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Table C.1

Characteristics of nearby SNRs.

# SNR other name distance radio index Brightness age Pulsar
G+long+lat [kpc] [Jy] [kyr]

1 18.95−1.1 2.  ±  0.1 0.28 40 11.75  ±  0.85 ?
2 65.3 + 5.7 0.9  ±  0.1 0.58  ±  0.07 52 26  ±  1
3 65.7 + 1.2 DA 495 1.0  ±  0.4 0.45  ±  0.1 5 16.75  ±  3.25 unknown
4 69.0 + 2.7 CTB 80 2.0  ±  0.1 0.20  ±  0.10 60   ±  10 20  ±  1 J1952+3252
5 74.0−8.5 Cygnus Loop 0.54 0.4  ±  0.06 175  ±  30 10  ±  1
6 78.2 + 2.1 γ Cygni 1.5  ±  0.1 0.75  ±  0.03 275  ±  25 7  ±  1
7 82.2 + 5.3 W63 2.3  ±  1.0 0.36  ±  0.08 105  ±  10 20.1  ±  6.6
8 89.0 + 4.7 HB 21 1.7  ±  0.5 0.27  ±  0.07 200  ±  15 5.60  ±  0.28
9 93.7−0.2 CTB 104A or DA 551 1.5  ±  0.2 0.52  ±  0.12 42   ±  7 50  ±  20
10 114.3 + 0.3 0.7 0.49  ±  0.25 6.4  ±  1.4 7.7    ±  0.1
11 116.5 + 1.1 1.6 0.16  ±  0.11 10.9  ±  1.2 20  ±  5 B2334+61 ?
12 116.9 + 0.2 CTB 1 1.6 0.33  ±  0.13 6.4  ±  1.4 20  ±  5 B2334+61 ?
13 119.5 + 10.2 CTA 1 1.4  ±  0.3 0.57  ±  0.06 42.5  ±  2.5 10  ±  5 J0010+7309
14 127.1 + 0.5 R5 1. ± 0.1 0.43  ±  0.1 12  ±  1 25  ±  5
15 156.2 + 5.7 0.8  ±  0.5 2.0 4.2  ±  0.1 10  ±  1 B0450+55 ?
16 160.9 + 2.6 HB 9 0.8  ±  0.4 0.48  ±  0.03  ~75 5.5   ±  1.5 B0458+46
17 180.0−1.7 S147 1.2  ±  0.4 0.75 74  ±  12 600  ±  10 J0538+2817
Crab nebula
or 3C144 or SN1054
19 189.1 + 3.0 IC 443 1.5  ±  0.1 0.36  ±  0.04 160  ±  5 30 or 4
20 203.0 + 12.0 Monogem ring 0.288 86   ±  1 B0656+14
21 205.5 + 0.5 Monoceros Nebula 1.63  ±  0.25 0.66  ±  0.2 156.1  ±  19.9 29  ±  1
22 263.9−3.3 Vela(XYZ) 0.295  ±  0.075 variable 2,000  ±  700 11.2  ±  0.1 B0833-45
RX J0852.0-4622 or Vela Jr
or SN1300
24 276.5 + 19.0 Antlia 0.2  ±  0.14  ≥1000 B0950+08
25 315.1 + 2.7 1.7  ±  0.8 0.7 50  ±  10 J1423-56
26 330.0 + 15.0 Lupus Loop 1.2  ±  0.3 50  ±  10 B1507-44 ?
27 347.3−0.5 SN393 1. ±  0.3 4.9   

Notes. Spectral index and brightness are inferred from measurements made at 1 GHz. Uncertainties in bold are not taken from bibliographic references, but just correspond to a rough uncertainty in the last relevant digit; hence they can be underestimated. An age is flagged with a    for an historical remnant; in this case, the age uncertainty is set from the distance uncertainty. Note that these ages are the observed ages, which differ from the actual ages by d/c.

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