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Table 3

Spectral fits to XMM-Newton pointed observations of XMMSL1 J0619-65.

Power-lawa Distant reflectionb zxipcfc Ionised reflectiond C/d.o.f.e
Γ Norm Norm N H xi cf xi Norm
keV-1 cm-2 s-1 keV-1 cm-2 s-1 1022 cm-2 log % log cm-2 s-1

XMM-Newton observation 1 - 2012-12-15

1.96 ± 0.02 3612/3230
1.98 ± 0.02 3573/3229
36 ± 6 3472/3226
1.92 ± 0.02 3471/3227

XMM-Newton observation 2 - 2013-04-24

1.81 ± 0.03 3072/3230
1.82 ± 0.03 3064/3229
1.76 ± + 0.04 3040/3226
1.79 ± 0.03 3055/3227

Joint fits to the XMM-Newton observations of 2012-12-15 and 2013-04-24f

6621/6457
43 ± 11
70 ± 2 6575/6455
6528/6454
1.87 ± 0.03
10g 6557/6455

Notes. All fits include absorption by the Galactic column (model TBABS, NH = 4.4 × 1020 cm-2). Errors are 90% confidence.

(a)

Continuum power law with photon index and normalisation;

(b)

reflection from distant matter with normalisation at 1 keV (pexmon; Nandra et al. 2007, with inclination fixed at 45°);

(c)

ionised absorption with equivalent column density, ionisation state and covering fraction;

(d)

ionised reflection (reflionx; Ross & Fabian 2005) with ionisation state and normalisation, convolved with a relativistic blurring model (kdblur; Laor 1991; Fabian et al. 2002), with fixed emissivity index = 3; inner radius = 4.5 GM/c2; outer radius = 100 GM/c2 and inclination = 45°;

(e)

C-statistic / number of degrees of freedom;

(f)

simultaneous fits to both XMM-Newton observations; for these, the first line of each model gives the tied parameters, the second line gives the free values for the 2012-12-15 observation and the third line the free values for the 2013-04-24 observation;

(g)

the parameter is unconstrained.

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