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 3:

X-ray pulse profile characterization of PSR J0205+6449 from a fit involving two asymmetric Lorentzians plus background.
Parameter	Value		$1\sigma$ -error
Pulse-1
$\Phi_1$ ^a	0.0831	$\pm$	0.0004
$\Gamma_{1l}$	0.0175	$\pm$	0.0009
$\Gamma_{1r}$	0.0252	$\pm$	0.0011
Pulse-2

$\Phi_2$	0.5709	$\pm$	0.0015
$\Gamma_{2l}$	0.0214	$\pm$	0.0036
$\Gamma_{2r}$	0.0502	$\pm$	0.0056
Derived quantities
$\Phi_2-\Phi_1$	0.488	$\pm$	0.002
N₁/N₂	3.72	$\pm$	0.23
I₁^b	0.688	$\pm$	0.011
I₂	0.312	$\pm$	0.014
R=I₁/I₂	2.2	$\pm$	0.1
$\Gamma_1=(\Gamma_{1l}+\Gamma_{1r})/2$	0.0214	$\pm$	0.0007
	1.41	$\pm$	0.05 ms
$\Gamma_2=(\Gamma_{2l}+\Gamma_{2r})/2$	0.0358	$\pm$	0.0034
	2.35	$\pm$	0.22 ms

Notes. ^(a) Statistical error only, the systematic error is of the order of 0.01 (see Livingstone et al. 2009). ^(b) Relative contribution of the integrated flux in pulse-1 to the total pulsed flux.

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