The soft gamma repeater (SGR) 1900+14 emitted the giant flare on 27 August 1998. Most gamma-ray detectors saturated during the initial spike of the giant flare because of the intense flux. However the plasma particle detector onboard GEOTAIL observed the first 300 ms time profile with a time resolution of 5.577 ms and the initial spike of the giant flare was first resolved. The time profile shows some similarities to that of the SGR 1806-20 giant flare in 2004: the clear exponential decay and the small hump in the decay phase around 300 or 400 ms
We report the detection of large flux changes in the persistent X-ray flux of SGR 1900+14 during its...
Diffuse radio emission was detected around the soft gamma-ray repeater SGR 1806-20 after its 2004 po...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...
We report on the results of a ~30 ks Chandra pointing of the soft gamma-ray repeater SGR 1806-20, th...
The Soft Gamma Repeater SGR 1900+14 entered a remarkable phase of activity during the summer of 1998...
The giant flare of December 27, 2004 from SGR 1806-20 represents one of the most extraordinary event...
We analyze the data obtained when the Konus-Wind gamma-ray spectrometer detected a giant flare in SG...
The multi-wavelength observations of the 2004 December~27 Giant Flare (GF) from SGR 1806-20 and its ...
Electronic version of an article published as Modern Physics Letters A 21 (29) pp.2171-2188 10.1142/...
Japanese magnetospheric explorer GEOTAIL recorded a detailed light curve during the initial 600 msec...
SGR 180620 has been observed for more than 2 years with the INTEGRAL satellite. In this period the s...
The giant flare of 1998 August 27 from SGR 1900+14 was extraordinary in many ways: it was the most i...
We report on the results of an ~30 ks Chandra pointing of the soft gamma-ray repeater SGR 1806-20, t...
A giant flare from the Soft Gamma-ray Repeater SGR 1806-20 has been detected by several satellites o...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...
We report the detection of large flux changes in the persistent X-ray flux of SGR 1900+14 during its...
Diffuse radio emission was detected around the soft gamma-ray repeater SGR 1806-20 after its 2004 po...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...
We report on the results of a ~30 ks Chandra pointing of the soft gamma-ray repeater SGR 1806-20, th...
The Soft Gamma Repeater SGR 1900+14 entered a remarkable phase of activity during the summer of 1998...
The giant flare of December 27, 2004 from SGR 1806-20 represents one of the most extraordinary event...
We analyze the data obtained when the Konus-Wind gamma-ray spectrometer detected a giant flare in SG...
The multi-wavelength observations of the 2004 December~27 Giant Flare (GF) from SGR 1806-20 and its ...
Electronic version of an article published as Modern Physics Letters A 21 (29) pp.2171-2188 10.1142/...
Japanese magnetospheric explorer GEOTAIL recorded a detailed light curve during the initial 600 msec...
SGR 180620 has been observed for more than 2 years with the INTEGRAL satellite. In this period the s...
The giant flare of 1998 August 27 from SGR 1900+14 was extraordinary in many ways: it was the most i...
We report on the results of an ~30 ks Chandra pointing of the soft gamma-ray repeater SGR 1806-20, t...
A giant flare from the Soft Gamma-ray Repeater SGR 1806-20 has been detected by several satellites o...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...
We report the detection of large flux changes in the persistent X-ray flux of SGR 1900+14 during its...
Diffuse radio emission was detected around the soft gamma-ray repeater SGR 1806-20 after its 2004 po...
In December 2004, the soft gamma-ray repeater SGR 1806-20 emitted the most powerful giant flare ever...