[著者版]Spectral and timing studies of Suzaku ToO observations of two SGRs, 1900+14 and 1806-20, are presented. The X-ray quiescent emission spectra were well fitted by a two blackbody function, or a blackbody plus a power-law model. The non-thermal hard component discovered by INTEGRAL was detected by PIN diodes and its spectrum was reproduced by the power-law model reported by INTEGRAL. The XIS detected a periodicity of P = 5.1998 +/- 0.0002s for SGR 1900+14 and P = 7.6022 +/- 0.0007s for SGR 1806-20. The pulsed fraction was related to the burst activity for SGR 1900+14
We present the first dedicated X-ray study of the supernova remnant (SNR) G32.8-0.1 (Kes 78) with Su...
50 pages, 14 figures, accepted for publication in PASJInternational audienceTemporal and spectral st...
We present a systematic analysis of all the BeppoSAX data of the soft gamma-ray repeater SGR 1900+14...
Spectral and timing studies of Suzaku ToO observations of two SGRs, 1900+14 and 1806-20, are present...
We observed the soft gamma repeater SGR 0501+4516 with Suzaku for ~51 ks on 2008 August 26-27, about...
We present the first Suzaku observation of the new Soft Gamma Repeater, SGR 0501+4516, performed on ...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...
We report on the timing and spectral analysis of two Suzaku observations with different flux levels ...
We analyzed temporal and spectral properties, focusing on the short bursts, for three anomalous X-ra...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...
The low energy (<10 keV) X-ray emission of the Soft Gamma-ray Repeater SGR1806-20 has been studied b...
The low-energy (<10 keV) X-ray emission of the soft gamma repeater SGR 1806-20 has been studied by m...
A ~50 ks XMM-Newton observation of SGR 1900+14 has been carried out in 2005 September, after almost ...
We present a systematic analysis of all the BeppoSAX data of SGR1900+14. The observations spanning f...
We present a detailed analysis of a 3.5 s long burst from SGR 1900+14 that occurred on 2001 July 2. ...
We present the first dedicated X-ray study of the supernova remnant (SNR) G32.8-0.1 (Kes 78) with Su...
50 pages, 14 figures, accepted for publication in PASJInternational audienceTemporal and spectral st...
We present a systematic analysis of all the BeppoSAX data of the soft gamma-ray repeater SGR 1900+14...
Spectral and timing studies of Suzaku ToO observations of two SGRs, 1900+14 and 1806-20, are present...
We observed the soft gamma repeater SGR 0501+4516 with Suzaku for ~51 ks on 2008 August 26-27, about...
We present the first Suzaku observation of the new Soft Gamma Repeater, SGR 0501+4516, performed on ...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...
We report on the timing and spectral analysis of two Suzaku observations with different flux levels ...
We analyzed temporal and spectral properties, focusing on the short bursts, for three anomalous X-ra...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...
The low energy (<10 keV) X-ray emission of the Soft Gamma-ray Repeater SGR1806-20 has been studied b...
The low-energy (<10 keV) X-ray emission of the soft gamma repeater SGR 1806-20 has been studied by m...
A ~50 ks XMM-Newton observation of SGR 1900+14 has been carried out in 2005 September, after almost ...
We present a systematic analysis of all the BeppoSAX data of SGR1900+14. The observations spanning f...
We present a detailed analysis of a 3.5 s long burst from SGR 1900+14 that occurred on 2001 July 2. ...
We present the first dedicated X-ray study of the supernova remnant (SNR) G32.8-0.1 (Kes 78) with Su...
50 pages, 14 figures, accepted for publication in PASJInternational audienceTemporal and spectral st...
We present a systematic analysis of all the BeppoSAX data of the soft gamma-ray repeater SGR 1900+14...