Table 1.
Supernova remnants already detected at energies higher than 4 and 10 GeV and confirmed by the present analysis.
| SNR | RANGE | TYPE | D | LX | Scls4 | Scls10 | Δ | MST N/M | MST N/M | Notes |
|---|---|---|---|---|---|---|---|---|---|---|
| (GeV) | (′) | (1035 erg s−1) | (′) | (4 GeV) | (10 GeV) | |||||
| N 44 | > 4;10 | – | 4.3 | 0.90 | 4.8 | 3.3 | 3.7 | 26/48.1 | 13/28.7 | |
| N 132D | > 4;10 | CC | 2.1 | 315.04 | 6.6 | 4.6 | 1.8 | 27/55.6 | 21/57.6 | 4FGL |
| N 49B | > 4( * );10 | CC | 2.8 | 38.03 | ( * )5.6 | ( * )3.9 | 3.4 | ( * )23/46.3 | 6/20.0 | Nf |
| N 49 | > 4( * );10 | CC-SGR | 1.4 | 64.37 | ( * )5.6 | ( * )3.9 | 3.5 | ( * )23/46.3 | 9/18.4 | Nf |
| B0528−692 | > 10 | 4.5 | 1.99 | 4.4 | 3.5 | 4.1 | 24/55.7 | 24/58.8 | ||
| N 63A | > 4;10 | CC | 1.4 | 185.68 | 6.5 | 4.1 | 0.4 | 33/92.9 | 15/53.7 | 4FGL |
| N 157B | > 4;10 | CC-PWN | 2.0 | 15.00 | 18.8 | 11.6 | 1.6 | 146/441.5 | 155/577.4 | Nf30D 4FGL |
| B0540−693 | > 10 | CC-PSR | 1.2 | 87.35 | 8.7 | 4.8 | 5.3 | 22/61.8 | 8/35.4 | Nf30D 4FGL |
| N 186D | > 4;6 | 1.9 | 1.09 | – | 3.7 | 9/17.1 | 7/19.0 |
Notes. ( * ): Unresolved cluster at energies lower than 10 GeV. D: SNR diameter. Δ : Angular separation. LX: X-ray luminosity in the band 0.3–8 keV from the Maggi et al. (2016) catalog. Scls: Significance of the DBSCAN clusters at energies higher than 4 and 10 GeV. N/M: Number of photons in the clusters and the corresponding magnitudes from MST search.
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