Table 3
Table of 31 firmly-identified objects among the HGPS sources.
| Source name | Identified object | Class | Evidence | Reference |
|---|---|---|---|---|
| HESS J1018−589 A | 1FGL J1018.6−5856 | Binary | Variability | H.E.S.S. Collaboration (2015c) |
| HESS J1302−638 | PSR B1259−63 | Binary | Variability | Aharonian et al. (2005c) |
| HESS J1826−148 | LS 5039 | Binary | Variability | Aharonian et al. (2006c) |
| HESS J0852−463 | Vela Junior | SNR | Morphology | Aharonian et al. (2005e) |
| HESS J1442−624 | RCW 86 | SNR | Morphology | H.E.S.S. Collaboration (2018i) |
| HESS J1534−571 | G323.7−1.0 | SNR | Morphology | H.E.S.S. Collaboration (2018j) |
| HESS J1713−397 | RX J1713.7−3946 | SNR | Morphology | Aharonian et al. (2004b) |
| HESS J1718−374 | G349.7+0.2 | SNR | Position | H.E.S.S. Collaboration (2015a) |
| HESS J1731−347 | G353.6−0.7 | SNR | Morphology | H.E.S.S. Collaboration (2011a) |
| HESS J1801−233 | W 28 | SNR | Position | Aharonian et al. (2008d) |
| HESS J1911+090 | W 49B | SNR | Position | H.E.S.S. Collaboration (2018d) |
| HESS J0835−455 | Vela X | PWN | Morphology | Aharonian et al. (2006d) |
| HESS J1303−631 | G304.10−0.24 | PWN | ED Morph. | H.E.S.S. Collaboration (2012) |
| HESS J1356−645 | G309.92−2.51 | PWN | Position | H.E.S.S. Collaboration (2011b) |
| HESS J1418−609 | G313.32+0.13 | PWN | Position | Aharonian et al. (2006e) |
| HESS J1420−607 | G313.54+0.23 | PWN | Position | Aharonian et al. (2006e) |
| HESS J1514−591 | MSH 15−52 | PWN | Morphology | Aharonian et al. (2005d) |
| HESS J1554−550 | G327.15−1.04 | PWN | Morphology | Sect. 5.6.5 |
| HESS J1747−281 | G0.87+0.08 | PWN | Morphology | Aharonian et al. (2005b) |
| HESS J1818−154 | G15.4+0.1 | PWN | Morphology | H.E.S.S. Collaboration (2014b) |
| HESS J1825−137 | G18.00−0.69 | PWN | ED Morph. | Aharonian et al. (2006f) |
| HESS J1837−069 | G25.24−0.19 | PWN | Morphology | Marandon et al. (2008) |
| HESS J1849−000 | G32.64+0.53 | PWN | Position | Sect. 5.6.15 |
| HESS J1119−614 | G292.2−0.5 | Composite | Position | Sect. 5.6.1 |
| HESS J1640−465 | G338.3−0.0 | Composite | Position | Abramowski et al. (2014b), Gotthelf et al. (2014) |
| HESS J1714−385 | CTB 37A | Composite | Position | Aharonian et al. (2008b) |
| HESS J1813−178 | G12.8−0.0 | Composite | Position | Funk et al. (2007), Gotthelf & Halpern (2009) |
| HESS J1833−105 | G21.5−0.9 | Composite | Position | Sect. 5.6.10 |
| HESS J1834−087 | W 41 | Composite | Morphology | H.E.S.S. Collaboration (2015d) |
| HESS J1846−029 | G29.7−0.3 | Composite | Position | Sect. 5.6.13 |
| HESS J1930+188 | G54.1+0.3 | Composite | Position | Acciari et al. (2010), Sect. 5.4 |
Notes. The object classes are γ-ray binary, shell-type supernova remnant (SNR), pulsar wind nebula (PWN), and composite SNR (in cases where it is not possible to distinguish between the shell and interior nebula). The evidence used to identify the VHE γ-ray emission include position, morphology, variability, and energy-dependent morphology (ED Morph.).
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