Table 1.
Data sets in the first H.E.S.S. public test data release (Abdalla et al. 2018c).
| Designation | Type | Extension | # Runs | Observation time | Zenith angle | Publications |
|---|---|---|---|---|---|---|
| (h) | (deg) | |||||
| Crab nebula | PWN | Point-like | 4 | 1.9 | 45.4–48.6 | (1,2) |
| PKS 2155−304 (flare) | AGN | Point-like | 15 | 7.0 | 7.2–50.4 | (3,4) |
| PKS 2155−304 (steady) | AGN | Point-like | 6 | 2.8 | 22.8–36.8 | (5,6,7) |
| MSH 15−52 | PWN | Extended | 20 | 9.1 | 36.1–40.2 | (8) |
| RX J1713.7−3946 | SNR | Extended | 15 | 7.0 | 16.7–26.3 | (9,10,11) |
| Off runs | – | – | 45 | 20.7 | 2.5–52.7 | – |
Notes. “Type” refers to the source type; PWN = pulsar wind nebula; AGN = active galactic nucleus; SNR = supernova remnant. “Extension” specifies whether or not the source can be spatially resolved using this data set. “Publications” lists (selected) H.E.S.S. publications about the sources (usually based on larger data sets). The data sets “PKS 2155−304 (flare)” and “Off runs” are not used in this paper.
References. (1) Aharonian et al. (2006a); (2) Holler et al. (2015); (3) Aharonian et al. (2007); (4) Aharonian et al. (2009); (5) Aharonian et al. (2005a); (6) Abramowski et al. (2010); (7) Abdalla et al. (2017); (8) Aharonian et al. (2005b); (9) Aharonian et al. (2004); (10) Aharonian et al. (2006b); (11) Abdalla et al. (2018d).
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