Table 3
Summary of the results for the data with the corresponding best fit model.
| SNR | Distance [kpc] | ψ (−5°) | Ratio: N/S | Image ref. | |||
|
|
|||||||
| Published | Model | Data | Model | Data | Model | ||
|
|
|||||||
| G001.9+00.3 | 8.5 |
|
–85 | –89 | 1.0 | 1.0 | 1 |
| G003.7–00.2 | unknown |
|
7 | 15 | 1.2 | 1.1 | 2 |
| G008.7–05.0 | unknown |
|
–35 | –35 | 1.0 | 1.1 | 3 |
| G016.2–02.7 | unknown |
|
–20 | –29 | 0.9 | 1.0 | 3 |
| G021.8–00.6 | 5.2–5.5 |
|
36 | 61 | 0.6 | 1.1 | 4 |
| G024.7–00.6 | unknown |
|
–87 | 61 | 2.0 | 1.1 | 4 |
| G028.6–00.1 | 6–8.5 |
|
63 | 79 | 0.8 | 0.9 | 4 |
| G036.6+02.6 | unknown |  [or  ] |
–24 | –35 | 1.4 | 1.7 | 3 |
| G046.8–00.3 | 4.3–8.6 |
|
46 | 50 | 1.3 | 0.9 | 4 |
| G054.4–00.3 | 3.3–9 |
|
47 | 50 | 2.0 | 0.9 | 5 |
| G065.1+00.6 | 9.0–9.6 |
|
40 | 42 | 0.7 | 0.9 | 5 |
| G093.3+06.9 | 1.7–2.7 |
|
6 | 11 | 0.8 | 0.6 | 6 |
| G116.9+00.2 | 1.6–3.5 |
|
–62 | –30 | 1.5 | 1.2 | 5 |
| G119.5+10.2 | 1.1–1.7 |
|
36 | 11 | 0.5 | 0.9 | 7 |
| G127.1+00.5 | 1.1–1.3 |
|
15 | 19 | 1.5 | 1.2 | 5 |
| G156.2+05.7 | 1.0–3.0 |  [or  ] |
–66 | –73 | 1.3 | 1.0 | 8 |
| G166.0+04.3 | 3–6 |  [or  ] |
0 | 3 | 1.8 | 0.8 | 5 |
| G182.4+04.3 | >3 |  [or  ] |
–17 | 3 | 0.5 | 0.7 | 5 |
| G296.5+10.0 | 1.3–3.9 |
|
81 | 80 | 1.1 | 1.1 | 9 |
| G302.3+00.7 | unknown |
|
45 | 50 | 1.2 | 1.0 | 9 |
| G315.1+02.7 | unknown |
|
65 | 67 | 1.1 | 1.0 | 10 |
| G317.3–00.2 | unknown |
|
–35 | –40 | 0.6 | 0.3 | 9 |
| G321.9–00.3 | unknown |  [or ] |
–35 | –50 | 1.3 | 1.1 | 9 |
| G327.4+01.0 | unknown |
|
–40 | –44 | 3.7 | 0.9 | 9 |
| G327.6+14.6 | 1.6–2.2 |
|
83 | 79 | 1.0 | 1.1 | 9 |
| G332.0+00.2 | >6.6 |
|
–10 | –11 | 0.9 | 0.3 | 9 |
| G332.4–00.4 | 3.4 |
|
11 | 15 | 0.9 | 1.1 | 9 |
| G338.1+00.4 | unknown |
|
–57 | –40 | 0.4 | 0.8 | 9 |
| G350.0–02.0 | unknown |
|
6 | 15 | 4.1 | 1.2 | 10 |
| G353.9–02.0 | unknown |
|
–33 | –25 | 0.8 | 1.0 | 3 |
| G354.8–00.8 | unknown |
|
–21 | –25 | 1.0 | 0.9 | 9 |
| G356.2+004.5 | unknown |
|
–34 | –40 | 1.0 | 0.9 | 3 |
| G359.1–00.5 | 8–10.5 |
|
–36 | –34 | 0.8 | 0.7 | 9 |
Reference. For the “Ratio” column, N/S refers to the ratio of the measurements of the north limb/south limb. (1) Reynolds et al. (2008); (2) very Large Array via NRAO Science Data Archive; (3) the NRAO VLA Sky Survey (NVSS, Condon et al. 1998); (4) MAGPIS: A Multi-Array Galactic Plane Imaging Survey (Helfand et al. 2006); (5) canadian Galactic Plane Survey, (CGPS, Taylor et al. 2003); (6) Landecker et al. (1999); (7) the Westerbork Northern Sky Survey (WENSS, Rengelink et al. 1997); (8) Urumqi 25 m telescope (Xu et al. 2007); (9) the Molonglo Observatory Synthesis Telescope (MOST) Supernova Remnant Catalogue, (Whiteoak & Green 1996); (10) the Parkes-MIT-NRAO surveys (Condon et al. 1993). Published distances are taken from SNRcat (Ferrand & Safi-Harb 2012) and references therein.
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