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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