Hard X-ray timing and spectral characteristics of the energetic pulsar PSR J0205+6449 in supernova remnant 3C 58 - An RXTE PCA/HEXTE and XMM-Newton view on the 0.5–250 keV band

L. Kuiper; W. Hermsen; J. O. Urama; P. R. den Hartog; A. G. Lyne; B. W. Stappers

doi:10.1051/0004-6361/200913851

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Volume 515 (June 2010)

A&A, 515 (2010) A34

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Table 4:

Best fit values for the photon flux spectra of the total pulsed emission (TP), the first (P1) and second (P2) pulse emissions of PSR J0205+6449 assuming a power-law model of the form $F_{\gamma }= K\cdot (E_{\gamma }/E_0)^{-\Gamma }$ .
Parameter	TP	P1	P2
PCA (2.5-54.0 keV)
K (10^-6 ph/cm² s keV)	$2.93 \pm 0.05$	$2.03 \pm 0.03$	$0.90 \pm 0.04$
$\Gamma$	$1.06 \pm 0.03$	$1.04 \pm 0.03$	$1.10 \pm 0.08$
E₀ (keV)	8.34	8.34	8.34
F_2-30 (10^-13 erg/cm² s)	$10.67\pm 0.16$	$7.43\pm 0.11$	$3.24\pm 0.13$
XMM/PCA/HEXTE (0.56-267.5 keV)
K (10^-6 ph/cm² s keV)	$2.85 \pm 0.04$
$\Gamma$	$1.03 \pm 0.02$
E₀ (keV)	8.49
F_0.5-150 (10^-12 erg/cm² s)	$5.48\pm 0.28$

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