Pulsating ultraluminous X-ray sources: Modeling the thermal emission and polarization properties

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Table 4.

Observed pulsed fractions of NGC 7793 P13 for the two XMM-Newton observations against simulated ones both calculated in the energy bands 2–3 keV and 3–4 keV.

Obs. ID	Observed PFs (%)		Simulated PFs (%)

	2–3 (keV)	3–4 (keV)	2–3 (keV)	3–4 (keV)
0693760401	$23_{19}^{26}$ $23^{26}_{19}$	$32_{28}^{37}$ $32^{37}_{28}$	24.3 ^(a)	29.8 ^(b)
0748390901	$22_{20}^{25}$ $22^{25}_{20}$	$29_{26}^{32}$ $29^{32}_{26}$	23.7 ^(a)	29.9 ^(b)

Notes.

^(a)

Geometry of view with χ = 40°.

^(b)

Geometry of view with χ = 60°.

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