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” | |||||
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XMM | Suzaku | XMM | Suzaku | XMM | Suzaku | XMM | Suzaku | |||
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local absorption | nH,fully [1022 cm-2] |
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0.93 ± 0.02 | 0.92 ± 0.02 | 0.95 ± 0.02 | 0.98 ± 0.02 | ||||
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... | nH,part [1022 cm-2] | ... |
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8.2 ± 1.5 | |||||
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... | cov. fraction [%] | ... |
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6 ± 3 | 50 ± 3 | 5 ± 3 |
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10 ± 6 | ||
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power law | Γ |
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1.66 ± 0.09 | 1.72 ± 0.02 |
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1.83 ± 0.06 | ||
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reflection | R | ... | ... | 0.48 ± 0.05 | 2 ± 1 | |||||
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... | Efold | ... | ... | 100 (f) | 200 ± 100 | |||||
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... | i [deg] | ... | ... | 45 (f) | 85-6 | |||||
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... | Ndir [10-3] |
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10.9 ± 0.2 | 7.1 ± 0.4 | 11.0 ± 0.3 |
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11.2 ± 0.2 | 7.5 ± 0.5 | 12.2 ± 0.6 | |
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... | Nabs [10-3] | ... | 6 ± 2 |
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7.6 ± 0.3 | 0.6 ± 0.4 | 5 ± 2 | 1.4 ± 0.8 | ||
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Gaussian line | Erest [keV] |
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6.40 ± 0.01 |
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6.40 ± 0.01 | ... | ... | |||
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... | σ [keV] |
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0.08 ± 0.02 | ... | ... | |||
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... | Nline [10-5] | 10 ± 3 |
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9 ± 3 |
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... | ... | |||
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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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