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Table 4

Best fit parameters of the MCD plus black body model for the XMM-Newton observations.

Source nH k T in R in k T bb R bb R sph a red. χ2/d.o.f.

[× 1021 cm2] K [km] K km km

Ho II X-1 0.40b 0.57 724 1.26 93.5 974 1.25/137
Ho IX X-1 0.33 0.91 198 1.95 59.2 1120 1.06/156
IC 342 X-1 7.42 0.61 ± 0.05 302 1.66 72.8 304 1.05/101
M33 X-8 0.82 0.70 202 1.11 62.1 155 1.01/121
M81 X-6 1.61 1.03 155 1.51 38.2 346 1.13/124
M83 ULX 0.39b 0.38 482 0.83 88.3 87.2 0.95/44
NGC 55 ULX 2.16 0.33 986 0.65 128 153 1.11/89
NGC 253 ULX2 2.35 0.95 121 1.39 51.8 258 1.05/120
NGC 253 XMM2 1.09 0.65 218 1.17 54.2 142 1.14/108
NGC 1313 X-1 1.83 0.44 778 1.39 52.8 730 1.09/113
NGC 1313 X-2 1.70 ± 0.11 0.86 261 1.66 54.6 700 1.01/144
NGC 4190 ULX1 0.56 0.87 256 1.51 85.0 505 1.06/112
NGC 4559 X-1 0.15b 0.43 1133 1.04 169 626 1.07/84
NGC 4736 ULX1 0.86 0.61 269 0.99 ± 0.06 76.6 272 1.12/68
NGC 4861 ULX 1.15 0.33 2398 0.93 205 176 1.10/22
NGC 5204 X-1 0.14b 0.43 1262 0.99 152 681 1.15/65
NGC 5907 ULX 6.04 0.74 ± 0.11 608 1.38 224 6740 1.09/83
NGC 7793 P13 0.66 ± 0.14 0.63 ± 0.04 251 1.70 ± 0.05 59.7 483 1.10/141

Notes. All errors are in the 1σ confidence range.

(a)

Spherisation radius (e.g. King & Lasota 2016): Rsph = 27/4Rg, where Rg = GM/c2 and = /Edd.

(b)

Parameter frozen at total galactic H I column density (Dickey & Lockman 1990).

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