SGR-like flaring activity of the anomalous X-ray pulsar 1E 1547.0-5408

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Table 1:

Comparison of peak fluxes and luminosities of the AXP bursts.
Name	F	L	Reference
	[10^-8 erg cm^-2s^-1]	[erg s^-1]
4U 0142+61	$0.3\div 4$ (2-30 keV)	$\le$ $1.7\times 10^{40}$	1
1E 1048-59	$0.5\div 1.1$ (2-40 keV)	$\le$ $1.6\times 10^{37}$	2
1E 1547.0-5408	> $3\times 10^4$ (>80 keV)	> $2.7\times 10^{42}$	this work
CXOU J1647-45	$\simeq$ 1 (15-150 keV)	$\le$ $1.7\times 10^{37}$	4
XTE J1810-197	$0.07\div 10$ (2-30 keV)	$\le$ 10³⁸	5
1E 2259+586	$0.1\div 40$ (2-60 keV)	$\le$ $2.5 \times 10^{39}$	6

References. (1) Gavriil et al. (2008); (2) Gavriil et al. (2002); (3) this work; (4) Israel et al. (2007); (5) Woods et al. (2005); (6) Kaspi et al. (2003); Gavriil et al. (2004).

Source LaTeX | All tables | In the text

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