Table A.1: The basic quantities for 148 SNRs in nearby galaxies used in this paper for deriving of the updated ${\Sigma -D}$relations.

Galaxy
Name D S1.4 $\alpha$ $\Sigma_{\rm 1GHz}$
    (pc) (mJy)   ( ${\rm {W\over m^2Hz~sr}}$)

Normal galaxies
LMC B0450-709 89 758 0.36 4.2E-21
LMC B0453-685 36 299 0.38 1.0E-20
LMC B0454-665 15 133 0.49 2.7E-20
LMC B0455-687 53 283 0.45 4.6E-21
LMC B0500-702 31 407 0.73 2.2E-20
LMC B0506-680 14 320a 0.58 7.7E-20
LMC B0513-692 55 289a 0.45 4.3E-21
LMC B0519-697 28 1692 0.35 9.7E-20
LMC B0519-690 7.5 110D 0.47 9.1E-20
LMC B0520-694 32 120a 0.32 5.0E-21
LMC B0524-664 46 73a 0.33 1.5E-21
LMC B0525-660 29 1265 0.60 7.1E-20
LMC B0525-696 29 5600D 0.58 3.1E-19
LMC B0525-661 17 1595 0.51 2.6E-19
LMC B0527-658 60 176 0.32 2.1E-21
LMC B0528-692 38 138a 0.44 4.3E-21
LMC B0532-710 47 505a 0.31 1.0E-20
LMC B0534-699 30 107a 0.48 5.6E-21
LMC B0534-705 45 103a 0.44 2.3E-21
LMC BO535-660 5.3 1613 0.57 2.7E-18
LMC B0536-676 50 201a 0.38 3.6E-21
LMC B0536-706 39 62a 0.61 2.0E-21
LMC B0547-697 56 1987 0.61 3.1E-20
LMC B0548-704 27 73a 0.55 4.6E-21
LMC B0528-672 50 81a 0.79 1.7E-21
SMC B0045-734 28 423a 0.15 3.0E-20
SMC B0047-735 38 24a 0.79 1.2E-21
SMC B0050-728 95 245a 0.40 1.7E-21
SMC B0058-718 50 189a 0.42 4.7E-21
SMC B0101-724 25 106a 0.50 1.1E-20
SMC B0102-722 8.5 285a 0.73 2.8E-19
SMC B0103-726 57 88a 0.47 1.8E-21
M 31 DDB-7 18 2.3 0.36 5.7E-20
M 31 DDB-11 29 0.83 $\pm$ 0.13 0.5b 8.6E-21
M 31 DDB-13 22 0.18 $\pm$ 0.05 0.5b 3.3E-21
M 31 DDB-15 36 0.51 $\pm$ 0.07 0.5b 3.3E-21
M 31 DDB-16 22 2.29 $\pm$ 0.08 0.41 4.2E-20
M 31 DDB-17 29 0.47 $\pm$ 0.07 0.5b 4.8E-21
M 31 DDB-18 31 1.35 $\pm$ 0.05 0.5b 1.3E-20
M 31 DDB-19 34 2.60 $\pm$ 0.10 0.22 2.1E-20
M 31 K53 68 2.00 $\pm$ 0.20 0.5b 3.9E-21
M 31 K86 92 0.45 $\pm$ 0.05 0.5b 4.6E-22
M 31 K180 27 0.50 $\pm$ 0.10 0.5b 5.7E-21
M 31 K230A 49 0.85 $\pm$ 0.15 0.5b 3.1E-21
M 31 K268 8.7 0.14 $\pm$ 0.03 0.5b 1.6E-20
M 31 K310 61 0.10 $\pm$ 0.03 0.5b 2.4E-22
M 31 K327 13 1.55 $\pm$ 0.10 0.5b 7.8E-20
M 31 K490A 63 2.60 $\pm$ 0.30 0.5b 5.6E-21
M 31 K506A 34 1.30 $\pm$ 0.10 0.5b 9.9E-21
M 31 K548 33 0.65 $\pm$ 0.05 0.5b 7.1E-21
M 31 K566 5.9 0.16 $\pm$ 0.03 0.5b 4.2E-20
M 31 K567 63 1.30 $\pm$ 0.10 0.5b 2.9E-21
M 31 K574 26 0.36 $\pm$ 0.02 0.5b 5.7E-21
M 31 K583 31 0.73 $\pm$ 0.10 0.5b 6.7E-21
M 31 K594 25 2.00 $\pm$ 0.05 0.5b 2.9E-20
M 31 K638 49 0.35 $\pm$ 0.05 0.5b 1.5E-21
M 31 K640A 59 0.62 $\pm$ 0.03 0.5b 1.7E-21
M 31 K774 17 0.17 $\pm$ 0.03 0.5b 5.3E-21
M 31 K782 15 2.26 $\pm$ 0.08 0.5b 8.3E-20
M 31 K817 25 0.30 $\pm$ 0.03 0.5b 4.1E-21
M 31 K891 105 1.00 $\pm$ 0.20 0.5b 7.9E-22
M 31 K947 71 0.90 $\pm$ 0.30 0.5b 1.6E-21
M 33 GDK2 104 5.0 $\pm$ 0.7 0.5 $\pm$ 0.1 4.8E-021
M 33 GDK3 32 0.3 $\pm$ 0.1 0.4 $\pm$ 0.5 2.9E-021
M 33 GDK5 94 2.3 $\pm$ 0.6 0.5 $\pm$ 0.2 2.7E-021
M 33 GDK8 53 0.9 $\pm$ 0.2 0.5b 3.4E-021
M 33 GDK9 112 1.0 $\pm$ 0.2 0.6 $\pm$ 0.2 8.5E-022
M 33 GDK11 18 0.7 $\pm$ 0.2 0.5 $\pm$ 0.3 2.3E-020
M 33 GDK13 17 0.6 $\pm$ 0.2 0.5b 2.4E-020
M 33 GDK17 26 1.1 $\pm$ 0.2 0.8 $\pm$ 0.3 1.8E-020
M 33 GDK20 47 0.6 $\pm$ 0.1 0.3 $\pm$ 0.3 2.6E-021
M 33 GDK24 64 2.3 $\pm$ 0.2 0.5 $\pm$ 0.1 5.9E-021
M 33 GDK25 10 0.8 $\pm$ 0.2 0.7 $\pm$ 0.3 9.4E-020
M 33 GDK28 89 0.7 $\pm$ 0.3 0.5 $\pm$ 0.5 9.2E-022
M 33 GDK29 27 0.9 $\pm$ 0.2 0.7 $\pm$ 0.3 1.3E-020
M 33 GDK35 36 0.3 $\pm$ 0.1 0.5b 2.4E-021
M 33 GDK39 22 1.8 $\pm$ 0.2 0.5 $\pm$ 0.1 4.0E-020
M 33 GDK42 26 1.4 $\pm$ 0.2 0.9 $\pm$ 0.2 2.4E-020
M 33 GDK46 48 0.7 $\pm$ 0.2 0.5b 3.2E-021
M 33 GDK47 23 1.2 $\pm$ 0.1 0.8 $\pm$ 0.2 2.8E-020
M 33 GDK50 11 0.8 $\pm$ 0.2 0.2 $\pm$ 0.2 6.4E-020
M 33 GDK52 20 0.5 $\pm$ 0.1 0.9 $\pm$ 0.5 1.6E-020
M 33 GDK54 28 0.4 $\pm$ 0.2 0.5 $\pm$ 0.5 5.2E-021
M 33 GDK57 38 1.8 $\pm$ 0.1 0.8 $\pm$ 0.1 1.4E-020
M 33 GDK64 31 3.5 $\pm$ 0.2 0.7 $\pm$ 0.1 4.0E-020
M 33 GDK74 50 0.5 $\pm$ 0.1 1.1 $\pm$ 0.7 2.6E-021
M 33 GDK75 28

0.5 $\pm$ 0.1

0.8 $\pm$ 0.4 7.2E-021
M 33 GDK77 33 1.3 $\pm$ 0.3 0.8 $\pm$ 0.3 1.4E-020
M 33 GDK81 20 1.2 $\pm$ 0.1 0.6 $\pm$ 0.2 3.4E-020
M 33 GDK90 35 0.2 $\pm$ 0.1 0.5b 1.7E-021
M 33 GDK92 22 0.3 $\pm$ 0.1 0.2 $\pm$ 0.2 6.0E-021
M 33 GDK99 29 0.6 $\pm$ 0.2 0.7 $\pm$ 0.5 7.8E-021
M 33 GDK103 41 0.4 $\pm$ 0.1 0.0 $\pm$ 0.3 2.0E-021
M 33 GDK105 48 0.7 $\pm$ 0.1 0.8 $\pm$ 0.3 3.6E-021
M 33 GDK110 39 0.2 $\pm$ 0.1 0.5b 1.4E-021
M 33 GDK111 16 1.3 $\pm$ 0.1 0.9 $\pm$ 0.1 6.4E-020
M 33 GDK112 18 4.4 $\pm$ 0.2 0.7 $\pm$ 0.1 1.6E-019
M 33 GDK114 21 0.4 $\pm$ 0.1 0.9 $\pm$ 0.7 1.1E-020
M 33 GDK116 28 1.1 $\pm$ 0.1 1.0 $\pm$ 0.2 1.7E-020
M 33 GDK121 16 0.3 $\pm$ 0.1 0.5b 1.3E-020
M 33 GDK122 33 0.3 $\pm$ 0.1 0.5b 2.8E-021
M 33 GDK125 28 0.4 $\pm$ 0.1 0.0 $\pm$ 0.3 4.3E-021
M 33 GDK130 26 0.5 $\pm$ 0.1 0.2 $\pm$ 0.2 6.6E-021
M 33 GDK138 48 0.6 $\pm$ 0.2 0.8 $\pm$ 0.5 3.0E-021
M 33 GDK139 35 0.6 $\pm$ 0.1 0.5b 5.0E-021
M 33 GDK140 31 0.4 $\pm$ 0.1 0.5 $\pm$ 0.3 4.2E-021
M 33 GDK148 17 0.5 $\pm$ 0.1 1.1 $\pm$ 0.4 2.3E-020
M 33 GDK154 25 0.4 $\pm$ 0.1 0.4 $\pm$ 0.3 6.2E-021
M 33 GDK158 123 1.8 $\pm$ 0.2 0.4 $\pm$ 0.1 1.2E-021
M 33 GDK160 43 0.4 $\pm$ 0.1 0.5 $\pm$ 0.3 2.3E-021
M 33 GDK168 50 0.8 $\pm$ 0.1 0.4 $\pm$ 0.2 3.2E-021
M 33 GDK170 45 0.3 $\pm$ 0.1 0.9 $\pm$ 0.4 1.8E-021
M 33 GDK181 34 0.8 $\pm$ 0.1 0.1 $\pm$ 0.2 6.1E-021
IC 1613 S8 8.4 1.9 $\pm$ 0.1 0.57 $\pm$ 0.05 2.0E-19
NGC 300 S10 16 0.29 $\pm$ 0.07 0.6 $\pm$ 0.3 8.0E-20
NGC 300 S11 43 0.89 $\pm$ 0.15 0.7 $\pm$ 0.2 3.5E-20
NGC 300 S26 33 0.22 $\pm$ 0.07 >0.7 1.5E-20
NGC 6946 S9 19 0.41 $\pm$ 0.08 0.8 $\pm$ 0.2 5.36E-19
NGC 6946 S16 19 1.59 $\pm$ 0.05 0.5 $\pm$ 0.1 1.85E-18
NGC 7793 S11 44 0.45 $\pm$ 0.15 0.6 $\pm$ 0.5 4.25E-20
NGC 7793 S26 450 4.88 $\pm$ 0.47 0.9 $\pm$ 0.2 4.96E-21
Starburst galaxies  
M 82 39.1+57.4 0.90 7.0 0.50c 1.6E-15
M 82 39.4+56.1 3.23 3.5 0.58c 6.1E-17
M 82 39.6+53.4 2.65 2.3 0.45c 5.7E-17
M 82 40.6+56.1 3.02 3.9 0.72c 8.3E-17
M 82 40.7+55.1 1.93 12.8 0.58c 6.3E-16
M 82 41.3+59.6 1.02 5.2 0.52c 9.0E-16
M 82 42.7+55.7 4.30 4.8 0.71c 5.0E-17
M 82 42.8+61.3 1.97 2.9 0.63c 1.4E-16
M 82 43.2+58.4 1.05 10.1 0.66c 1.7E-15
M 82 43.3+59.2 0.60 23.5 0.68c 1.2E-14
M 82 44.3+59.3 1.96 4.4 0.64c 2.1E-16
M 82 44.5+58.2 2.25 3.0 0.50c 1.1E-16
M 82 45.2+61.3 1.12 15.6 0.67c 2.3E-15
M 82 45.3+65.2 2.05 4.4 0.82c 2.1E-16
M 82 45.4+67.4 2.23 4.0 0.67c 1.5E-16
M 82 45.8+65.3 2.13 3.2 0.46c 1.3E-16
M 82 45.9+63.9 2.22 3.7 0.41c 1.3E-16
M 82 46.5+63.9 1.39 5.4 0.74c 5.4E-16
M 82 46.7+67.0 2.95 3.4 0.76c 7.7E-17
M 82 41.9+58.0 0.52 120.4 0.75c 8.6E-14
M 82 44.0+59.6 0.79 46.7 0.48c 1.3E-14
NGC 1569 VLA-8 20 0.479 $\pm$ 0.032 0.24 $\pm$ 0.10 8.1E-20
NGC 1569 VLA-16 15 0.681 $\pm$ 0.046 0.27 $\pm$ 0.14 2.1E-19
NGC 1569 M-6 17 $1.89\pm 0.03$ $0.55\pm 0.02$ 5.0E-19
NGC 2146 37.6+24.2 8.6 6.1e 1.1 3.35E-16
NGC 2146 38.9+42.5 28 4.7e 1.1 2.35E-17
NGC 2146 41.4+15.0 8.6 0.5e 0.6 2.45E-17
Note:

a S20 has been extrapolated from the values listed for $\alpha$ and S36 by Filipovic et al. (1998b).

b No spectral index data available; a value of $\alpha$ = 0.5 is assumed.

c S20 has been extrapolated from the values listed for $\alpha$ by McDonald et al. (2002) and S3.6 by Huang et al. (1994).

D The flux densities are from the paper by Dickel & Milne (1995).

e S20 has been extrapolated from the values listed for $\alpha$ and S18 by Tarchi et al. (2000).

Radio observations: LMC & SMC - at 1400 and 1420 MHz, respectively (Filipovic et al. 1998b); M 31 - at 1465 MHz (Braun & Walterbos 1993); M 33 - 1420 MHz (Gordon et al. 1999); IC 1613 - at 1460 MHz (Lozinskaya et al. 1998); NGC 300 - at 1450 MHz (Pannuti et al. 2000); NGC 6946 - at 1450 MHz (Lacey et al. 1997); NGC 7793 - at 1470 MHz (Pannuti et al. 2002); M 82 - at 8400 MHz (Huang et al. 1994); NGC 1569 - at 1400 MHz (Greve et al. 2002); NGC 2146 - at 1600 MHz (Tarchi et al. 2000).


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