Table 5
Analysis datasets used in this study.
| Target | Type | Extension | Runs | Observation time (h) | Zenith angle (°) |  |
|---|---|---|---|---|---|---|
| Reticulum II(d) | dSph | None | 16 | 7.0 | 34°–50° | 0.24 |
| Tucana II(d) | dSph | None | 14 | 6.2 | 35°–38° | 0.28 |
| Sculptor Dwarf Galaxy(e) | Sph | None | 22 | 10.0 | 11°–19° | 0.22 |
| Crab Nebula(b) | PWN | Point-like | 4 | 1.9 | 45°–49° | 0.35 |
| PKS 2155–304 (steady) (a,b) | AGN | Point-like | 6 | 2.8 | 23°–37° | 0.89 |
| MSH 15–52(b) | PWN | Extended | 15 | 6.8 | 36°–39° | 0.22 |
| RXJ1713.7–3946(b) | SNR | Extended | 15 | 7.0 | 16°–26° | 0.58 |
| RXJ1713.7–3946 (large)(c) | SNR | Extended | 153 | 51.0 | 17°–59° | 0.57 |
Notes. The source extension noted in this table does not necessarily match the best description found in the literature, but rather the description used in Mohrmann et al. (2019) and in the present analysis.(a)Observations of PKS 2155–304 taken outside of periods when the source undergoes γ-ray outbursts. (b)This dataset is part of the first public data release of the H.E.S.S. collaboration (H.E.S.S. Collaboration 2018). (c)More information on this dataset can be found in H.E.S.S. Collaboration (2018). (d)More information on this dataset can be found in Abdallah et al. (2020). (e)More information on this dataset can be found in Abramowski et al. (2014a).
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