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Table 1

Spectral analysis of 4U 1344-60 – the model parameters.

Model component Parameter Flat power-law model “Part. cov.” model Complex model “fix” Complex model “free”

XMM Suzaku XMM Suzaku XMM Suzaku XMM Suzaku

local absorption nH,fully [1022 cm-2 0.93 ± 0.02 0.92 ± 0.02 0.95 ± 0.02 0.98 ± 0.02

... nH,part [1022 cm-2 ... 8.2 ± 1.5

... cov. fraction [%] ... 6 ± 3 50 ± 3 5 ± 3 10 ± 6

power law Γ 1.66 ± 0.09 1.72 ± 0.02 1.83 ± 0.06

reflection R ... ... 0.48 ± 0.05 2 ± 1

... Efold ... ... 100 (f) 200 ± 100

... i [deg] ... ... 45 (f) 85-6

... Ndir [10-3 10.9 ± 0.2 7.1 ± 0.4 11.0 ± 0.3 11.2 ± 0.2 7.5 ± 0.5 12.2 ± 0.6

... Nabs [10-3 ... 6 ± 2 7.6 ± 0.3 0.6 ± 0.4 5 ± 2 1.4 ± 0.8

Gaussian line Erest [keV] 6.40 ± 0.01 6.40 ± 0.01 ... ...

... σ [keV] 0.08 ± 0.02 ... ...

... Nline  [10-5 10 ± 3 9 ± 3 ... ...

fit goodness C/ν 9543/9110 9484/9108 9477/9114 9460/9111

Notes. The common parameters for all the fits are the column density of the absorber due to interstellar matter in our Galaxy nH,ISM = 1.06 × 1022 cm-2 (Kalberla et al. 2005), and the cosmological redshift z = 0.012 ± 0.002 (Piconcelli et al. 2006). Solar abundances were assumed in the reflection models. The Ndir parameter is a normalisation factor of the direct component while Nabs corresponds to the component affected by the partially covering absorber. They belong to the power-law, or the reflection model by pexmon, respectively. The sign “(f)” means that the parameter was fixed to that value.

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