Table 2.
New SNRs detected at energies higher than 4 GeV.
| SNR | l | b | TYPE | D | LX | Scls4 | Δ | MST | Notes |
|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (′) | (′) | (N/M) | |||||
| B0453−685 | 279.793 | −35.765 | CC | 2.0 | 13.85 | 3.7 | 2.0 | 10/18.3 | |
| B0532−675 | 277.638 | −32.346 | 4.7 | 2.48 | 3.1 | 5.8 | 7/23.5 | e | |
| [HP99]1139 | 281.589 | −34.229 | 4.4 | 1.44 | 3.1 | 6.4 | 13/24.7 | e | |
| N 103B | 279.624 | −34.401 | Ia | 0.5 | 51.70 | 3.3 | 2.7 | 10/19.8 | |
| B0519−690 | 279.617 | −33.323 | Ia | 0.6 | 34.94 | 4.2 | 5.0 | 13/26.6 | |
| DEM L316A/B | 279.984 | −30.859 | Ia/CC | 3.2 | 1.47/1.26 | 4.7 | 4.1 | 11/21.5 | Nf |
| DEM L241 | 277.712 | −32.150 | 5.3 | 3.84 | 5.2 | 1.2 | 35/79.6 | ||
Notes. Galactic coordinates and angular separations are from MST; the X-ray luminosity is in units of 1035 erg/s. e: MST analysis at energies > 6 GeV. Nf: M value obtained in a field with b > −31°. Scls: Significance of the DBSCAN clusters at energies higher than 4 GeV. N/M: Number of photons in the clusters and the corresponding magnitudes from the MST search.
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