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Table 3.
Results from fitting the XMM-Newton EPIC-pn data with the four phase-resolved absorbed magnetar emission models.
| Model name | χ2/D.o.F. | norm | χ | ξ | Δϕ | β | nH | offset |
|---|---|---|---|---|---|---|---|---|
| [10−9] | [°] | [°] | [rad] | [c] | [1022cm−2] | |||
| Blackbody | 3372.5/703 | 12.6 | 0.1 | 0.1 | 0.40 | 0.47 | 0.610 | 0.864 |
| Blackbody ( † ) | 3419.4/703 | 12.1 | 15 | 60 | 0.30 | 0.40 | 0.556 | 0.860 |
| Magnetized atmosphere | 37432.5/703 | 6.14 | 15.0 | 0.1 | 0.30 | 0.20 | 0. | 0.856 |
| Free-ions cond. surf. | 3728.9/703 | 9.16 | 0.1 | 87 | 0.30 | 0.39 | 0.335 | 0.864 |
| Fixed-ions cond. surf. | 3103.9/703 | 8.74 | 15 | 60 | 0.50 | 0.35 | 0.513 | 0.858 |
Notes. ( † )Fit with χ and ξ tied to the best-fit values of the fixed-ions condensed surface model.
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