7.76e−17 6.54e−17
130.07 112.78 150.00 0.00 145 1.20e−23 2.21e−16 2.48e−17 1.20e−23

Spectral points of HESS J1702-420B

e_ref e_min e_max sqrt_ts counts dnde dnde_ul dnde_errp dnde_errn
[TeV] [TeV] [TeV] [TeV−1 cm−2 s−1] [TeV−1 cm−2 s−1] [TeV−1 cm−2 s−1] [TeV−1 cm−2 s−1]

2.77 2.08 3.68 18.62 31603 5.86e−13 7.16e−13 3.62e−14 3.58e−14
4.25 3.68 4.90 12.13 9370 1.98e−13 2.36e−13 1.92e−14 1.87e−14
6.51 4.90 8.66 11.01 10687 4.98e−14 5.78e−14 5.18e−15 5.06e−15
11.52 8.66 15.32 6.60 5125 9.82e−15 1.14e−14 1.68e−15 1.64e−15
23.50 15.32 36.04 6.89 3363 2.40e−15 3.44e−15 4.02e−16 3.89e−16
63.76 36.04 112.78 3.20 1289 1.78e−16 3.74e−16 6.31e−17 5.94e−17
130.07 112.78 150.00 0.49 145 2.48e−17 3.34e−16 5.62e−17 2.48e−17

Notes. The points were obtained by rescaling the amplitude of the reference spectral model within each energy bin, re-optimizing at the same time all free nuisance parameters of the model. The column names follow the convensions defined by the open-source “data formats for gamma-ray astronomy” community (https://gamma-astro-data-formats.readthedocs.io/en/latest/).

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