Table C.1.
Super-soft X-ray sources.
ID | Galaxy | RA | Dec | Counts0.3−2 | Bkg0.3−2 | Rate0.3−2 | NH | kTbb | ![]() |
---|---|---|---|---|---|---|---|---|---|
(10−4 cnt s−1) | (1021 cm−2) | (eV) | (1037 erg s−1) | ||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
1 | M 81 | 09 55 42.14 | +69 03 36.40 | 2565.0 ± 51.7 | 8.7 ± 0.9 | 145.30 ± 2.94 | 1.19 | 85![]() |
15.87![]() |
2 | M 81 | 09 56 8.98 | +69 01 6.79 | 360.0 ± 20.0 | 1.6 ± 0.5 | 20.37 ± 1.14 | 1.39 | 86![]() |
7.04![]() |
3 | NGC 3379 | 10 47 47.23 | +12 34 59.78 | 72.0 ± 9.5 | 0.5 ± 0.3 | 3.03 ± 0.40 | 0.26 | 100![]() |
3.68![]() |
4 | NGC 4278 | 12 19 56.67 | +29 16 31.08 | 20.0 ± 5.6 | 1.6 ± 0.5 | 0.42 ± 0.13 | 0.20 | 65![]() |
2.76![]() |
5 | NGC 4278 | 12 20 12.43 | +29 17 41.86 | 25.0 ± 6.1 | 1.3 ± 0.4 | 0.55 ± 0.14 | 0.20 | 72![]() |
2.26![]() |
6 | NGC 4697 | 12 48 34.55 | –5 47 49.34 | 36.0 ± 7.1 | 0.8 ± 0.3 | 2.29 ± 0.46 | 0.21 | 102![]() |
2.79![]() |
7 | NGC 4697 | 12 48 41.28 | –5 48 19.73 | 24.0 ± 6.0 | 0.2 ± 0.2 | 1.55 ± 0.39 | 0.21 | 70![]() |
2.41![]() |
8 | Cen A | 13 25 14.60 | –42 56 11.57 | 83.0 ± 10.2 | 19.3 ± 1.4 | 2.28 ± 0.37 | 0.24 | 79![]() |
2.60![]() |
9 | Cen A | 13 25 18.14 | –43 03 42.53 | 100.0 ± 11.0 | 27.8 ± 1.7 | 1.29 ± 0.20 | 0.24 | 73![]() |
2.06![]() |
10 | M 51 | 13 29 41.23 | +47 11 15.57 | 48.0 ± 8.0 | 16.1 ± 1.2 | 0.43 ± 0.11 | 0.92 | 33![]() |
1.27![]() |
11 | M 51 | 13 29 46.00 | +47 10 56.36 | 55.0 ± 8.5 | 9.5 ± 1.0 | 0.61 ± 0.11 | 0.69 | 67![]() |
0.96![]() |
12 | M 51 | 13 29 51.69 | +47 12 3.82 | 86.1 ± 10.3 | 56.9 ± 2.3 | 0.39 ± 0.14 | 3.93 | 62![]() |
0.29![]() |
13 | M 51 | 13 29 54.02 | +47 11 25.68 | 64.0 ± 9.0 | 15.4 ± 1.2 | 0.65 ± 0.12 | 2.89 | 40![]() |
0.57![]() |
14 | M 51 | 13 29 54.99 | +47 12 4.74 | 62.0 ± 8.9 | 16.0 ± 1.3 | 0.62 ± 0.12 | 2.92 | 76![]() |
0.53![]() |
15 | M 83 | 13 36 52.45 | –29 52 52.09 | 242.0 ± 16.6 | 113.3 ± 3.2 | 1.76 ± 0.23 | 5.40 | 53![]() |
0.42![]() |
16 | M 83 | 13 36 52.66 | –29 49 37.45 | 67.0 ± 9.2 | 9.1 ± 1.0 | 0.79 ± 0.13 | 1.32 | 35![]() |
0.87![]() |
17 | M 83 | 13 36 53.97 | –29 50 32.52 | 40.0 ± 7.4 | 14.3 ± 1.2 | 0.35 ± 0.10 | 3.60 | 33![]() |
0.19![]() |
18 | M 83 | 13 36 56.45 | –29 52 57.25 | 50.0 ± 8.1 | 21.3 ± 1.5 | 0.39 ± 0.11 | 5.00 | 26![]() |
0.20![]() |
19 | M 83 | 13 36 56.77 | –29 53 16.20 | 95.0 ± 10.8 | 22.5 ± 1.5 | 0.99 ± 0.15 | 3.39 | 46![]() |
0.35![]() |
20 | M 83 | 13 36 58.62 | –29 51 56.84 | 88.0 ± 10.4 | 49.2 ± 2.1 | 0.53 ± 0.15 | 10.41 | 74![]() |
0.11![]() |
21 | M 83 | 13 36 58.64 | –29 53 38.86 | 87.0 ± 10.4 | 30.6 ± 1.7 | 0.77 ± 0.14 | 1.82 | 30![]() |
0.69![]() |
22 | M 83 | 13 36 59.04 | –29 52 18.07 | 50.0 ± 8.1 | 22.5 ± 1.5 | 0.38 ± 0.11 | 11.69 | 71![]() |
0.09![]() |
23 | M 83 | 13 36 59.25 | –29 51 43.82 | 85.0 ± 10.3 | 49.4 ± 2.2 | 0.49 ± 0.14 | 9.95 | 69![]() |
0.11![]() |
24 | M 83 | 13 36 59.34 | –29 53 17.90 | 49.0 ± 8.1 | 19.1 ± 1.3 | 0.41 ± 0.11 | 2.50 | 65![]() |
0.12![]() |
25 | M 83 | 13 37 0.45 | –29 50 54.02 | 173.0 ± 14.2 | 9.1 ± 1.0 | 2.25 ± 0.19 | 4.05 | 28![]() |
1.13![]() |
26 | M 83 | 13 37 3.86 | –29 52 23.02 | 41.0 ± 7.5 | 10.8 ± 1.0 | 0.41 ± 0.10 | 4.36 | 42![]() |
0.18![]() |
27 | M 83 | 13 37 5.53 | –29 50 32.24 | 34.0 ± 6.9 | 6.0 ± 0.8 | 0.42 ± 0.10 | 3.01 | 42![]() |
0.21![]() |
28 | M 83 | 13 37 18.55 | –29 52 7.59 | 29.0 ± 6.5 | 10.6 ± 1.0 | 0.25 ± 0.09 | 1.57 | 71![]() |
0.12![]() |
29 | M 101 | 14 02 51.34 | +54 19 18.24 | 178.0 ± 14.4 | 14.7 ± 1.2 | 2.02 ± 0.18 | 1.50 | 85![]() |
0.91![]() |
30 | M 101 | 14 02 51.64 | +54 22 3.97 | 33.0 ± 6.8 | 10.5 ± 1.0 | 0.28 ± 0.08 | 1.17 | 70![]() |
0.13![]() |
31 | M 101 | 14 03 1.22 | +54 23 41.41 | 324.0 ± 19.0 | 13.3 ± 1.1 | 3.83 ± 0.23 | 1.13 | 66![]() |
1.85![]() |
32 | M 101 | 14 03 12.75 | +54 21 11.52 | 38.0 ± 7.2 | 13.1 ± 1.1 | 0.28 ± 0.08 | 1.99 | 73![]() |
0.10![]() |
33 | M 101 | 14 03 13.65 | +54 20 9.39 | 700.0 ± 27.5 | 10.9 ± 1.0 | 7.24 ± 0.29 | 1.57 | 53![]() |
3.17![]() |
34 | M 101 | 14 03 15.52 | +54 17 3.81 | 339.0 ± 19.4 | 30.7 ± 1.7 | 3.24 ± 0.20 | 2.52 | 104![]() |
1.24![]() |
35 | M 101 | 14 03 16.52 | +54 20 54.80 | 44.0 ± 7.7 | 12.5 ± 1.1 | 0.34 ± 0.08 | 1.85 | 66![]() |
0.16![]() |
36 | M 101 | 14 03 19.02 | +54 17 19.48 | 254.0 ± 17.0 | 33.5 ± 1.8 | 2.32 ± 0.18 | 1.40 | 61![]() |
1.32![]() |
37 | M 101 | 14 03 27.38 | +54 21 11.62 | 109.0 ± 11.5 | 24.4 ± 1.5 | 0.89 ± 0.12 | 1.67 | 27![]() |
0.83![]() |
38 | M 101 | 14 03 29.91 | +54 20 57.27 | 259.0 ± 17.1 | 16.7 ± 1.3 | 2.54 ± 0.18 | 1.81 | 64![]() |
1.15![]() |
39 | M 101 | 14 03 33.35 | +54 17 59.73 | 433.0 ± 21.8 | 22.2 ± 1.4 | 4.32 ± 0.23 | 2.24 | 60![]() |
2.62![]() |
Notes. Description of columns: (1) Source ID; (2) Galaxy name; (3) Right ascension (J2000); (4) Declination (J2000); (5) Counts in the source region in the 0.3−2 keV band and its 1σ error (68%); (6) Background counts in the source region in 0.3−2 keV band and its 1σ error; (7) Source count rate in 0.3−2 keV band; (8) Absorption column density in units of 1021 cm−2 obtained by combining CO 2−1 and 21 cm data as described in Sect. 5.1; (9) Best fit color temperature in units of eV; (10) Absorbed X-ray luminosity in the 0.3−2 keV band in units of 1037 erg s−1. Parameters given in Cols. (9) and (10) were obtained by approximating spectra with the black body model with absorption fixed at the value from Col. (8).
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