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Table 1
Assumed properties of the sample of supernova remnants where the errors on the distance are 1σ and are described in Appendix A.
| SNR | Known as | RA | Dec | Diameter (arcmin) | Distance (kpc) | NTGAS | NTGAS + APASS |
|
|
|||||||
| G065.3+ 05.7 | – | 19:33:00 | +31:10 | 310 × 240 | 0.77 ± 0.2 | 294 | 7 |
| G069.0+ 02.7 | CTB 80 | 19:53:20 | +32:55 | 80 | 1.5 ± 0.5 | 14 | 11 |
| G074.0−08.5 | Cygnus Loop | 20:51:00 | +30:40 | 230 × 160 |
|
115 | 76 |
| G089.0+ 04.7 | HB 21 | 20:45:00 | +50:35 | 120 × 90 | 1.7 ± 0.5 | 25 | 3 |
| G093.7−00.2 | CTB 104A, DA 551 | 21:29:20 | +50:50 | 80 | 1.5 ± 0.2 | 10 | 10 |
| G114.3+ 00.3 | – | 23:37:00 | +61:55 | 90 × 55 | 0.7 ± 0.35 | 19 | 17 |
| G119.5+ 10.2 | CTA 1 | 00:06:40 | +72:45 | 90 | 1.4 ± 0.3 | 8 | 7 |
| G160.9+ 02.6 | HB 9 | 05:01:00 | +46:40 | 140 × 120 | 0.8 ± 0.4 | 19 | 18 |
| G180.0−01.7 | S147 | 05:39:00 | +27:50 | 180 |
|
36 | 31 |
| G205.5+ 00.5 | Monoceros Loop | 06:39:00 | +06:30 | 220 | 1.2 ± 0.4 | 53 | 47 |
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